The ALMA Spectroscopic Survey in the HUDF: CO Excitation and Atomic Carbon in Star-Forming Galaxies at $z=1-3$

TL;DR

This study uses ALMA and VLA observations to analyze CO excitation and atomic carbon in star-forming galaxies at redshifts 0.46 to 3.60, revealing insights into ISM conditions and their evolution with redshift.

Contribution

First comprehensive analysis of CO excitation and atomic carbon in a gas mass-selected galaxy sample across $z=0.46$ to $3.60$, highlighting redshift-dependent ISM properties.

Findings

Galaxies at $z extgreater=2$ show higher excitation than those at $z extless2$.

Average CO line ratios are $r_{21}=0.75 ext{ and } r_{31}=0.77$.

Atomic carbon abundance is similar to the Milky Way, indicating high-density ISM conditions.

Abstract

We investigate the CO excitation and interstellar medium (ISM) conditions in a cold gas mass-selected sample of 22 star-forming galaxies at $z=0.46-3.60$, observed as part of the ALMA Spectroscopic Survey in the Hubble Ultra Deep Field (ASPECS). Combined with VLA follow-up observations, we detect a total of 34 CO $J \rightarrow J-1$ transitions with $J=1$ up to $8$ (and an additional 21 upper limits, up to $J=10$) and six [C I] ${^3P}_1 \rightarrow {^3P}_0$ and ${^3P}_2 \rightarrow {^3P}_1$ transitions (and 12 upper limits). The CO(2-1) and CO(3-2)-selected galaxies, at $z=1.2$ and $2.5$, respectively, exhibit a range in excitation in their mid-$J=4,5$ and high-$J=7,8$ lines, on average lower than ($L_{\rm IR}$-brighter) BzK-color- and submillimeter-selected galaxies at similar redshifts. The former implies that a warm ISM component is not necessarily prevalent in gas mass-selected galaxies at $z=1.2$. We use stacking and Large Velocity Gradient models to measure and predict the average CO ladders at $z<2$ and $z\geq2$, finding $r_{21}=0.75 \pm 0.11$ and $r_{31}=0.77 \pm 0.14$, respectively. From the models, we infer that the galaxies at $z\geq2$ have intrinsically higher excitation than those at $z<2$. This fits a picture in which the global excitation is driven by an increase in the star formation rate surface density of galaxies with redshift. We derive a neutral atomic carbon abundance of $(1.9 \pm 0.4) \times 10^{-5}$, comparable to the Milky Way and main-sequence galaxies at similar redshifts, and fairly high densities ($\geq 10^4$ cm$^{-3}$), consistent with the low-$J$ CO excitation. Our results imply a decrease in the cosmic molecular gas mass density at $z\geq2$ compared to previous ASPECS measurements.