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20142025
most citedInspiraling streams of enriched gas observed around a massive galaxy 11 billion years ago

36 citations · 134 across the 19 of their papers we have counts for

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19 papers · 1 filter

astro-ph.GA2025★ 1 cited

Probing the influence of the protocluster environment on galaxy morphology at z = 2.23

Emmet Golden-Marx, Zheng Cai, Dongdong Shi +7

As galaxies evolve in dense cluster and protocluster environments, they interact and quench their star formation, which gradually transforms the galaxy population from star-forming…

astro-ph.GA2025★ 1 cited

The HST-Hyperion Survey: Environmental Imprints on the Stellar-Mass Function at z~2.5

Derek Sikorski, Ben Forrest, Brian C. Lemaux +19

Not all galaxies at Cosmic Noon evolve in the same way. It remains unclear how the local environment -- especially the extreme overdensities of protoclusters -- affects stellar mas…

astro-ph.GA2025

A 13-Billion-Year View of Galaxy Growth: Metallicity Gradient Evolution from the Local Universe to with JWST and Archival Surveys

Zihao Li, Zheng Cai, Xin Wang +25

The galaxy gas-phase metallicity gradients have been extensively studied over the past four decades, both in the local and high-redshift universe, as they trace the baryon cycle an…

astro-ph.GA2025★ 5 cited

Gas properties as a function of environment in the proto-supercluster Hyperion at z ~ 2.45

G. Gururajan, O. Cucciati, B. C. Lemaux +26

The cosmic star-formation rate density, molecular gas density and the AGN activity of the Universe peak at z~ 2-3, showing the Universe is most active at this epoch. The nature of…

astro-ph.GA2025★ 4 cited

Quantifying the Impact of Incompleteness on Identifying and Interpreting Galaxy Protocluster Populations with the TNG-Cluster Simulation

Devontae C. Baxter, Alison L. Coil, Ethan O. Nadler +7

We use the TNG-Cluster simulation to investigate how stellar mass and star formation rate (SFR) incompleteness affect the identification of density peaks within galaxy protocluster…

astro-ph.GA2025★ 3 cited

HST Grism Observations of a z~1.8 Cluster Candidate from the Clusters Occupied by Bent Radio AGN (COBRA) Survey

Courtney B. Watson, Elizabeth L. Blanton, Emmet Golden-Marx +4

We present new Hubble Space Telescope/Wide Field Camera 3 G141 grism observations for COBRA1411+3415, originally identified as a high-redshift cluster candidate in the Clusters Occ…

astro-ph.GA2025

The HST-Hyperion Survey: Grism Observations of a Proto-Supercluster

Ben Forrest, Lu Shen, Brian C. Lemaux +19

We present first results and catalogs from the HST-Hyperion survey. This survey has collected 50 orbits of WFC3/F160W imaging and WFC3/G141 grism spectroscopy in the most overdense…

astro-ph.GA2025★ 2 cited

The HST-Hyperion Survey: Companion Fraction and Overdensity in a z ~ 2.5 Proto-supercluster

F. Giddings, B. C. Lemaux, B. Forrest +22

We present a study of the galaxy merger and interaction activity within the Hyperion Proto-supercluster at z~2.5 in an effort to assess the occurrence of galaxy mergers and interac…

astro-ph.GA2024★ 13 cited

Discovering Large-Scale Structure at in the C3VO Survey

Denise Hung, Brian C. Lemaux, Olga Cucciati +23

The Charting Cluster Construction with VUDS and ORELSE (C3VO) survey is an ongoing imaging and spectroscopic campaign aiming to map out the growth of structure up to and w…

astro-ph.GA2024★ 2 cited

Enhanced AGN Activity in Overdense Galactic Environments at

Ekta A. Shah, Brian C. Lemaux, Benjamin Forrest +17

We conduct a study on the relationship between galaxy environments and their active galactic nuclei (AGN) activity at high redshifts (). Specifically, we study the AGN f…

astro-ph.GA2024

Environmental Effects on the Stellar Mass Function in a z~3.3 Overdensity of Galaxies in the COSMOS Field

Ben Forrest, Brian C. Lemaux, Ekta A. Shah +17

We present an analysis of the number density of galaxies as a function of stellar mass (i.e., the stellar mass function, SMF) in the COSMOS field at z~3.3, making a comparison betw…

astro-ph.GA2023★ 4 cited

Searching for [CII] Emission from the First Sample of OI Absorption-Associated Galaxies with ALMA

Yunjing Wu, Zheng Cai, Jianan Li +13

We report the first statistical analyses of [CII] and dust continuum observations in six strong OI absorber fields at the end of the reionization epoch obtained by the Atacama Larg…

astro-ph.GA2023

The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Investigating the Role of Environment on Bent Radio AGNs using LOFAR

Emmet Golden-Marx, Emily Moravec, Lu Shen +10

Bent radio AGN morphology depends on the density of the surrounding gas. However, bent sources are found inside and outside clusters, raising the question of how environment impact…

astro-ph.GA2023★ 36 cited

Inspiraling streams of enriched gas observed around a massive galaxy 11 billion years ago

Shiwu Zhang, Zheng Cai, Dandan Xu +19

Stars form in galaxies, from gas that has been accreted from the intergalactic medium. Simulations have shown that recycling of gas-the reaccretion of gas that was previously eject…

astro-ph.GA2021★ 19 cited

VLA resolves unexpected radio structures in the Perseus cluster of galaxies

Marie-Lou Gendron-Marsolais, Charles L. H. Hull, Rick Perley +10

We present new deep, high-resolution, 1.5 GHz observations of the prototypical nearby Perseus galaxy cluster from the Karl G. Jansky Very Large Array. We isolate for the first time…

astro-ph.GA2020★ 15 cited

The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Radio Source Properties

Emmet Golden-Marx, Elizabeth Blanton, Rachel-Paterno-Mahler +8

The shape of bent, double-lobed radio sources requires a dense gaseous medium. Bent sources can therefore be used to identify galaxy clusters and characterize their evolutionary hi…

astro-ph.GA2020★ 7 cited

Extended radio AGN at z ~ 1 in the ORELSE survey: The confining effect of dense environments

Lu Shen, Guilin Liu, Mengfei Zhang +16

Recent hydrodynamic simulations and observations of radio jets have shown that the surrounding environment has a large effect on their resulting morphology. To investigate this we…

astro-ph.GA2019★ 18 cited

The High-Redshift Clusters Occupied by Bent Radio AGN (COBRA) Survey: Follow-Up Optical Imaging

Emmet Golden-Marx, E. L. Blanton, R. Paterno-Mahler +6

Here we present new red sequence overdensity measurements for 77 fields in the high- Clusters Occupied by Bent Radio AGN (COBRA) survey, based on - and -band imaging taken…

astro-ph.GA2014★ 4 cited

Extragalactic Jets as Probes of Distant Clusters of Galaxies and the Clusters Occupied by Bent Radio AGN (COBRA) Survey

Elizabeth L. Blanton, Rachel Paterno-Mahler, Joshua D. Wing +6

We are conducting a large survey of distant clusters of galaxies using radio sources with bent jets and lobes as tracers. These radio sources are driven by AGN and achieve their be…