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Environmental impacts on molecular gas in protocluster galaxies at z ∼ 2

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What this work says

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

inferredcites →https://doi.org/10.1038/nature07648openalex-snapshot
Cold streams in early massive hot haloes as the main mode of galaxy formation
inferredcites →https://doi.org/10.1051/0004-6361/201117239openalex-snapshot
GOODS– Herschel : an infrared main sequence for star-forming galaxies
inferredcites →https://doi.org/10.1051/0004-6361/201322313openalex-snapshot
Cold gas properties of the Herschel Reference Survey
inferredcites →https://doi.org/10.1051/0004-6361/201527705openalex-snapshot
Simulations of ram-pressure stripping in galaxy-cluster interactions
inferredcites →https://doi.org/10.1051/0004-6361/201730449openalex-snapshot
The implications of the surprising existence of a large, massive CO disk in a distant protocluster
inferredcites →https://doi.org/10.1051/0004-6361:20021368openalex-snapshot
A ${\vec Chandra}$ study of X-ray sources in the field of the $\mathsf{\vec z=}$ 2.16 radio galaxy MRC 1138-262
inferredcites →https://doi.org/10.1086/162519openalex-snapshot
The evolution of galaxies in clusters. V - A study of populations since Z approximately equal to 0.5
inferredcites →https://doi.org/10.1086/167787openalex-snapshot
The effects of environment on the molecular and atomic gas properties of large Virgo cluster spirals
inferredcites →https://doi.org/10.1086/312981openalex-snapshot
Deep Imaging of the Field of the High‐Redshift Radio Source 4C 23.56
inferredcites →https://doi.org/10.1086/321609openalex-snapshot
Interpreting the Cosmic Infrared Background: Constraints on the Evolution of the Dust‐enshrouded Star Formation Rate
inferredcites →https://doi.org/10.1086/376392openalex-snapshot
Galactic Stellar and Substellar Initial Mass Function
inferredcites →https://doi.org/10.1086/588749openalex-snapshot
FIREWORKSU38–to–24 μm Photometry of the GOODS Chandra Deep Field–South: Multiwavelength Catalog and Total Infrared Properties of DistantKs‐selected Galaxies
inferredcites →https://doi.org/10.1088/0004-637x/738/1/106openalex-snapshot
ON STAR FORMATION RATES AND STAR FORMATION HISTORIES OF GALAXIES OUT TO z ∼ 3
inferredcites →https://doi.org/10.1088/0004-637x/746/1/69openalex-snapshot
THE METALLICITY DEPENDENCE OF THE CO → H 2 CONVERSION FACTOR IN z ⩾ 1 STAR-FORMING GALAXIES
inferredcites →https://doi.org/10.1088/0004-637x/757/1/15openalex-snapshot
A STARBURSTING PROTO-CLUSTER IN MAKING ASSOCIATED WITH A RADIO GALAXY ATz= 2.53 DISCOVERED BY Hα IMAGING
inferredcites →https://doi.org/10.1088/0004-637x/758/2/73openalex-snapshot
THE IMPACT OF INTERACTIONS, BARS, BULGES, AND ACTIVE GALACTIC NUCLEI ON STAR FORMATION EFFICIENCY IN LOCAL MASSIVE GALAXIES
inferredcites →https://doi.org/10.1088/0004-637x/795/2/165openalex-snapshot
