Gas conditions of a star-formation selected sample in the first billion years (2406.19439v1)

Abstract: We present Atacama Large Millimetre/submillimetre Array (ALMA) observations of the [O${\rm III}$] 88 $\mu$m emission of a sample of thirteen galaxies at $z$ = 6 to 7.6 selected as [C${\rm II}$]-emitting companion sources of quasars. To disentangle the origins of the luminous Oxygen line in the $z$ > 6 Universe, we looked at emission-line galaxies that are selected through an excellent star-formation tracer [C${\rm II}$] with star-formation rates between 9 and 162 M${\odot}$/yr. Direct observations reveal [O${\rm III}$] emission in just a single galaxy (L${\rm [O_{\rm III}]}$/L${\rm [C{\rm II}]}$ = 2.3), and a stacked image shows no [O${\rm III}$] detection, providing deep upper limits on the L${\rm [O_{\rm III}]}$/L${\rm [C{\rm II}]}$ ratios in the $z > 6$ Universe (L${\rm [O{\rm III}]}$/L${\rm [C{\rm II}]}$ < 1.2 at 3${\sigma}$). While the fidelity of this sample is high, no obvious optical/near-infrared counterpart is seen in the JWST imaging available for four galaxies. Additionally accounting for low-redshift CO emitters, line stacking shows that our sample-wide result remains robust: The enhanced L${\rm [O{\rm III}]}$/L${\rm [C{\rm II}]}$ reported in the first billion years of the Universe is likely due to the selection towards bright, blue Lyman-break galaxies with high surface star-formation rates or young stellar populations. The deep upper limit on the rest-frame 90 $\mu$m continuum emission (< 141 $\mu$Jy at 3${\sigma}$), implies a low average dust temperature (T${\rm dust}$ < 30K) and high dust mass (M${\rm dust}$ ~ 10$^8$ M$_{\odot}$). As more normal galaxies are explored in the early Universe, synergy between JWST and ALMA is fundamental to further investigate the ISM properties of the a broad range of samples of high-$z$ galaxies.