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Reanalysis of the MACHO constraints on PBH in the light of Gaia DR3 data (2402.00212v2)

Published 31 Jan 2024 in astro-ph.GA, astro-ph.CO, and hep-ph

Abstract: The recent astrometric data of hundreds of millions of stars from Gaia DR3 has allowed a precise determination of the Milky Way rotation curve up to $28$~kpc. The data suggests a rapid decline in the density of dark matter beyond $19$~kpc. We fit the whole rotation curve with four components (gas, disk, bulge and halo) and compute the microlensing optical depth to the Large Magellanic Cloud. With this model of the galaxy we reanalyse the microlensing events of the MACHO and EROS-2 Collaborations. Using the published MACHO efficiency function for the duration of their survey, together with the rate of expected events according to the new density profile, we find that the Dark Matter halo could be composed up to $100\%$ of massive compact halo objects for any mass between $10{-4}$ to $100~M_\odot$, except a broad range around $0.01~M_\odot$, where it cannot be larger than $\sim20~\%$. For the EROS-2 survey, using a modified efficiency curve for consistency with the MACHO analysis, we also find compatibility with a 100\% MACHO halo, but with a tighter constraint around $0.001~M_\odot$ where the halo fraction cannot be larger than $\sim12~\%$. This result assumes that MACHOs all have the same mass. If these were distributed in an extended mass function like that of the Thermal History Model, the constraints are weakened, allowing $100\%$ of all DM in the form of Primordial Black Holes.