STRONG NEBULAR LINE RATIOS IN THE SPECTRA ofz∼ 2-3 STAR FORMING GALAXIES: FIRST RESULTS FROM KBSS-MOSFIRE
inferredcites →https://doi.org/10.1088/0004-637x/800/1/20openalex-snapshot
COMBINED CO AND DUST SCALING RELATIONS OF DEPLETION TIME AND MOLECULAR GAS FRACTIONS WITH COSMIC TIME, SPECIFIC STAR-FORMATION RATE, AND STELLAR MASS
inferredcites →https://doi.org/10.1088/0067-0049/214/2/15openalex-snapshot
A HIGHLY CONSISTENT FRAMEWORK FOR THE EVOLUTION OF THE STAR-FORMING “MAIN SEQUENCE” FROM z ∼ 0-6
inferredcites →https://doi.org/10.1088/0067-0049/214/2/24openalex-snapshot
3D-HST WFC3-SELECTED PHOTOMETRIC CATALOGS IN THE FIVE CANDELS/3D-HST FIELDS: PHOTOMETRY, PHOTOMETRIC REDSHIFTS, AND STELLAR MASSES
inferredcites →https://doi.org/10.1088/2041-8205/788/2/l23openalex-snapshot
EVIDENCE FOR A GAS-RICH MAJOR MERGER IN A PROTO-CLUSTER AT z = 2.5
inferredcites →https://doi.org/10.1093/mnras/sts096openalex-snapshot
A large Hα survey at z = 2.23, 1.47, 0.84 and 0.40: the 11 Gyr evolution of star-forming galaxies from HiZELS★
inferredcites →https://doi.org/10.1093/mnras/sts133openalex-snapshot
Massive starburst galaxies in a z = 2.16 proto-cluster unveiled by panoramic Hα mapping
inferredcites →https://doi.org/10.1093/mnras/stu677openalex-snapshot
Active galactic nuclei-driven outflows without immediate quenching in simulations of high-redshift disc galaxies
inferredcites →https://doi.org/10.1093/mnras/stv1599openalex-snapshot
Predicting dust extinction properties of star-forming galaxies from Hα/UV ratio
inferredcites →https://doi.org/10.1093/mnras/stx2494openalex-snapshot
MAHALO Deep Cluster Survey I. Accelerated and enhanced galaxy formation in the densest regions of a protocluster at z = 2.5
inferredcites →https://doi.org/10.1093/mnras/sty2618openalex-snapshot
MAHALO Deep Cluster Survey II. Characterizing massive forming galaxies in the Spiderweb protocluster at z = 2.2
inferredcites →https://doi.org/10.1093/mnras/sty469openalex-snapshot
The VANDELS survey: dust attenuation in star-forming galaxies at z = 3-4
inferredcites →https://doi.org/10.1093/mnrasl/slu029openalex-snapshot
Identification of the progenitors of rich clusters and member galaxies in rapid formation at z > 2
inferredcites →https://doi.org/10.1093/mnrasl/slx019openalex-snapshot
Direct evidence for Ly$\boldsymbol{\alpha }$ depletion in the protocluster core
inferredcites →https://doi.org/10.1093/mnrasl/sly034openalex-snapshot
Giant galaxy growing from recycled gas: ALMA maps the circumgalactic molecular medium of the Spiderweb in [ C i ]
inferredcites →https://doi.org/10.1093/pasj/63.sp2.s415openalex-snapshot
Discovery of an Excess of H Emitters around 4C 23.56 at z = 2.48
inferredcites →https://doi.org/10.1093/pasj/64.2.22openalex-snapshot
X-Ray Groups of Galaxies at 0.5 1 in zCOSMOS: Increased AGN Activities in High Redshift Groups
inferredcites →https://doi.org/10.1111/j.1365-2966.2005.09451.xopenalex-snapshot
How do galaxies get their gas?
