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An environment-dependent halo mass function as a driver for the early quenching of z ≥ 1.5 cluster galaxies

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What this work says

Outgoing claims: the papers this work cites, builds on, or argues with.

inferredcites →https://doi.org/10.1007/s00159-022-00140-3openalex-snapshot
Ram pressure stripping in high-density environments
inferredcites →https://doi.org/10.1016/j.ascom.2016.02.004openalex-snapshot
The eagle simulations of galaxy formation: Public release of halo and galaxy catalogues
inferredcites →https://doi.org/10.1046/j.1365-8711.2001.04912.xopenalex-snapshot
Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
inferredcites →https://doi.org/10.1051/0004-6361/201321237openalex-snapshot
The environmental dependence of the stellar mass function atz~ 1
inferredcites →https://doi.org/10.1051/0004-6361/201321591openalex-snapshot
Planck 2013 results. XVI. Cosmological parameters
inferredcites →https://doi.org/10.1051/0004-6361/201322068openalex-snapshot
Astropy: A community Python package for astronomy
inferredcites →https://doi.org/10.1051/0004-6361/202037754openalex-snapshot
The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching
inferredcites →https://doi.org/10.1051/aas:1996164openalex-snapshot
SExtractor: Software for source extraction
inferredcites →https://doi.org/10.1086/151605openalex-snapshot
On the Infall of Matter Into Clusters of Galaxies and Some Effects on Their Evolution
inferredcites →https://doi.org/10.1086/157917openalex-snapshot
The evolution of disk galaxies and the origin of S0 galaxies
inferredcites →https://doi.org/10.1086/305264openalex-snapshot
Morphological Transformation from Galaxy Harassment
inferredcites →https://doi.org/10.1086/426016openalex-snapshot
The Radial Distribution of Galaxies in Λ Cold Dark Matter Clusters
inferredcites →https://doi.org/10.1086/520083openalex-snapshot
The Discovery of 1000 km s[FORMULA][F][SUP]-1[/SUP][/F][/FORMULA] Outflows in Massive Poststarburst Galaxies at [FORMULA][F]z=0.6[/F][/FORMULA]
inferredcites →https://doi.org/10.1088/0004-637x/721/1/193openalex-snapshot
MASS AND ENVIRONMENT AS DRIVERS OF GALAXY EVOLUTION IN SDSS AND zCOSMOS AND THE ORIGIN OF THE SCHECHTER FUNCTION
inferredcites →https://doi.org/10.1088/0004-637x/757/1/4openalex-snapshot
MASS AND ENVIRONMENT AS DRIVERS OF GALAXY EVOLUTION. II. THE QUENCHING OF SATELLITE GALAXIES AS THE ORIGIN OF ENVIRONMENTAL EFFECTS
inferredcites →https://doi.org/10.1088/0004-637x/771/1/30openalex-snapshot
THE CONNECTION BETWEEN GALAXIES AND DARK MATTER STRUCTURES IN THE LOCAL UNIVERSE
inferredcites →https://doi.org/10.1088/0067-0049/206/1/8openalex-snapshot
A PUBLIC K s -SELECTED CATALOG IN THE COSMOS/ULTRAVISTA FIELD: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR POPULATION PARAMETERS ,
inferredcites →https://doi.org/10.1088/1674-4527/12/8/004openalex-snapshot
The current status of galaxy formation
inferredcites →https://doi.org/10.1093/mnras/staa2752openalex-snapshot
The GOGREEN survey: post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z > 1
inferredcites →https://doi.org/10.1093/mnras/staa3008openalex-snapshot
The GOGREEN and GCLASS surveys: first data release
inferredcites →https://doi.org/10.1093/mnras/stab1036openalex-snapshot
The stellar mass function and evolution of the density profile of galaxy clusters from the Hydrangea simulations at 0 < z < 1.5
inferredcites →https://doi.org/10.1093/mnras/stab3484openalex-snapshot
Satellite quenching was not important for z ∼ 1 clusters: most quenching occurred during infall
inferredcites →https://doi.org/10.1093/mnras/stab3673openalex-snapshot
On the quenching of star formation in observed and simulated central galaxies: evidence for the role of integrated AGN feedback
inferredcites →https://doi.org/10.1093/mnras/stac3438openalex-snapshot
GOGREEN: A critical assessment of environmental trends in cosmological hydrodynamical simulations at z ≈ 1
inferredcites →https://doi.org/10.1093/mnras/stad1098openalex-snapshot
The role of mass and environment in the build-up of the quenched galaxy population since cosmic noon
inferredcites →https://doi.org/10.1093/mnras/stad2995openalex-snapshot
When the well runs dry: modelling environmental quenching of high-mass satellites in massive clusters at z ≳ 1
inferredcites →https://doi.org/10.1093/mnras/stu1227openalex-snapshot
Dancing in the dark: galactic properties trace spin swings along the cosmic web
inferredcites →https://doi.org/10.1093/mnras/stu2058openalex-snapshot
The EAGLE project: simulating the evolution and assembly of galaxies and their environments
inferredcites →https://doi.org/10.1093/mnras/stv725openalex-snapshot
The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
inferredcites →https://doi.org/10.1093/mnras/stv852openalex-snapshot
Evolution of galaxy stellar masses and star formation rates in the eagle simulations
inferredcites →https://doi.org/10.1093/mnras/stw188openalex-snapshot
Strong bimodality in the host halo mass of central galaxies from galaxy–galaxy lensing
inferredcites →https://doi.org/10.1093/mnras/stw2735openalex-snapshot
The dark nemesis of galaxy formation: why hot haloes trigger black hole growth and bring star formation to an end
inferredcites →https://doi.org/10.1093/mnras/stw2740openalex-snapshot
Size evolution of normal and compact galaxies in the EAGLE simulation
inferredcites →https://doi.org/10.1093/mnras/stx1370openalex-snapshot
Gemini Observations of Galaxies in Rich Early Environments (GOGREEN) I: survey description
inferredcites →https://doi.org/10.1093/mnras/stx1403openalex-snapshot
The Hydrangea simulations: galaxy formation in and around massive clusters
inferredcites →https://doi.org/10.1093/mnras/stx1647openalex-snapshot
The Cluster-EAGLE project: global properties of simulated clusters with resolved galaxies
inferredcites →https://doi.org/10.1093/mnras/stx3112openalex-snapshot
First results from the IllustrisTNG simulations: the stellar mass content of groups and clusters of galaxies
inferredcites →https://doi.org/10.1093/mnras/stz937openalex-snapshot
simba: Cosmological simulations with black hole growth and feedback
inferredcites →https://doi.org/10.1109/mcse.2007.55openalex-snapshot
Matplotlib: A 2D Graphics Environment
inferredcites →https://doi.org/10.1111/j.1365-2966.2009.15034.xopenalex-snapshot
Substructures in hydrodynamical cluster simulations
inferredcites →https://doi.org/10.1111/j.1365-2966.2009.15338.xopenalex-snapshot
The 6dF Galaxy Survey: final redshift release (DR3) and southern large-scale structures
inferredcites →https://doi.org/10.1111/j.1365-2966.2012.21564.xopenalex-snapshot
The Phoenix Project: the dark side of rich Galaxy clusters
inferredcites →https://doi.org/10.1146/annurev-astro-081811-125521openalex-snapshot
Observational Evidence of Active Galactic Nuclei Feedback
inferredcites →https://doi.org/10.3847/0004-637x/825/2/113openalex-snapshot
THE EFFECTS OF THE LOCAL ENVIRONMENT AND STELLAR MASS ON GALAXY QUENCHING TO z ∼ 3
inferredcites →https://doi.org/10.3847/1538-4357/aa6258openalex-snapshot
Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5 < z < 2.5
inferredcites →https://doi.org/10.3847/1538-4357/ab14eeopenalex-snapshot
The Evolution of the Quenching of Star Formation in Cluster Galaxies since z ∼ 1
inferredcites →https://doi.org/10.3847/2041-8205/817/2/l21openalex-snapshot
THE RELATION BETWEEN GALAXY STRUCTURE AND SPECTRAL TYPE: IMPLICATIONS FOR THE BUILDUP OF THE QUIESCENT GALAXY POPULATION AT 0.5 < z < 2.0
inferredcites →https://doi.org/10.48550/arxiv.1706.09899openalex-snapshot
The EAGLE simulations of galaxy formation: Public release of particle data

