Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2
arXiv:1611.07524 · doi:10.3847/1538-4357/835/2/153
Abstract
We make publicly available a catalog of calibrated environmental measures for galaxies in the five 3D-HST/CANDELS deep fields. Leveraging the spectroscopic and grism redshifts from the 3D-HST survey, multi wavelength photometry from CANDELS, and wider field public data for edge corrections, we derive densities in fixed apertures to characterize the environment of galaxies brighter than mag in the redshift range . By linking observed galaxies to a mock sample, selected to reproduce the 3D-HST sample selection and redshift accuracy, each 3D-HST galaxy is assigned a probability density function of the host halo mass, and a probability that is a central or a satellite galaxy. The same procedure is applied to a sample selected from SDSS. We compute the fraction of passive central and satellite galaxies as a function of stellar and halo mass, and redshift, and then derive the fraction of galaxies that were quenched by environment specific processes. Using the mock sample, we estimate that the timescale for satellite quenching is Gyr; longer at lower stellar mass or lower redshift, but remarkably independent of halo mass. This indicates that, in the range of environments commonly found within the 3D-HST sample, satellites are quenched by exhaustion of their gas reservoir in absence of cosmological accretion. We find that the quenching times can be separated into a delay phase during which satellite galaxies behave similarly to centrals at fixed stellar mass, and a phase where the star formation rate drops rapidly ( Gyr), as shown previously at . We conclude that this scenario requires satellite galaxies to retain a large reservoir of multi-phase gas upon accretion, even at high redshift, and that this gas sustains star formation for the long quenching times observed.
35 pages, 29 figures, 2 tables. Accepted for publication in ApJ. The catalogue of environmental measures is available at: http://dx.doi.org/10.5281/zenodo.168056
References in corpus (47)
- Mass and environment as drivers of galaxy evolution in SDSS and zCOSMOS and the origin of the Schechter function
- 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
- The propagation of uncertainties in stellar population synthesis modeling I: The relevance of uncertain aspects of stellar evolution and the IMF to the derived physical properties of galaxies
- EAZY: A Fast, Public Photometric Redshift Code
- K-corrections and filter transformations in the ultraviolet, optical, and near infrared
- The hierarchical formation of the brightest cluster galaxies
- COSMOS Photometric Redshifts with 30-bands for 2-deg2
- An ultra-deep near-infrared spectrum of a compact quiescent galaxy at z=2.2
- zCOSMOS: A Large VLT/VIMOS redshift survey covering 0 < z < 3 in the COSMOS field
- 3D-HST WFC3-selected Photometric Catalogs in the Five CANDELS/3D-HST Fields: Photometry, Photometric Redshifts and Stellar Masses
- Detection of quiescent galaxies in a bicolor sequence from z=0-2
- Constraining the Low-Mass Slope of the Star Formation Sequence at 0.5<z<2.5
- UltraVISTA: a new ultra-deep near-infrared survey in COSMOS
- Combined CO & Dust Scaling Relations of Depletion Time and Molecular Gas Fractions with Cosmic Time, Specific Star Formation Rate and Stellar Mass
- The KMOS^3D Survey: design, first results, and the evolution of galaxy kinematics from 0.7<z<2.7
- Structure and star formation in galaxies out to z=3: evidence for surface density dependent evolution and upsizing
- The Importance of Satellite Quenching for the Build-Up of the Red Sequence of Present Day Galaxies
- The MOSFIRE Deep Evolution Field (MOSDEF) Survey: Rest-Frame Optical Spectroscopy for ~1500 H-Selected Galaxies at 1.37 < z < 3.8
- A Cosmological Framework for the Co-Evolution of Quasars, Supermassive Black Holes, and Elliptical Galaxies: II. Formation of Red Ellipticals
- COLD GASS, an IRAM Legacy Survey of Molecular Gas in Massive Galaxies: II. The non-universality of the Molecular Gas Depletion Timescale
- The Cosmic Evolution Survey (COSMOS): Subaru Observations of the HST COSMOS Field