inferredcites →https://doi.org/10.1111/j.1365-2966.2006.10145.xopenalex-snapshot
Galaxy bimodality due to cold flows and shock heating
inferredcites →https://doi.org/10.1111/j.1365-2966.2006.10704.xopenalex-snapshot
Protoclusters with evolved populations around radio galaxies at z 2.5
inferredcites →https://doi.org/10.1111/j.1365-2966.2007.11739.xopenalex-snapshot
The first appearance of the red sequence of galaxies in proto-clusters at 2 lsimzlsim 3
inferredcites →https://doi.org/10.1111/j.1365-2966.2012.21697.xopenalex-snapshot
Deep observations of CO line emission from star-forming galaxies in a cluster candidate atz=1.5
inferredcites →https://doi.org/10.1126/science.aag0512openalex-snapshot
Molecular gas in the halo fuels the growth of a massive cluster galaxy at high redshift
inferredcites →https://doi.org/10.1146/annurev-astro-082812-140944openalex-snapshot
The CO-to-H 2 Conversion Factor
inferredcites →https://doi.org/10.1146/annurev.astro.36.1.189openalex-snapshot
STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
inferredcites →https://doi.org/10.3847/0067-0049/225/2/27openalex-snapshot
THE 3D-HST SURVEY: HUBBLE SPACE TELESCOPE WFC3/G141 GRISM SPECTRA, REDSHIFTS, AND EMISSION LINE MEASUREMENTS FOR ∼100,000 GALAXIES
inferredcites →https://doi.org/10.3847/1538-4357/aa61a0openalex-snapshot
Evolution of Interstellar Medium, Star Formation, and Accretion at High Redshift
inferredcites →https://doi.org/10.3847/1538-4357/aa74c2openalex-snapshot
A Radio-to-mm Census of Star-forming Galaxies in Protocluster 4C23.56 at Z = 2.5: Gas Mass and Its Fraction Revealed with ALMA
inferredcites →https://doi.org/10.3847/1538-4357/aa87b2openalex-snapshot
Deep CO(1–0) Observations of z = 1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
inferredcites →https://doi.org/10.3847/1538-4357/aa93f6openalex-snapshot
ALMA Pinpoints a Strong Overdensity of U/LIRGs in the Massive Cluster XCS J2215 at z = 1.46
inferredcites →https://doi.org/10.3847/1538-4357/aaa4b4openalex-snapshot
PHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions*
inferredcites →https://doi.org/10.3847/1538-4357/aab3e7openalex-snapshot
Molecular Gas Reservoirs in Cluster Galaxies at z = 1.46
inferredcites →https://doi.org/10.3847/1538-4357/aac836openalex-snapshot
Similar Scaling Relations for the Gas Content of Galaxies Across Environments to z ∼ 3.5
inferredcites →https://doi.org/10.3847/1538-4365/aa97e0openalex-snapshot
xCOLD GASS: The Complete IRAM 30 m Legacy Survey of Molecular Gas for Galaxy Evolution Studies
inferredcites →https://doi.org/10.3847/2041-8205/826/2/l28openalex-snapshot
ENHANCED STAR FORMATION OF LESS MASSIVE GALAXIES IN A PROTOCLUSTER AT z = 2.5
inferredcites →https://doi.org/10.3847/2041-8213/aa71adopenalex-snapshot
Evolutionary Phases of Gas-rich Galaxies in a Galaxy Cluster at z = 1.46
inferredcites →https://doi.org/10.3847/2041-8213/aa7338openalex-snapshot
Rotating Starburst Cores in Massive Galaxies at z = 2.5
inferredcites →https://doi.org/10.3847/2041-8213/aa77f3openalex-snapshot
ALMA Observations of Gas-rich Galaxies in z ∼ 1.6 Galaxy Clusters: Evidence for Higher Gas Fractions in High-density Environments
inferredcites →https://doi.org/10.3847/2041-8213/aaeb2copenalex-snapshot
Revealing the Environmental Dependence of Molecular Gas Content in a Distant X-Ray Cluster at z = 2.51

What points at this work

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

inferred← citeshttps://doi.org/10.12688/openreseurope.17445.1zenodo-depositor-declared
Atacama Large Aperture Submillimeter Telescope (AtLAST) science: Surveying the distant Universe
inferred← citeshttps://doi.org/10.1016/j.newast.2026.102561openalex-snapshot
