activity
20172026
most citedPHIBSS: Unified Scaling Relations of Gas Depletion Time and Molecular Gas Fractions

642 citations · 723 across the 20 of their papers we have counts for

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Showing 2024Show all

8 papers · 1 filter

astro-ph.GA2024

MAGAZ3NE: Evidence for Galactic Conformity in Protoclusters

Ian McConachie, