ACOSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time
arXiv:2201.12070 · doi:10.1051/0004-6361/202142299
Abstract
To constrain for the first time the mean mass and extent of the molecular gas of a mass-complete sample of M main-sequence (MS) galaxies at . We apply an innovative -based stacking analysis to a large set of archival Atacama Large Millimeter/submillimeter Array (ALMA) observations. This stacking analysis provides measurements of the mean mass and extent of the molecular gas of galaxy populations. The molecular gas mass of MS galaxies evolves with redshift and stellar mass. At all stellar masses, the molecular gas fraction decreases by a factor of 24 from to . At a given redshift, the molecular gas fraction of MS galaxies decreases with stellar mass, at roughly the same rate as their specific star formation rate decreases. The molecular gas depletion time of MS galaxies remains roughly constant at with a value of 300--500 Myr, but increases by a factor of 3 from to . This evolution of the molecular gas depletion time of MS galaxies can be predicted from the evolution of their molecular gas surface density and a seemingly universal MS-only relation with an inferred slope of 1.13, i.e., the so-called KS relation. The far-infrared size of MS galaxies shows no significant evolution with redshift or stellar mass, with a mean circularized half-light radius of 2.2 kpc. Finally, our mean molecular gas masses are lower than previous estimates, likely caused by the fact that literature studies were biased towards individually-detected MS galaxies with massive gas reservoirs. To first order, the molecular gas content of MS galaxies regulates their star formation across cosmic time, while variation of their star formation efficiency plays a secondary role. Despite a large evolution of their gas content and SFRs, MS galaxies evolved along a seemingly universal MS-only KS relation.
27 pages, 19 figures
References in corpus (80)
- Cosmic Star Formation History
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- The Cosmic Evolution Survey (COSMOS) -- Overview
- Star Formation in AEGIS Field Galaxies since z=1.1 : The Dominance of Gradually Declining Star Formation, and the Main Sequence of Star-Forming Galaxies
- Cold streams in early massive hot haloes as the main mode of galaxy formation
- A Highly Consistent Framework for the Evolution of the Star-Forming "Main Sequence" from z~0-6
- 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since
- A simple model to interpret the ultraviolet, optical and infrared emission from galaxies
- UV Luminosity Functions at redshifts z~4 to z~10: 10000 Galaxies from HST Legacy Fields
- Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
- The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
- Combined CO & Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star Formation Rate and Stellar Mass
- A Dust-Obscured Massive Maximum-Starburst Galaxy at a Redshift of 6.34
- The All-wavelength Extended Groth Strip International Survey (AEGIS) Data Sets
- xCOLD GASS: the complete IRAM-30m legacy survey of molecular gas for galaxy evolution studies
- The Cosmic Infrared Background Resolved by Spitzer. Contributions of Mid-Infrared Galaxies to the Far-Infrared Background
- An ALMA survey of Sub-millimeter Galaxies in the Extended Chandra Deep Field South: Physical properties derived from ultraviolet-to-radio modelling
- The Evolution of the Star-forming Interstellar Medium across Cosmic Time
- H-alpha Observations of a Large Sample of Galaxies at z~2: Implications for Star Formation in High Redshift Galaxies