Fueling and feedback mechanisms at the nodes of the cosmic web
inferred← citeshttps://doi.org/10.1038/s41586-023-05761-xopenalex-snapshot
Forming intracluster gas in a galaxy protocluster at a redshift of 2.16
inferred← citeshttps://doi.org/10.1051/0004-6361/201936148openalex-snapshot
Molecular gas in distant brightest cluster galaxies
inferred← citeshttps://doi.org/10.1051/0004-6361/202038081openalex-snapshot
Molecular gas in CLASH brightest cluster galaxies at z ∼ 0.2 – 0.9
inferred← citeshttps://doi.org/10.1051/0004-6361/202038231openalex-snapshot
The ALPINE-ALMA [C II] survey
inferred← citeshttps://doi.org/10.1051/0004-6361/202038673openalex-snapshot
Massive molecular gas reservoir around the central AGN in the CARLA J1103 + 3449 cluster at z = 1.44
inferred← citeshttps://doi.org/10.1051/0004-6361/202039346openalex-snapshot
The VIMOS Ultra Deep Survey: The reversal of the star-formation rate − density relation at 2 <z< 5
inferred← citeshttps://doi.org/10.1051/0004-6361/202040232openalex-snapshot
COALAS
inferred← citeshttps://doi.org/10.1051/0004-6361/202140612openalex-snapshot
Spectroscopic observations of PHz G237.01+42.50: A galaxy protocluster at z = 2.16 in the Cosmos field
inferred← citeshttps://doi.org/10.1051/0004-6361/202142255openalex-snapshot
Molecular gas properties of Planck-selected protocluster candidates at z ≃ 1.3–3
inferred← citeshttps://doi.org/10.1051/0004-6361/202142264openalex-snapshot
Atomic and molecular gas from the epoch of reionisation down to redshift 2
inferred← citeshttps://doi.org/10.1051/0004-6361/202142333openalex-snapshot
The 700 ks Chandra Spiderweb Field
inferred← citeshttps://doi.org/10.1051/0004-6361/202346444openalex-snapshot
The ALMA-ALPAKA survey
inferred← citeshttps://doi.org/10.1051/0004-6361/202348500openalex-snapshot
The RAdio Galaxy Environment Reference Survey (RAGERS)
inferred← citeshttps://doi.org/10.1051/0004-6361/202348659openalex-snapshot
ALMA survey of a massive node of the Cosmic Web at z ∼ 3
inferred← citeshttps://doi.org/10.1051/0004-6361/202450785openalex-snapshot
COALAS
inferred← citeshttps://doi.org/10.1051/0004-6361/202452179openalex-snapshot
X-ray view of a massive node of the Cosmic Web at z ∼ 3
inferred← citeshttps://doi.org/10.1051/0004-6361/202453238openalex-snapshot
An ALMA spectroscopic survey of the Planck high-redshift object PLCK G073.4−57.5 confirms two protoclusters
inferred← citeshttps://doi.org/10.1051/0004-6361/202553926openalex-snapshot
Gas properties as a function of environment in the proto-supercluster Hyperion at z ∼ 2.45
inferred← citeshttps://doi.org/10.1051/0004-6361/202555372openalex-snapshot
Insights on metal enrichment and environmental effects at z ≈ 5–7 with JWST ASPIRE/EIGER and the chemical evolution model
inferred← citeshttps://doi.org/10.1051/0004-6361/202659613openalex-snapshot
Strong environmental active galactic nuclei enhancement among dusty star-forming galaxies in z > 2 protoclusters
inferred← citeshttps://doi.org/10.1093/mnras/staa1275openalex-snapshot
Megaparsec-scale structure around the proto-cluster core SPT2349$-$56 at $z\,{=}\,4.3$
inferred← citeshttps://doi.org/10.1093/mnras/staa2015openalex-snapshot
The formation of ultradiffuse galaxies in the RomulusC galaxy cluster simulation
inferred← citeshttps://doi.org/10.1093/mnras/staa2872openalex-snapshot
The H α star formation main sequence in cluster and field galaxies at z ∼ 1.6
inferred← citeshttps://doi.org/10.1093/mnras/staa3662openalex-snapshot
Molecular hydrogen in IllustrisTNG galaxies: carefully comparing signatures of environment with local CO and SFR data
inferred← citeshttps://doi.org/10.1093/mnras/staa3693openalex-snapshot
Is there enough star formation in simulated protoclusters?
