High Molecular Gas Masses in Absorption-selected Galaxies at z ≈ 2
Nissim Kanekar, J. X. Prochaska, Marcel Neeleman, L. Christensen, P. Møller, M. A. Zwaan, J. P. U. Fynbo, M. Dessauges‐Zavadsky
Abstract
Abstract We have used the Atacama Large Millimeter/submillimeter Array (ALMA) to carry out a search for CO (3−2) or (4−3) emission from the fields of 12 high-metallicity ([M/H] ≥ −0.72 dex) damped Ly α absorbers (DLAs) at z ≈ 1.7–2.6. We detected CO emission from galaxies in the fields of five DLAs (two of which have been reported earlier), obtaining high molecular gas masses, . The impact parameters of the CO emitters to the QSO sight line lie in the range b ≈ 5.6–100 kpc, with the three new CO detections having . The highest CO line luminosities and inferred molecular gas masses are associated with the highest-metallicity DLAs, with [M/H] ≳ −0.3 dex. The high inferred molecular gas masses may be explained by a combination of a stellar mass–metallicity relation and a high molecular gas-to-star mass ratio in high-redshift galaxies; the DLA galaxies identified by our CO searches have properties consistent with those of emission-selected samples. None of the DLA galaxies detected in CO emission were identified in earlier optical or near-IR searches and vice versa; DLA galaxies earlier identified in optical/near-IR searches were not detected in CO emission. The high ALMA CO and C[ ii ] 158 μ m detection rate in high- z , high-metallicity DLA galaxies has revolutionized the field, allowing the identification of dusty, massive galaxies associated with high- z DLAs. The H i -absorption criterion identifying DLAs selects the entire high- z galaxy population, including dusty and UV-bright galaxies, in a wide range of environments.