The Gas Mass Reservoir of Quiescent Galaxies at Cosmic Noon

Abstract

We present a 1.1mm stacking analysis of moderately massive (log($M_{\ast }$/$M_{\odot }$) = 10.7 $\pm$ 0.2) quiescent galaxies (QGs) at $⟨z⟩\sim 1.5$, searching for cold dust continuum emission, an excellent tracer of dust and gas mass. Using both the recent GOODS-ALMA survey as well as the full suite of ALMA Band-6 ancillary data in the GOODS-S field, we report the tentative detection of dust continuum equivalent of dust mass log($M_{dust}$/$M_{\odot }$) = 7.47 $\pm$ 0.13 and gas mass log($M_{gas}$/$M_{\odot }$) = 9.42 $\pm$ 0.14. The emerging gas fraction is $f_{gas}$ = 5.3 $\pm$ 1.8%, consistent with the results of previous stacking analyses based on lower resolution sub(mm) observations. Our results support the scenario where high-z QGs have an order of magnitude larger $f_{gas}$ compared to their local counterparts and have experienced quenching with a non negligible gas reservoir in their interstellar medium - i.e. with gas retention. Subsequent analysis yields an anti-correlation between the $f_{gas}$ and the stellar mass of QGs, especially in the high mass end where galaxies reside in the most massive haloes. The $f_{gas}$ - $M_{\ast }$ anti-correlation promotes the selection bias as a possible solution to the tension between the stacking results pointing towards gas retention in high-z QGs of moderate $M_{\ast }$ and the studies of individual targets that favour a fully depleted ISM in massive (log($M_{\ast }$/$M_{\odot }$) high-z QGs.

arXiv commentAccepted to A&A on the 16/03/2023

References in corpus (65)

