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Ben Forrest

0000-0001-6003-0541
astro-ph.GAastro-ph.CO

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published · living versions
W_jhxkcpxw·v1 · currentpublished
The HST-Hyperion Survey: X-ray AGN Enhancement in the Hyperion Proto-supercluster
with Ashlen Coburn, Finn Giddings, Derek Sikorski, Roy Gal +16
1 version

Preprints & journals

51 papers in the corpus · 2016–2026
The GOGREEN Survey: AI Powered Deconvolution Lifts The Veil on Outside-in Environmental Quenching at z > 12609.01903v1 · Aurelien Henry, Gillian Wilson, Gregory Rudnick et al.2026 · 0 citationsarXiv
Cluster vs Field: Clear Evidence for a Morphology-Density Relation in All Environments at z∼1.6z\sim1.62606.26252v1 · Westley Brown, Adam Muzzin, Jasleen Matharu et al.2026 · 0 citationsarXiv
Strong environmental AGN enhancement among DSFGs in z > 2 protoclusters2606.05283v1 · Monica Natalia Isla Llave, Fabio Vito, Alberto Traina et al.2026 · 0 citationsarXiv
Metal-Poor Gas Accretion Drives Giant Clump Formation at 0.6 < z < 2.62606.05284v1 · Visal Sok, Adam Muzzin, Ben Forrest et al.2026 · 0 citationsarXiv
Toward Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-Early Star Formation Tensions2606.02698v3 · Sam E. Cutler, Luke Robbins, Danilo Marchesini et al.2026 · 0 citationsThe Astrophysical Journal Letters Volume 1008 (2026) L11
MAGAZ3NE: Spatially Resolved Ages and Chemical Abundances of Ultra-Massive Quiescent Galaxies at z ∼\sim 3.5 using JWST/NIRSpec IFU2605.27555v1 · Adit H. Edward, Jacqueline Antwi-Danso, Adam Muzzin et al.2026 · 0 citationsarXiv
MAGAZ3NE: Dust Deficiency in Ultramassive Quiescent Galaxies at 3<z<43<z<4 with ALMA Observations2601.22844v1 · Wenjun Chang, Gillian Wilson, Ben Forrest et al.2026 · 0 citationsarXiv
The HST-Hyperion Survey: Environmental Imprints on the Stellar-Mass Function at z~2.52509.02714v2 · Derek Sikorski, Ben Forrest, Brian C. Lemaux et al.2025 · 2 citationsA&A 708, A114 (2026)
A massive and evolved slow-rotating galaxy in the early Universe2508.10987v2 · Ben Forrest, Adam Muzzin, Danilo Marchesini et al.2025 · 1 citationarXiv
MAGAZ3NE: Far-IR and Radio Insights into the Nature and Properties of Ultramassive Galaxies at z≳3z\gtrsim32508.08460v1 · Wenjun Chang, Gillian Wilson, Ben Forrest et al.2025 · 0 citationsarXiv
Excavating The Ruins: an Ancient z=2.675z=2.675 Galaxy Which Formed in the First 500 Myr2508.05752v1 · Ian McConachie, Jacqueline Antwi-Danso, Wenjun Chang et al.2025 · 1 citationarXiv
CANUCS/Technicolor Data Release 1: Imaging, Photometry, Slit Spectroscopy, and Stellar Population Parameters2506.21685v1 · Ghassan T. E. Sarrouh, Yoshihisa Asada, Nicholas S. Martis et al.2025 · 22 citationsarXiv
Distinct origins of environmentally quenched galaxies in the core and outer virialised regions of massive clusters at 0.8<z<1.50.8<z<1.52506.06434v1 · Guillaume Hewitt, Florian Sarron, Michael L. Balogh et al.2025 · 0 citationsarXiv
Insights into environmental quenching at z∼1z\sim1: an enhancement of faint, low-mass passive galaxies in clusters2504.12394v1 · Harry Gully, Nina Hatch, Syeda Lammim Ahad et al.2025 · 4 citationsarXiv
Gas properties as a function of environment in the proto-supercluster Hyperion at z ~ 2.452504.08894v1 · G. Gururajan, O. Cucciati, B. C. Lemaux et al.2025 · 7 citationsA&A 698, A312 (2025)
Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation2504.03836v3 · Devontae C. Baxter, Alison L. Coil, Ethan O. Nadler et al.2025 · 5 citationsApJ, 990, 225 (2025)
MAGAZ3NE: Evidence for Galactic Conformity in z≳3z\gtrsim3 Protoclusters2411.14641v1 · Ian McConachie, Gillian Wilson, Ben Forrest et al.2024 · 0 citationsarXiv
Discovering Large-Scale Structure at 2<z<52<z<5 in the C3VO Survey2410.00237v2 · Denise Hung, Brian C. Lemaux, Olga Cucciati et al.2024 · 14 citationsApJ 980 155 (2025)
Enhanced AGN Activity in Overdense Galactic Environments at 2<z<42 < z < 42409.02996v1 · Ekta A. Shah, Brian C. Lemaux, Benjamin Forrest et al.2024 · 6 citationsA&A 704, A101 (2025)
Environmental Effects on the Stellar Mass Function in a z~3.3 Overdensity of Galaxies in the COSMOS Field2405.18491v2 · Ben Forrest, Brian C. Lemaux, Ekta A. Shah et al.2024 · 22 citationsarXiv
MOSEL survey: Unwrapping the Epoch of Reionization through mimic galaxies at Cosmic Noon2405.04870v1 · Ravi Jaiswar, Anshu Gupta, Elisabete da Cunha et al.2024 · 0 citationsarXiv
MAGAZ3NE: Massive, Extremely Dusty Galaxies at z∼2z\sim2 Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at 3<z<43<z<42404.19018v2 · Ben Forrest, M. C. Cooper, Adam Muzzin et al.2024 · 10 citationsarXiv
Spectroscopic Confirmation of an Ultra-Massive Galaxy in a Protocluster at z∼4.9z \sim 4.92404.16036v3 · Stephanie M. Urbano Stawinski, M. C. Cooper, Ben Forrest et al.2024 · 20 citationsarXiv
MOSEL survey: Spatially offset Lyman-continuum emission in a new emitter at z=3.0882403.13285v1 · Anshu Gupta, Cathryn M. Trott, Ravi Jaiswar et al.2024 · 0 citationsarXiv
The first quenched galaxies, when and how?2402.01314v2 · Lizhi Xie, Gabriella De Lucia, Fabio Fontanot et al.2024 · 36 citationsarXiv
The stellar mass function of quiescent galaxies in 2 < z < 2.5 protoclusters2312.12380v1 · Adit H. Edward, Michael L. Balogh, Yannick M. Bahe et al.2023 · 18 citationsarXiv
Protoclusters as Drivers of Stellar Mass Growth in the Early Universe, a Case Study: Taralay -- a Massive Protocluster at z ~ 4.572312.11465v1 · Priti Staab, Brian C. Lemaux, Ben Forrest et al.2023 · 22 citationsarXiv
Identification and Characterization of Six Spectroscopically Confirmed Massive Protostructures at 2.5<z<4.52.5<z<4.52312.04634v1 · Ekta A. Shah, Brian Lemaux, Benjamin Forrest et al.2023 · 17 citationsarXiv
MOSEL survey: JWST reveals major mergers/strong interactions drive the extreme emission lines in the early universe2311.02158v1 · Anshu Gupta, Ravi Jaiswar, Vicente Rodriguez-Gomez et al.2023 · 11 citationsThe Astrophysical Journal Letters, 2023
Elentári: A z∼3.3z\sim3.3 Proto-Supercluster in COSMOS2307.15113v1 · Ben Forrest, Brian C. Lemaux, Ekta Shah et al.2023 · 27 citationsarXiv
When the Well Runs Dry: Modeling Environmental Quenching of High-mass Satellites in Massive Clusters at \boldmathz≳1z \gtrsim 12306.09404v2 · Devontae C. Baxter, Michael C. Cooper, Michael L. Balogh et al.2023 · 16 citationsMonthly Notices of the Royal Astronomical Society, Volume 526, Issue 3, December 2023
MOSEL Survey: Extremely weak outflows in EoR analogues at z=3-42211.13763v1 · Anshu Gupta, Kim-Vy Tran, Trevor Mendel et al.2022 · 11 citationsarXiv
MAGAZ3NE: High Stellar Velocity Dispersions for Ultra-Massive Quiescent Galaxies at z≳3z\gtrsim32208.04329v1 · Ben Forrest, Gillian Wilson, Adam Muzzin et al.2022 · 36 citationsarXiv