inferred← citeshttps://doi.org/10.1093/mnras/staa541openalex-snapshot
Rapid early coeval star formation and assembly of the most-massive galaxies in the Universe
inferred← citeshttps://doi.org/10.1093/mnras/stab3539openalex-snapshot
Rapid build-up of the stellar content in the protocluster core SPT2349−56 at z = 4.3
inferred← citeshttps://doi.org/10.1093/mnras/stab852openalex-snapshot
Resolving discs and mergers in z ∼ 2 heavily reddened quasars and their companion galaxies with ALMA
inferred← citeshttps://doi.org/10.1093/mnras/stac2784openalex-snapshot
Signs of environmental effects on star-forming galaxies in the Spiderweb protocluster at z = 2.16
inferred← citeshttps://doi.org/10.1093/mnras/stad1587openalex-snapshot
The relationship between cluster environment and molecular gas content of star-forming galaxies in the eagle simulation
inferred← citeshttps://doi.org/10.1093/mnras/stad3805openalex-snapshot
Enhanced star formation and metallicity deficit in the USS 1558−003 forming protocluster at z = 2.53
inferred← citeshttps://doi.org/10.1093/mnras/stae1155openalex-snapshot
A dusty protocluster surrounding the binary galaxy HerBS-70 at z = 2.3
inferred← citeshttps://doi.org/10.1093/mnras/stae118openalex-snapshot
New insights into the role of AGNs in forming the cluster red sequence
inferred← citeshttps://doi.org/10.1093/mnras/stae279openalex-snapshot
Star formation efficiency across large-scale galactic environments
inferred← citeshttps://doi.org/10.1093/mnras/stag858openalex-snapshot
Spider-Webb: enhanced star formation in low-mass galaxies within the Spiderweb protocluster revealed by JWST Pa β narrow-band imaging
inferred← citeshttps://doi.org/10.1093/pasj/psag120openalex-snapshot
ADF22-WEB: Massive galaxy formation shaped by cosmic web filaments in the z = 3.1 proto-cluster core
inferred← citeshttps://doi.org/10.1146/annurev-astro-082812-141034openalex-snapshot
The Evolution of the Star-Forming Interstellar Medium Across Cosmic Time
inferred← citeshttps://doi.org/10.3390/universe8110554openalex-snapshot
From Clusters to Proto-Clusters: The Infrared Perspective on Environmental Galaxy Evolution
inferred← citeshttps://doi.org/10.3847/1538-4357/ab3392openalex-snapshot
Large Molecular Gas Reservoirs in Star-forming Cluster Galaxies
inferred← citeshttps://doi.org/10.3847/1538-4357/ab3b5bopenalex-snapshot
A Radio-to-millimeter Census of Star-forming Galaxies in Protocluster 4C 23.56 at z = 2.5: Global and Local Gas Kinematics
inferred← citeshttps://doi.org/10.3847/1538-4357/ab5302openalex-snapshot
On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Protoclusters at z ≈ 2.0–2.5
inferred← citeshttps://doi.org/10.3847/1538-4357/ab75c3openalex-snapshot
Spectroscopic Confirmation of a Coma Cluster Progenitor at z ∼ 2.2
inferred← citeshttps://doi.org/10.3847/1538-4357/ab9d1fopenalex-snapshot
Emergence of an Ultrared, Ultramassive Galaxy Cluster Core at z = 4
inferred← citeshttps://doi.org/10.3847/1538-4357/abdbb5openalex-snapshot
Revisited Cold Gas Content with Atomic Carbon [C i] in z = 2.5 Protocluster Galaxies
inferred← citeshttps://doi.org/10.3847/1538-4357/abf4e6openalex-snapshot
Comprehensive Gas Characterization of a z = 2.5 Protocluster: A Cluster Core Caught in the Beginning of Virialization?