• Stellar population synthesis at the resolution of 2003
• The Dust Content and Opacity of Actively Star-Forming Galaxies
• Cosmic Star Formation History
• Energy input from quasars regulates the growth and activity of black holes and their host galaxies
• EAZY: A Fast, Public Photometric Redshift Code
• Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
• Galaxies on FIRE (Feedback In Realistic Environments): Stellar Feedback Explains Cosmologically Inefficient Star Formation
• 3D-HST+CANDELS: The Evolution of the Galaxy Size-Mass Distribution since $z=3$
• GOODS-Herschel: an infrared main sequence for star-forming galaxies
• The Evolution of the Stellar Mass Functions of Star-Forming and Quiescent Galaxies to z = 4 from the COSMOS/UltraVISTA Survey
• Detection of quiescent galaxies in a bicolor sequence from z=0-2
• Passively Evolving Early-type Galaxies at 1.4<z<2.5 in the Hubble Ultra Deep Field
• The Herschel view of the dominant mode of galaxy growth from z=4 to the present day
• Morphological quenching of star formation: making early-type galaxies red
• The Atlas3D project - XX. Mass-size and mass-sigma distributions of early-type galaxies: bulge fraction drives kinematics, mass-to-light ratio, molecular gas fraction and stellar initial mass function
• The CO-to-H2 Conversion Factor From Infrared Dust Emission Across the Local Group
• The Evolving Interstellar Medium of Star Forming Galaxies Since z=2 as Probed by Their Infrared Spectral Energy Distributions
• xCOLD GASS: the complete IRAM-30m legacy survey of molecular gas for galaxy evolution studies
• Galaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-Mass Galaxies Since z=2 and the Rapid Buildup of Quiescent Galaxies
• The Atlas3D project -- IV: the molecular gas content of early-type galaxies
• Regularity underlying complexity: a redshift-independent description of the continuous variation of galaxy-scale molecular gas properties in the mass-star formation rate plane
• Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift
• The FourStar Galaxy Evolution Survey (ZFOURGE): ultraviolet to far-infrared catalogs, medium-bandwidth photometric redshifts with improved accuracy, stellar masses, and confirmation of quiescent galaxies to z~3.5
• The [C II] emission as a molecular gas mass tracer in galaxies at low and high redshift
• Spectroscopic Identification of Massive Galaxies at z~2.3 with Strongly Suppressed Star Formation
• The cold interstellar medium of galaxies in the Local Universe
• Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors
• The ATLAS3D Project - XXVIII. Dynamically-driven star formation suppression in early-type galaxies
• A surprising abundance of massive quiescent galaxies at 3 < z < 5 in the first data from JWST CEERS
• Quiescent Galaxies in the 3D-HST Survey: Spectroscopic Confirmation of a Large Number of Galaxies with Relatively Old Stellar Populations at z~2
• Cold gas properties of the Herschel Reference Survey. I. 12CO(1-0) and HI data
• Star formation quenching in massive galaxies
• The Great Observatories Origins Deep Survey - VLT/ISAAC Near-Infrared Imaging of the GOODS-South Field
• Deep Absorption Line Studies of Quiescent Galaxies at z~2: The Dynamical Mass-Size Relation, and First Constraints on the Fundamental plane
• The Argo Simulation: I. Quenching of Massive Galaxies at High Redshift as a Result of Cosmological Starvation
• The Hubble Sequence beyond z=2 for Massive Galaxies: Contrasting Large Star-Forming and Compact Quiescent Galaxies
• The Hawk-I UDS and GOODS Survey (HUGS): Survey design and deep K-band number counts
• The Taiwan ECDFS Near-Infrared Survey: Ultra-deep J and Ks Imaging in the Extended Chandra Deep Field-South
• Jekyll & Hyde: quiescence and extreme obscuration in a pair of massive galaxies 1.5 Gyr after the Big Bang
• The unexpectedly large dust and gas content of quiescent galaxies at z>1.4
• 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
• How dead are dead galaxies? Mid-Infrared fluxes of quiescent galaxies at redshift 0.3 < z < 2.5: implications for star formation rates and dust heating
• The VANDELS ESO public spectroscopic survey: final Data Release of 2087 spectra and spectroscopic measurements
• GOODS-ALMA 2.0: Source catalog, number counts, and prevailing compact sizes in 1.1 mm galaxies
• Massive quenched galaxies at z~0.7 retain large molecular gas reservoirs
• Molecular gas reservoirs in cluster galaxies at z=1.46
• Molecular Gas Contents and Scaling Relations for Massive Passive Galaxies at Intermediate Redshifts from the LEGA-C Survey
• The final data release of ALLSMOG: a survey of CO in typical local low-M* star-forming galaxies
• Quenching of star formation from a lack of inflowing gas to galaxies
• A direct constraint on the gas content of a massive, passively evolving elliptical galaxy at z = 1.43
• ALMA measures rapidly depleted molecular gas reservoirs in massive quiescent galaxies at z~1.5
• The Typical Massive Quiescent Galaxy at z$\sim$3 is a Post-starburst
• Distant red galaxies in the Hubble Ultra Deep Field
• The Interstellar Medium of Quiescent Galaxies and its Evolution With Time
• A${}^3$COSMOS: A census on the molecular gas mass and extent of main-sequence galaxies across cosmic time
• Extremely Low Molecular Gas Content in a Compact, Quiescent Galaxy at z=1.522
• Stacking of large interferometric data sets in the image- and uv-domain -- a comparative study
• Are Cosmological Gas Accretion Streams Multiphase and Turbulent?
• The Diverse Molecular Gas Content of Massive Galaxies Undergoing Quenching at z~1
• High Molecular-Gas to Dust Mass Ratios Predicted in Most Quiescent Galaxies
• Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxies
• The dustier early-type galaxies deviate from late-type galaxies' scaling relations
• Early Science with the Large Millimeter Telescope: Constraining the Gas Fraction of a Compact Quiescent Galaxy at z=1.883
• The evolution of the gas fraction of quiescent galaxies modeled as a consequence of their creation rate
• The uncertain interstellar medium of high-redshift quiescent galaxies: Impact of methodology

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• In pursuit of giants: II. Evolution of dusty quiescent galaxies over the last six billion years from the hCOSMOS survey
• The large molecular gas fraction of post-starburst galaxies at z > 1
• The [CII] 158 $\mu$m emission line as a gas mass tracer in high redshift quiescent galaxies
• The Fate of the Interstellar Medium in Early-type Galaxies. II. Observational Evidence for Morphological Quenching
• Tracing the evolutionary pathways of dust and cold gas in high-z quiescent galaxies with SIMBA
• COALAS III: The ATCA CO(1-0) look at the growth and death of H$\alpha$ emitters in the Spiderweb protocluster at z=2.16
• A${}^3$COSMOS: The dust content of massive quiescent galaxies and its evolution with cosmic time
• Measuring the gas reservoirs in $10^8<$ M${}_{\star }<10^{11}$ M${}_{\odot }$ galaxies at $1\le z\le 3$
• Uncovering the MIR emission of quiescent galaxies with $JWST$