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- Evidence for Mature Bulges and an Inside-out Quenching Phase 3 Billion Years After the Big Bang
- Evolution of the dust emission of massive galaxies up to z=4 and constraints on their dominant mode of star formation
- The XMM-Newton wide-field survey in the COSMOS field. The point-like X-ray source catalogue
- Molecular and atomic gas along and across the main sequence of star-forming galaxies
- Dust temperature and mid-to-total infrared color distributions for star-forming galaxies at 0<z<4
- The ALPINE-ALMA [CII] Survey: The nature, luminosity function and star formation history of dusty galaxies up to z~6
- The far-infrared/radio correlation and radio spectral index of galaxies in the SFR-M* plane up to z 2
- Star formation is boosted (and quenched) from the inside out: radial star formation profiles from MaNGA
- A Model for Star Formation, Gas Flows and Chemical Evolution in Galaxies at High Redshifts
- Quenched fractions in the IllustrisTNG simulations: the roles of AGN feedback, environment, and pre-processing
- Sub-kpc ALMA imaging of compact star-forming galaxies at z~2.5: revealing the formation of dense galactic cores in the progenitors of compact quiescent galaxies
- The Evolution of the Baryons Associated with Galaxies Averaged over Cosmic Time and Space
- A complete 12CO 2-1 map of M51 with HERA: I. Radial averages of CO, HI, and radio continuum
- Half-mass radii for ~7,000 galaxies at 1.0 < z < 2.5: most of the evolution in the mass-size relation is due to color gradients
- VLA and ALMA Imaging of Intense, Galaxy-Wide Star Formation in z ~ 2 Galaxies
- The VLA-COSMOS 3 GHz Large Project: Evolution of specific star formation rates out to
- Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): II. Cold Molecular Gas Evolution out to Redshift 6
- Revisiting the Integrated Star Formation Law. Paper I: Non-Starbursting Galaxies
- A Multiwavelength Consensus on the Main Sequence of Star-Forming Galaxies at z~2
- The ALPINE-ALMA [CII] survey: Dust attenuation properties and obscured star formation at z~4.4-5.8
- The ALPINE-ALMA [CII] survey: Molecular gas budget in the Early Universe as traced by [CII]
- Dust continuum emission as a tracer of gas mass in galaxies
- Gas Fraction and Depletion Time of Massive Star Forming Galaxies at z~3.2: No Change in Global Star Formation Process out to z>3
- A spatially resolved study of cold dust, molecular gas, HII regions, and stars in the submillimeter galaxy ALESS67.1
- Automated Mining of the ALMA Archive in the COSMOS Field (A3COSMOS): I. Robust ALMA Continuum Photometry Catalogs and Stellar Mass and Star Formation Properties for ~700 Galaxies at z=0.5-6
- Star formation scaling relations at ~100 pc from PHANGS: Impact of completeness and spatial scale
- Structural evolution in massive galaxies at z~2
- Evolution of cosmic star formation in the SCUBA-2 Cosmology Legacy Survey
- The ALMaQUEST Survey: V. The non-universality of kpc-scale star formation relations and the factors that drive them
- An ALMA survey of submillimetre galaxies in the COSMOS field: Physical properties derived from energy balance spectral energy distribution modelling
- The dust-continuum size of TNG50 galaxies at : a comparison with the distribution of stellar light, stars, dust and H
- The ALMA Spectroscopic Survey in the HUDF: The Cosmic Dust and Gas Mass Densities in Galaxies up to
- The Main Sequence at contains a sizable fraction of galaxies with compact star formation sizes: a new population of early post-starbursts?
