Key points are not available for this paper at this time.
We present Atacama Large Millimetre/submillimetre Array (ALMA) observations of the O ₈₈₈ 88 m emission of a sample of thirteen galaxies at z = 6 to 7. 6 selected as C ₈₈-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 ₈₈ with star-formation rates between 9 and 162 M_/yr. Direct observations reveal O ₈₈₈ emission in just a single galaxy (L ₎_ ₈₈₈/L ₂_ ₈₈ = 2. 3), and a stacked image shows no O ₈₈₈ detection, providing deep upper limits on the L ₎_ ₈₈₈/L ₂_ ₈₈ ratios in the z > 6 Universe (L ₎_ ₈₈₈/L ₂_ ₈₈ < 1. 2 at 3). 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 ₎_ ₈₈₈/L ₂_ ₈₈ 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 m continuum emission (< 141 Jy at 3), implies a low average dust temperature (T ₃ₔₒₓ < 30K) and high dust mass (M ₃ₔₒₓ ~ 10⁸ M_). 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.
Bakx et al. (2024) studied this question.