The Fraction of Quiescent Massive Galaxies in the Early Universe
arXiv:0901.2898 · doi:10.1051/0004-6361/200911650
Abstract
Aims: The aim of this work is to collect a complete, mass--selected sample of galaxies with very low specific star formation rate, for a comparison with the prediction of recent theoretical models. Method: We use the 24/K flux ratio, complemented by the SED fitting to the full 0.35-8.0 mum spectral distribution, to select quiescent galaxies from z~0.4 to z~4 in the GOODS--MUSIC sample. Our observational selection can be translated into thresholds on the specific star formation rate SFR/M_*, that can be used to compare with the theoretical predictions. Results: We find that, in the framework of the well known global decline of the quiescent fraction with redshift, a non-negligible fraction ~15-20% of massive galaxies with very low specific star formation rate exists up to z~4, including a tail of "Red&Dead" galaxies with SFR/M_*<10^{-11}/yr. Recent theoretical models vary to a large extent in the prediction of the fraction of galaxies with very low specific star formation rates, and are unable to provide a global match to our data.
The replaced version matches the published one (typos corrected)
References in corpus (20)
- Multiwavelength study of massive galaxies at z~2. I. Star formation and galaxy growth
- Spectral Energy Distributions of Hard X-ray selected AGNs in the XMDS Survey
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
- The Galaxy Mass Function up to z=4 in the GOODS-MUSIC sample: into the epoch of formation of massive galaxies
- What do we learn from IRAC observations of galaxies at 2 < z < 3.5?
- Multiwavelength study of massive galaxies at z~2. II. Widespread Compton thick AGN and the concurrent growth of black holes and bulges
- The GOODS-MUSIC sample: a multicolour catalog of near-IR selected galaxies in the GOODS-South field
- The SWIRE-VVDS-CFHTLS surveys: stellar mass assembly over the last 10 Gyears. Evidence for a major build up of the red sequence between z=2 and z=1
- The high redshift galaxy population in hierarchical galaxy formation models
- Unveiling obscured accretion in the Chandra Deep Field South
- Spectroscopic Identification of Massive Galaxies at z~2.3 with Strongly Suppressed Star Formation
- Spitzer Mid-to-Far-Infrared Flux Densities of Distant Galaxies
- The History of Cosmological Star Formation: Three Independent Approaches and a Critical Test Using the Extragalactic Background Light
- Cosmic evolution of the galaxy mass and luminosity functions by morphological type from multi-wavelength data in the CDF-South
- A comparison among LBGs, DRGs and BzK galaxies: their contribution to the stellar mass density in the GOODS-MUSIC sample
- The Gemini Deep Deep Survey: VIII. When Did Early-type Galaxies Form?
- The Nascent Red Sequence at z~2
- Reproducing the assembly of massive galaxies within the hierarchical cosmogony
- The red and blue galaxy populations in the GOODS field: evidence for an excess of red dwarfs
- The contribution of very massive high-redshift SWIRE galaxies to the stellar mass function
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- What turns galaxies off? The different morphologies of star-forming and quiescent galaxies since z~2 from CANDELS
- Star formation rates and masses of z ~ 2 galaxies from multicolour photometry
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- The evolving relations between size, mass, surface density, and star formation in 3x10^4 galaxies since z=2
- The evolution of the dust temperatures of galaxies in the SFR plane up to
- Near infrared spectroscopy and star-formation histories of 3<z<4 quiescent galaxies
- A substantial population of massive quiescent galaxies at z~4 from ZFOURGE
- Quiescent galaxies 1.5 billion years after the Big Bang and their progenitors
- An Atlas of Color-selected Quiescent Galaxies at in Public Fields
- Effects of Local Environment and Stellar Mass on Galaxy Quenching out to z~3
- CANDELS+3D-HST: compact SFGs at z~2-3, the progenitors of the first quiescent galaxies
- T-PHOT: A new code for PSF-matched, prior-based, multiwavelength extragalactic deconfusion photometry
- The FMOS-COSMOS survey of star-forming galaxies at z~1.6 III. Survey design, performance, and sample characteristics
- Red & Dead CANDELS: massive passive galaxies at the dawn of the Universe
- The Argo Simulation: I. Quenching of Massive Galaxies at High Redshift as a Result of Cosmological Starvation
- Nuclear Activity is more prevalent in Star-Forming Galaxies
- Black hole growth and starburst activity at z = 0.6-4 in the Chandra Deep Field South. Host galaxies properties of obscured AGN
- Exploring the z=3-4 massive galaxy population with ZFOURGE: the prevalence of dusty and quiescent galaxies
- Supermassive Black Holes at High Redshift are Expected to be Obscured by their Massive Host Galaxies' Inter Stellar Medium
