Boogaard, Leindert A.Leindert A.Boogaardvan der Werf, PaulPaulvan der WerfWeiss, AxelAxelWeissPopping, GergöGergöPoppingDECARLI, ROBERTOROBERTODECARLIWalter, FabianFabianWalterAravena, ManuelManuelAravenaBouwens, RychardRychardBouwensRiechers, DominikDominikRiechersGonzález-López, JorgeJorgeGonzález-LópezSmail, IanIanSmailCarilli, ChrisChrisCarilliKaasinen, MelanieMelanieKaasinenDaddi, EmanueleEmanueleDaddiCox, PierrePierreCoxDíaz-Santos, TanioTanioDíaz-SantosInami, HanaeHanaeInamiCortes, Paulo C.Paulo C.CortesWagg, JeffJeffWagg2021-09-012021-09-0120200004-637Xhttp://hdl.handle.net/20.500.12386/31001We 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 Very Large Array follow-up observations, we detect a total of 34 CO $J\to J-1$ transitions with J = 1 up to 8 (and an additional 21 upper limits, up to J = 10) and 6 $[{\rm{C}}\,{\rm\small{I}}]$ ${}^{3}{P}_{1}{\to }^{3}\,{P}_{0}$ and ${}^{3}{P}_{2}{\to }^{3}\,{P}_{1}$ transitions (and 12 upper limits). The CO(2-1) and CO(3-2)-selected galaxies, at $\langle z\rangle =1.2$ 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 ( ${L}_{\mathrm{IR}}$ -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 $\langle z\rangle =1.2$ . We use stacking and Large Velocity Gradient models to measure and predict the average CO ladders at z < 2 and z ≥ 2, 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 ≥ 2 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 (≥10<SUP>4</SUP> cm<SUP>-3</SUP>), consistent with the low-J CO excitation. Our results imply a decrease in the cosmic molecular gas mass density at z ≥ 2 compared to previous ASPECS measurements.STAMPAenArticle10.3847/1538-4357/abb82fhttps://iopscience.iop.org/article/10.3847/1538-4357/abb82f2020ApJ...902..109BFIS/05 - ASTRONOMIA E ASTROFISICAERC sectors::Physical Sciences and Engineering::PE9 Universe sciences: astro-physics/chemistry/biology; solar systems; stellar, galactic and extragalactic astronomy, planetary systems, cosmology, space science, instrumentation