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Cosmicflows-3 (1605.01765v1)

Published 5 May 2016 in astro-ph.CO and astro-ph.GA

Abstract: The Cosmicflows database of galaxy distances that in the 2nd edition contained 8,188 entries is now expanded to 17,669 entries. The major additions are 2,257 distances that we have derived from the correlation between galaxy rotation and luminosity with photometry at 3.6 microns obtained with Spitzer Space Telescope and 8,885 distances based on the Fundamental Plane methodology from the 6dFGS collaboration. There are minor augmentations to the Tip of the Red Giant Branch and Type Ia supernova compilations. A zero point calibration of the supernova luminosities give a value for the Hubble Constant of 76.2 +-3.4(r) +-2.7(s) km/s/Mpc. Alternatively, a restriction on the peculiar velocity monopole term representing global infall/outflow implies H_0 = 75 +-2 km/s/Mpc.

Citations (254)

Summary

  • The paper significantly expands the cosmic distance database, increasing galaxy entries to 17,669 by integrating Spitzer photometry and 6dFGS Fundamental Plane data.
  • The study refines calibration techniques using Cepheid and TRGB methods, yielding a Hubble Constant of 76.2 ± 3.4 ± 2.7 km s⁻¹ Mpc⁻¹ with enhanced dataset compatibility.
  • The enhanced dataset improves modeling of large-scale cosmic flows and peculiar velocities, laying the groundwork for future cosmological research including Cosmicflows-4.

Overview of the "Cosmicflows-3" Paper

The paper "Cosmicflows-3" by R. Brent Tully and his collaborators delineates an expansion of the previous Cosmicflows database, essential for understanding large-scale cosmic structures through galaxy distances. In its third edition, the database is expanded from its predecessor's 8,188 galaxy distance entries to a comprehensive 17,669. This substantial increase prominently features data derived from two primary methodologies: the correlation between galaxy rotation and luminosity using photometry at 3.6 microns from the Spitzer Space Telescope, and the Fundamental Plane methodology as gathered from the Six Degree Field Galaxy Survey (6dFGS).

Spitzer Data and 3.6 Micron Calibration

The authors introduce a novel Spitzer photometry sample that significantly augments the Cosmicflows catalog. This sample incorporates galaxies with rotational and luminosity data (T-F relation), achieving a zero-point calibration of the T-F relation using distances from known Cepheid-calibrated distances or TRGB (Tip of the Red Giant Branch) methods. Particular attention is given to refining the photometric accuracy despite challenges in inclination measurement and possible systematic errors.

Six Degree Field Galaxy Survey (6dFGS) Contributions

The 6dFGS data contributes an additional 8,885 distance entries based on the Fundamental Plane analysis, adding robustness, particularly to the southern celestial hemisphere dataset. The paper details a methodology for harmonizing the distance scale from the 6dFGS data with existing Cosmicflows-2 datasets. Through detailed statistical comparison, the authors ensure compatibility between the new and existing data, effectively stitching together a more global understanding of the cosmic variance in galaxy distribution.

Enhanced Dataset and Calibration

In addition to the significant inclusion of Spitzer and 6dFGS datasets, refinements have been made in minor data subsets encompassing updated SNIa (Type Ia supernova) compilations and TRGB adjustments. The calibration process yields a recalibrated value for the Hubble Constant (H_0) of 76.2 ± 3.4 ± 2.7 km s-1 Mpc-1 when accounting for random and systematic errors, respectively.

Implications and Future Directions

The expanded Cosmicflows-3 database provides a rich resource for analyzing cosmic flows, peculiar velocities, and large-scale structure, building on a more homogenized and integrated global dataset. The high-resolution data obtained near the Local Sheet and out to deeper cosmic scales aids in modeling local bulk flows and constraining differing models of cosmic expansion. More importantly, it lays the groundwork for future observations and theoretical models that can probe finer scales and refine the cosmic distance ladder.

The paper innately addresses challenges such as systematic biases and the accurate characterization of peculiar velocities. It hints at the potential for Cosmicflows-4 to enhance coverage further, potentially leveraging forthcoming all-sky WISE data, solidifying these datasets as instrumental for cosmological investigations.

This enriched database serves as a cornerstone for continued exploration of cosmic expansion and the underlying structure of the universe, inviting theoretical and observational research to keep pace with these advancing frontiers in cosmic cartography.

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