- The VIMOS Ultra-Deep Survey: ~10,000 galaxies with spectroscopic redshifts to study galaxy assembly at early epochs 2<z<~6
- The Subaru/XMM-Newton Deep Survey (SXDS) - II. Optical Imaging and Photometric Catalogs
- The XMM-Newton wide-field survey in the COSMOS field: VI. Statistical properties of clusters of galaxies
- The Multiwavelength Survey by Yale-Chile (MUSYC): Deep Medium-Band optical imaging and high quality 32-band photometric redshifts in the ECDF-S
- The DEEP2 Galaxy Redshift Survey: The Relationship Between Galaxy Properties and Environment at z ~ 1
- LoCuSS: The slow quenching of star formation in cluster galaxies and the need for pre-processing
- The origin of dwarf ellipticals in the Virgo cluster
- The build-up of the colour-magnitude relation in galaxy clusters since z~0.8
- MUSE sneaks a peek at extreme ram-pressure stripping events. I. A kinematic study of the archetypal galaxy ESO137-001
- CARS: the CFHTLS-Archive-Research Survey; I. Five-band multi-colour data from 37 sq. deg. CFHTLS-Wide observations
- On the origin of the faint-end of the red sequence in high density environments
- Large Structures and Galaxy Evolution in COSMOS at z < 1.1
- The GALEX Ultraviolet Virgo Cluster Survey (GUViCS). IV: The role of the cluster environment on galaxy evolution
- A Public, K-Selected, Optical-to-Near-Infrared Catalog of the Extended Chandra Deep Field South (ECDFS) from the MUltiwavelength Survey by Yale-Chile (MUSYC)
- The influence of the environmental history on quenching star formation in a CDM universe
- The Dependence of Galaxy Formation on Cosmological Parameters: Can we distinguish the WMAP1 and WMAP3 Parameter Sets?
- The Rest-Frame Optical Luminosity Function of Cluster Galaxies at z<0.8 and the Assembly of the Cluster Red Sequence
- Overconsumption, outflows and the quenching of satellite galaxies
- The quenching of the star formation activity in cluster galaxies
- The GEEC2 spectroscopic survey of Galaxy Groups at
- Ultra-deep catalog of X-ray groups in the Extended Chandra Deep Field South
- First results from the VIRIAL survey: the stellar content of -selected quiescent galaxies at from KMOS
- X-Ray Groups of Galaxies in the Aegis Deep and Wide Fields
- Low-power radio galaxy environments in the Subaru/XMM-Newton Deep Field at z~0.5
- A new (2+1)D cluster finding algorithm based on photometric redshifts: large scale structure in the Chandra Deep Field South
- The definition of environment and its relation to the quenching of galaxies at z=1-2 in a hierarchical Universe
Cited by in corpus (17)
- Effect of local environment and stellar mass on galaxy quenching and morphology at
- The KMOS^3D Survey: data release and final survey paper
- The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0<z<1.4 and the complex nature of satellite quenching
- ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
- Large Scale Structures in the CANDELS Fields: The Role of the Environment in Star Formation Activity
- Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: Survey Description
- The Roles of Mass and Environment in the Quenching of Galaxies. II
- On stellar mass loss from galaxies in groups and clusters
- Multiscale cosmic web detachments, connectivity, and preprocessing in the supercluster SClA2142 cocoon
- Galaxy interactions in IllustrisTNG-100, I: The power and limitations of visual identification
- MUSE sneaks a peek at extreme ram-pressure stripping events - IV. Hydrodynamic and gravitational interactions in the Blue Infalling Group
- CANDELS Sheds Light on the Environmental Quenching of Low-mass Galaxies
- Specific Frequencies and Luminosity Profiles of Cluster Galaxies and Intracluster Light in Abell 1689
- The MOSDEF Survey: Environmental dependence of the gas-phase metallicity of galaxies at
- Structural and dynamical modeling of WINGS clusters. I. The distribution of cluster galaxies of different morphological classes within regular and irregular clusters
- Growing up in a megalopolis: Environmental effects on galaxy evolution in a supercluster at z~0.65 in UKIDSS UDS
- Quenched galaxies in clusters of galaxies and their outskirts