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- Color and Stellar Population Gradients in Passively Evolving Galaxies at z~2 from HST/WFC3 Deep Imaging in the Hubble Ultra Deep Field
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- The sizes of massive quiescent and star forming galaxies at z~4 with ZFOURGE and CANDELS
- Timing the earliest quenching events with a robust sample of massive quiescent galaxies at 2 < z < 5
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- The Age Spread of Quiescent Galaxies with the NEWFIRM Medium-band Survey: Identification of the Oldest Galaxies out to z~2
- The VIMOS VLT Deep Survey: the contribution of minor mergers to the growth of L_B >= L*_B galaxies since z ~ 1 from spectroscopically identified pairs
- Chasing passive galaxies in the early Universe: a critical analysis in CANDELS GOODS-South
- The evolution of quiescent galaxies at high redshift (z > 1.4)
- The unusual NIV]-emitter galaxy GDS J033218.92-275302.7: star formation or AGN-driven winds from a massive galaxy at z=5.56
- The bolometric output and host-galaxy properties of obscured AGN in the XMM-COSMOS survey
- Inferring the star formation histories of the most massive and passive early-type galaxies at z<0.3
- Optically-faint massive Balmer Break Galaxies at z>3 in the CANDELS/GOODS fields
- What Are the Progenitors of Compact, Massive, Quiescent Galaxies at z=2.3? The Population of Massive Galaxies at z>3 from NMBS and CANDELS
- Cosmic evolution of low-excitation radio galaxies in the LOFAR Two-meter Sky Survey Deep Fields
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- COSMOS2020: Exploring the dawn of quenching for massive galaxies at 3 < z < 5 with a new colour selection method
- Pathways to quiescence: SHARDS view on the Star Formation Histories of massive quiescent galaxies at 1.0 < z < 1.5
- Stellar mass functions of galaxies at 4<z<7 from an IRAC-selected sample in COSMOS/UltraVISTA: limits on the abundance of very massive galaxies
- The Next Generation Virgo Cluster Survey (NGVS). XXIV. The Red Sequence to 10 L and Comparisons with Galaxy Formation Models
- Filament profiles from WISExSCOS galaxies as probes of the impact of environmental effects
- The emergence of passive galaxies in the early Universe
- A Study of Massive and Evolved Galaxies at High Redshift
- Morphology Dependence Of Stellar Age in Quenched Galaxies at Redshift ~ 1.2: Massive Compact Galaxies Are Older Than More Extended Ones
- The minor role of gas-rich major mergers in the rise of intermediate-mass early types at z <~ 1
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- The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe
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- The interaction-driven starburst contribution to the cosmic star formation rate density
- The Stellar Mass Function in CANDELS and Frontier Fields: the build-up of low mass passive galaxies since z~3
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- MOIRCS Deep Survey. X. Evolution of Quiescent Galaxies as a Function of Stellar Mass at 0.5<z<2.5
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- Exploring the High-Mass End of the Stellar Mass Function of Star Forming Galaxies at Cosmic Noon
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- Massive Quiescent Galaxies at z>3 in The Millennium Simulation Populated by A Semi-analytic Galaxy Formation Model
- Maximising the power of deep extragalactic imaging surveys with the James Webb Space Telescope
- PRIMER & JADES reveal an abundance of massive quiescent galaxies at 2 < z < 5
- Physical Properties of the Host Galaxies of Ca-rich Transients
- The detection of ultra-faint low surface brightness dwarf galaxies in the Virgo Cluster: a Probe of Dark Matter and Baryonic Physics
- Accretion and jets in a low luminosity AGN: the nucleus of NGC 1052
- Recently Quenched Galaxies at z = 0.2 - 4.8 in the COSMOS UltraVISTA Field
- A mass threshold in the number density of passive galaxies at z2
- The morphologies and masses of extremely red galaxies in the Groth Strip survey
- Great Balls of FIRE IV. The contribution of massive star clusters to the astrophysical population of merging binary black holes
- Cosmic Stillness: High Quiescent Galaxy Fractions Across Upper Mass Scales in the Early Universe to z = 7 with JWST
- A Galaxy-Halo Model for Multiple Cosmological Tracers
- The Formation and Evolution of Massive Galaxies
- A census of quiescent galaxies across with JWST/MIRI: Mass-dependent number density evolution of quiescent galaxies in the early Universe
- A Large Massive Quiescent Galaxy Sample at z~1.2
- The stellar mass function of quiescent and star-forming galaxies and its dependence on morphology in COSMOS-Web
- The Connection between Dusty Star-Forming Galaxies and the First Massive Quenched Galaxies
- LEGA-C stellar populations scaling relations. II: Dissecting mass-complete archaeological trends and their evolution since z~0.7 with LEGA-C and SDSS
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