The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z ∼\sim 4.4-5.92207.07137v1 · Lu Shen, Brian C. Lemaux, Lori M. Lubin et al.2022 · 3 citationsarXiv
Spectroscopic Confirmation of a Protocluster at z=3.37z=3.37 with a High Fraction of Quiescent Galaxies2109.07696v2 · Ian McConachie, Gillian Wilson, Ben Forrest et al.2021 · 96 citationsarXiv
The GOGREEN survey: Transition Galaxies and The Evolution of Environmental Quenching2109.03105v1 · Karen McNab, Michael L. Balogh, Remco F. J. van der Burg et al.2021 · 34 citationsarXiv
The GOGREEN Survey: Evidence of an excess of quiescent disks in clusters at 1.0<z<1.41.0<z<1.42107.03403v1 · Jeffrey C.C. Chan, Gillian Wilson, Michael Balogh et al.2021 · 12 citationsarXiv
The Number Densities and Stellar Populations of Massive Galaxies at 3 < z < 6: A Diverse, Rapidly Forming Population in the Early Universe2010.04725v1 · Z. Cemile Marsan, Adam Muzzin, Danilo Marchesini et al.2020 · 34 citationsarXiv
The GOGREEN and GCLASS Surveys: First Data Release2009.13345v1 · Michael L. Balogh, Remco F. J. van der Burg, Adam Muzzin et al.2020 · 48 citationsarXiv
The Hα\alpha star formation main sequence in cluster and field galaxies at z∼1.6z\sim1.62009.07861v1 · Julie Nantais, Gillian Wilson, Adam Muzzin et al.2020 · 15 citationsarXiv
The GOGREEN survey: Post-infall environmental quenching fails to predict the observed age difference between quiescent field and cluster galaxies at z>12009.03953v1 · Kristi Webb, Michael L. Balogh, Joel Leja et al.2020 · 51 citationsarXiv
MOSEL: Strong [OIII]5007 Å\ Emitting Galaxies at (3<z<4) from the ZFOURGE Survey2004.13079v1 · Kim-Vy H. Tran, Ben Forrest, Leo Y. Alcorn et al.2020 · 24 citationsarXiv
The GOGREEN survey: The environmental dependence of the star-forming galaxy main sequence at 1.0<z<1.51.0<z<1.52002.11735v3 · Lyndsay J. Old, Michael. L. Balogh, Remco F. J van der Burg et al.2020 · 66 citationsarXiv
An Extremely Massive Quiescent Galaxy at z=3.493z=3.493: Evidence of Insufficiently Rapid Quenching Mechanisms in Theoretical Models1910.10158v1 · Ben Forrest, Marianna Annunziatella, Gillian Wilson et al.2019 · 100 citationsarXiv
ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1<z<41807.03785v1 · Ben Forrest, Kim-Vy H. Tran, Adam Broussard et al.2018 · 37 citationsarXiv
A Low Lyman Continuum Escape Fraction of <10%<10\% for Extreme [OIII] Emitters in an Overdensity at z∼3.5\sim3.51804.06845v1 · Rohan P. Naidu, Ben Forrest, Pascal A. Oesch et al.2018 · 74 citationsarXiv
ZFIRE: 3D Modeling of Rotation, Dispersion, and Angular Momentum of Star-Forming Galaxies at z~21804.03669v1 · Leo Y. Alcorn, Kim-Vy Tran, Karl Glazebrook et al.2018 · 21 citationsarXiv
The Effects of Environment on the Evolution of the Galaxy Stellar Mass Function1801.04934v1 · Casey Papovich, Lalitwadee Kawinwanichakij, Ryan Quadri et al.2018 · 78 citationsarXiv
Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.51710.04225v1 · Michael J. Cowley, Lee R. Spitler, Ryan F. Quadri et al.2017 · 5 citationsarXiv
Discovery of Extreme [OIII]+Hβ\beta Emitting Galaxies Tracing an Overdensity at z~3.5 in CDF-South1703.03814v1 · Ben Forrest, Kim-Vy H. Tran, Adam Broussard et al.2017 · 47 citationsarXiv
Career total: 78 works. 51 are in this corpus.Showing the 50 most recent.

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