What points at this work

Incoming claims: where this work appears in other papers’ reference lists and arguments.

inferred← uses_datahttps://doi.org/10.5281/zenodo.12544655zenodo-depositor-declared
inferred← citeshttps://doi.org/10.1051/0004-6361/202554407openalex-snapshot
The HST -Hyperion Survey: Companion fraction and overdensity in a z ∼ 2.5 proto-supercluster
inferred← citeshttps://doi.org/10.1093/mnras/staf635openalex-snapshot
Insights into environmental quenching at z ∼ 1: an enhancement of faint, low-mass passive galaxies in clusters
inferred← citeshttps://doi.org/10.1093/mnras/staf932openalex-snapshot
Distinct origins of environmentally quenched galaxies in the core and outer virialized regions of massive clusters at 0.8 < z < 1.5
inferred← citeshttps://doi.org/10.3847/1538-4357/ad5e78openalex-snapshot
Environmental Effects on the Stellar Mass Function in a z ∼ 3.3 Overdensity of Galaxies in the COSMOS Field*
inferred← citeshttps://doi.org/10.3847/1538-4357/ad90aeopenalex-snapshot
Modeling the Multiwavelength Detection of Protoclusters. I. An Excess of Submillimeter Galaxies in Protocluster Cores
inferred← citeshttps://doi.org/10.3847/1538-4357/ad9aa4openalex-snapshot
The Importance of Gas Starvation in Driving Satellite Quenching in Galaxy Groups at z ~ 0.8
inferred← citeshttps://doi.org/10.3847/1538-4357/ae2c00openalex-snapshot
The Distribution of Quenched Galaxies in the Massive z = 0.87 Galaxy Cluster El Gordo
inferred← citeshttps://doi.org/10.3847/1538-4357/ae876bopenalex-snapshot
Cluster versus Field: Clear Evidence for a Morphology–Density Relation in All Environments at z ∼ 1.6
inferred← citeshttps://doi.org/10.3847/2041-8213/adf7abopenalex-snapshot
UNCOVER/MegaScience: No Evidence of Environmental Quenching in a z ∼ 2.6 Protocluster
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