inferred← citeshttps://doi.org/10.3847/1538-4357/abfc50openalex-snapshot
Interrelation of the Environment of Lyα Emitters and Massive Galaxies at 2 < z < 4.5
inferred← citeshttps://doi.org/10.3847/1538-4357/ac0435openalex-snapshot
Molecular Gas in a Gravitationally Lensed Galaxy Group at z = 2.9
inferred← citeshttps://doi.org/10.3847/1538-4357/ac34faopenalex-snapshot
The Environmental Dependence of Gas Properties in Dense Cores of a Protocluster at z ∼ 2.5 Revealed with ALMA
inferred← citeshttps://doi.org/10.3847/1538-4357/ac48f6openalex-snapshot
Significant Molecular Gas Deficiencies in Star-forming Cluster Galaxies at z ∼ 1.4
inferred← citeshttps://doi.org/10.3847/1538-4357/ac58faopenalex-snapshot
ALMA Measures Molecular Gas Reservoirs Comparable to Field Galaxies in a Low-mass Galaxy Cluster at z = 1.3
inferred← citeshttps://doi.org/10.3847/1538-4357/ac6cdcopenalex-snapshot
High-resolution ALMA Study of CO J = 2–1 Line and Dust Continuum Emissions in Cluster Galaxies at z = 1.46
inferred← citeshttps://doi.org/10.3847/1538-4357/ac9d96openalex-snapshot
COSMOS2020: Identification of High-z Protocluster Candidates in COSMOS
inferred← citeshttps://doi.org/10.3847/1538-4357/acae96openalex-snapshot
A Large-scale Kinematic Study of Molecular Gas in High-z Cluster Galaxies: Evidence for High Levels of Kinematic Asymmetry
inferred← citeshttps://doi.org/10.3847/1538-4357/aced47openalex-snapshot
NeutralUniverseMachine: An Empirical Model for the Evolution of H i and H2 Gas in the Universe
inferred← citeshttps://doi.org/10.3847/1538-4357/ad7bb4openalex-snapshot
Kinematic Analysis of z = 4.3 Galaxies in the SPT2349–56 Protocluster Core
inferred← citeshttps://doi.org/10.3847/1538-4357/ad8156openalex-snapshot
JWST/NIRCam Paβ Narrowband Imaging Reveals Ordinary Dust Extinction for Hα Emitters within the Spiderweb Protocluster at z = 2.16
inferred← citeshttps://doi.org/10.3847/1538-4357/ad8dcfopenalex-snapshot
Revealing the Quiescent Galaxy Population in the Spiderweb Protocluster at z = 2.16 with Deep HST/WFC3 Slitless Spectroscopy
inferred← citeshttps://doi.org/10.3847/1538-4357/adff7dopenalex-snapshot
A Multiwavelength Study of ELAN Environments (AMUSE 2 ): The Impact of Dense Environment on Massive Dusty Star-forming Galaxies at Cosmic Noon
inferred← citeshttps://doi.org/10.3847/1538-4357/ae160dopenalex-snapshot
The Photometric Analysis of the Environment Around Two Dusty Star-forming Galaxies at z ∼ 2
inferred← citeshttps://doi.org/10.3847/1538-4357/ae3003openalex-snapshot
Spider-webb: Spatially Resolved Evidence of Inside-out Quenching in the Spiderweb Protocluster at z ∼ 2
inferred← citeshttps://doi.org/10.3847/1538-4357/ae3c06openalex-snapshot
Environment and Gas Fraction in Type 2 AGN versus Non-AGN Galaxies
inferred← citeshttps://doi.org/10.3847/1538-4357/ae87a1openalex-snapshot
BEACON: JWST NIRCam Pure-parallel Imaging Survey. IV. A Systematic Search for Galaxy Overdensities and Evidence for Gas Accretion Mode Transition
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