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References (26)
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[2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 García-Bellido, J., Linde, A.D., Wands, D.: Density perturbations and black hole formation in hybrid inflation. Phys. Rev. D 54, 6040 (1996) arXiv:astro-ph/9605094 Jedamzik [1997] Jedamzik, K.: Primordial black hole formation during the QCD epoch. Phys. Rev. D 55, 5871 (1997) arXiv:astro-ph/9605152 Paczynski [1986] Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jedamzik, K.: Primordial black hole formation during the QCD epoch. Phys. Rev. D 55, 5871 (1997) arXiv:astro-ph/9605152 Paczynski [1986] Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. 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[2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jedamzik, K.: Primordial black hole formation during the QCD epoch. Phys. Rev. D 55, 5871 (1997) arXiv:astro-ph/9605152 Paczynski [1986] Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. 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J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. 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[2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. 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JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  3. Jedamzik, K.: Primordial black hole formation during the QCD epoch. Phys. Rev. D 55, 5871 (1997) arXiv:astro-ph/9605152 Paczynski [1986] Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. 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[2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. 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[2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. 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[2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  4. Paczynski, B.: Gravitational microlensing by the galactic halo. Astrophys. J. 304, 1 (1986) Alcock et al. [1996] Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project first year LMC results: The Microlensing rate and the nature of the galactic dark halo. Astrophys. J. 461, 84 (1996) arXiv:astro-ph/9506113 Alcock et al. [2000] Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. 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[2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. 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Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
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Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. 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[2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. 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J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. 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JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  6. Alcock, C., et al.: The MACHO project: Microlensing results from 5.7 years of LMC observations. Astrophys. J. 542, 281 (2000) arXiv:astro-ph/0001272 Hawkins [2015] Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. 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Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. 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Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. 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[2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  7. Hawkins, M.R.S.: A new look at microlensing limits on dark matter in the Galactic halo. Astron. Astrophys. 575, 107 (2015) arXiv:1503.01935 Tisserand et al. [2007] Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Tisserand, P., et al.: Limits on the Macho Content of the Galactic Halo from the EROS-2 Survey of the Magellanic Clouds. Astron. Astrophys. 469, 387 (2007) arXiv:astro-ph/0607207 Wyrzykowski et al. [2011] Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wyrzykowski, L., et al.: The OGLE View of Microlensing towards the Magellanic Clouds. IV. OGLE-III SMC Data and Final Conclusions on MACHOs. Mon. Not. Roy. Astron. Soc. 416, 2949 (2011) arXiv:1106.2925 Clemens [1985] Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. 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Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. 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Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. 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J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Clemens, D.P.: Massachusetts-Stony Brook Galactic plane CO survey: the galactic disk rotation curve. Astrophys. J. 295, 422 (1985) Xue et al. [2008] Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Xue, X.X., et al.: The Milky Way’s Circular Velocity Curve to 60 kpc and an Estimate of the Dark Matter Halo Mass from Kinematics of ~2400 SDSS Blue Horizontal Branch Stars. Astrophys. J. 684, 1143 (2008) arXiv:0801.1232 Sofue [2013] Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. 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Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sofue, Y.: Rotation Curve and Mass Distribution in the Galactic Center — From Black Hole to Entire Galaxy —. Publ. Astron. Soc. Jap. 65, 118 (2013) arXiv:1307.8241 Bhattacharjee et al. [2014] Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. 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[2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bhattacharjee, P., Chaudhury, S., Kundu, S.: Rotation Curve of the Milky Way out to ∼similar-to\sim∼ 200 kpc. Astrophys. J. 785, 63 (2014) arXiv:1310.2659 Calcino et al. [2018] Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. 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J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. 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[2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. 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Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. 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[2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. 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[2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. 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  14. Calcino, J., García-Bellido, J., Davis, T.M.: Updating the MACHO fraction of the Milky Way dark halo with improved mass models. Mon. Not. Roy. Astron. Soc. 479(3), 2889 (2018) arXiv:1803.09205 Huang et al. [2016] Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. 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[2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  15. Huang, Y., et al.: The Milky Way’s rotation curve out to 100 kpc and its constraint on the Galactic mass distribution. Mon. Not. Roy. Astron. Soc. 463, 2623 (2016) arXiv:1604.01216 Ou et al. [2023] Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. 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J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. 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J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  16. Ou, X., Eilers, A.-C., Necib, L., Frebel, A.: The dark matter profile of the Milky Way inferred from its circular velocity curve (2023) arXiv:2303.12838 Jiao et al. [2023] Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Jiao, Y., Hammer, F., Wang, H., Wang, J., Amram, P., Chemin, L., Yang, Y.: Detection of the Keplerian decline in the Milky Way rotation curve. Astron. Astrophys. 678, 208 (2023) arXiv:2309.00048 Wang et al. [2023] Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
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[2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. 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[2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  18. Wang, H.-F., Chrobáková, Z., López-Corredoira, M., Sylos Labini, F.: Mapping the Milky Way Disk with Gaia DR3: 3D Extended Kinematic Maps and Rotation Curve to 30 kpc. Astrophys. J. 942, 12 (2023) Sylos Labini et al. [2023] Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Sylos Labini, F., Chrobáková, Z., Capuzzo-Dolcetta, R., López-Corredoira, M.: Mass Models of the Milky Way and Estimation of Its Mass from the Gaia DR3 Data Set. Astrophys. J. 945, 3 (2023) Vallenari et al. [2023] Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
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JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Vallenari, A., et al.: Gaia Data Release 3. Summary of the content and survey properties. Astron. Astrophys. 674, 1 (2023) arXiv:2208.00211 Bennett [2005] Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
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  21. Bennett, D.P.: Large Magellanic Cloud microlensing optical depth with imperfect event selection. Astrophys. J. 633, 906 (2005) arXiv:astro-ph/0502354 Alcock et al. [2001] Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  22. Alcock, C., et al.: The MACHO project Hubble Space Telescope follow-up: preliminary results on the location of the large magellanic cloud microlensing source stars. Astrophys. J. 552, 582 (2001) arXiv:astro-ph/0008282 Byrnes et al. [2018] Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  23. Byrnes, C.T., Hindmarsh, M., Young, S., Hawkins, M.R.S.: Primordial black holes with an accurate QCD equation of state. JCAP 08, 041 (2018) arXiv:1801.06138 Refsdal and Stabell [1991] Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  24. Refsdal, S., Stabell: Gravitational micro-lensing for large sources. Astron. Astrophys. 250, 62 (1991) Alcock et al. [2001] Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  25. Alcock, C., et al.: The MACHO project: microlensing detection efficiency. Astrophys. J. Suppl. 136, 439 (2001) arXiv:astro-ph/0003392 Carr et al. [2021] Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217 Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
  26. Carr, B., Clesse, S., García-Bellido, J., Kühnel, F.: Cosmic conundra explained by thermal history and primordial black holes. Phys. Dark Univ. 31, 100755 (2021) arXiv:1906.08217
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