The Nature of Hi-absorption-selected Galaxies at z ≈ 4

Abstract

Abstract We report a Karl G. Jansky Very Large Array (JVLA) search for redshifted CO(1–0) or CO(2–1) emission, and a Hubble Space Telescope Wide Field Camera 3 (HST-WFC3) search for rest-frame near-ultraviolet (NUV) stellar emission, from seven Hi-selected galaxies associated with high-metallicity ([M/H] ≥ −1.3) damped Lyα absorbers (DLAs) at z ≈ 4. The galaxies were earlier identified by Atacama Large Millimeter/submillimeter Array imaging of their [Cii] 158 μm emission. We also used the JVLA to search for CO(2–1) emission from the field of a low-metallicity ([M/H] = −2.47) DLA at z ≈ 4.8. No statistically significant CO emission is detected from any of the galaxies, yielding upper limits of M mol < (7.4–17.9) × 1010 × (α CO/4.36) M ⊙ on their molecular gas mass. We detect rest-frame NUV emission from four of the seven [Cii] 158 μm-emitting galaxies, the first detections of the stellar continuum from Hi-selected galaxies at z ≳ 4. The HST-WFC3 images yield typical sizes of the stellar continua of ≈2–4 kpc and inferred dust-unobscured star formation rates (SFRs) of ≈5.0–17.5 M ⊙ yr−1, consistent with, or slightly lower than, the total SFRs estimated from the far-infrared (FIR) luminosity. We further stacked the CO(2–1) emission signals of six [Cii] 158 μm-emitting galaxies in the image plane. Our non-detection of CO(2–1) emission in the stacked image yields the limit M mol < 4.1 × 1010 × (α CO/4.36) M ⊙ on the average molecular gas mass of the six galaxies. Our molecular gas mass estimates and NUV SFR estimates in Hi-selected galaxies at z ≈ 4 are consistent with those of main-sequence galaxies with similar [Cii] 158 μm and FIR luminosities at similar redshifts. However, the NUV emission in the Hi-selected galaxies appears more extended than that in main-sequence galaxies at similar redshifts.