- Revealing the Stellar Mass and Dust Distributions of Submillimeter Galaxies at Redshift 2
- The Molecular Gas Reservoirs of Galaxies: A comparison of CO(1-0) and dust-based molecular gas masses
- Central Star Formation in Pseudobulges and Classical Bulges
- The EDGE-CALIFA survey: The local and global relations between , and that regulate star-formation
- The EDGE-CALIFA survey: exploring the role of the molecular gas on the galaxy star formation quenching
- Scaling relations and baryonic cycling in local star-forming galaxies: II. Gas content and star-formation efficiency
- Stacking of large interferometric data sets in the image- and uv-domain -- a comparative study
- Radio continuum size evolution of star-forming galaxies over 0.35 < z < 2.25
- High gas fraction in a CO-selected main-sequence galaxy at
- The MUSE Hubble Ultra Deep Field Survey. XV. The mean rest-UV spectra of Ly-alpha emitters at z>3
- Connections between galaxy mergers and Starburst: evidence from local Universe
- An ALMA Survey of the SCUBA-2 Cosmology Legacy Survey UKIDSS/UDS Field: The Far-infrared/Radio correlation for High-redshift Dusty Star-forming Galaxies
- The UV Luminosity Function of Protocluster Galaxies at : the Bright-end Excess and the Enhanced Star Formation Rate Density
- S2COSMOS: Evolution of Gas Mass with Redshift Using Dust Emission
- Galaxy Lookback Evolution Models -- a Comparison with Magneticum Cosmological Simulations and Observations
- ALMA reveals the molecular gas properties of 5 star-forming galaxies across the main sequence at 3 < z < 3.5
- Estimating sizes of faint, distant galaxies in the submillimetre regime
- The VLA Frontier Field Survey: A Comparison of the Radio and UV/optical size of star-forming galaxies
- Evolution of the Gas Mass Fraction of Progenitors to Today's Massive Galaxies: ALMA Observations in the CANDELS GOODS-S Field
- New empirical constraints on the cosmological evolution of gas and stars in galaxies
- Enhancement of CO(3-2)/CO(1-0) Ratios and Star Formation Efficiencies in Supergiant HII Regions
- Unveiling Sizes of Compact AGN Hosts with ALMA
- A Universal Relation of Dust Obscuration Across Cosmic Time
- On the Kennicutt-Schmidt scaling law of submillimetre galaxies
- Radio emission from dust-obscured galaxies
- The dust and cold gas content of local star forming galaxies
- Properties of Compact Faint Radio Sources as a Function of Angular Size from Stacking
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- The merger-starburst connection across cosmic times
- The bending of the star-forming main sequence traces the cold- to hot-accretion transition mass over 0<z<4
- [CII] line intensity mapping the epoch of reionization with the Prime-Cam on FYST
- Formation of globular clusters in dwarf galaxies of the Local Group
- CO Emission, Molecular Gas, and Metallicity in Main-Sequence Star-Forming Galaxies at
- VINTERGATAN IV: Cosmic phases of star formation in Milky Way-like galaxies
- VLA Legacy Survey of Molecular Gas in Massive Star-forming Galaxies at High Redshift
- Modeling the kinematics of globular cluster systems
- CEERS: MIRI deciphers the spatial distribution of dust-obscured star formation in galaxies at
- Charting the main sequence of star-forming galaxies out to redshifts z<5.7
- Catalogue of model star clusters in the Milky Way and M31 galaxies
- A super-linear "radio-AGN main sequence'' links mean radio-AGN power and galaxy stellar mass since z3
- The Gas Mass Reservoir of Quiescent Galaxies at Cosmic Noon
- New constraints on the evolution of the MHI-M* scaling relation combining CHILES and MIGHTEE-HI data
- The Subtle Effects of Mergers on Star Formation in Nearby Galaxies
- Detailed Study of Stars and Gas in a z = 8.3 Massive Merger with Extreme Dust Conditions
- ACOSMOS: Measuring the cosmic dust-attenuated star formation rate density at
- Active galactic nuclei-heated dust revealed in "little red dots"
- Effects of secular growth and mergers on the evolution of metallicity gradients and azimuthal variations in a Milky Way-like galaxy
- PRIMER: JWST/MIRI reveals the evolution of star-forming structures in galaxies at z<2.5
- Galaxy Zoo JWST: Up to 75% of discs are featureless at
- Star formation across cosmic time
- Dust emission from the bulk of galaxies at the Epoch of Reionization
- Introducing cosmosTNG: simulating galaxy formation with constrained realizations of the COSMOS field
- ACOSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time
- The ALPINE-CRISTAL-JWST survey: spatially resolved star formation relations at
- Vz-GAL: Probing Cold Molecular Gas in Dusty Star-forming Galaxies at z=1-6
- Measuring the gas reservoirs in M M galaxies at
- Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8
- Investigating the role of turbulence in the interstellar medium in dusty star-forming galaxies using kpc-resolution ALMA dust and gas maps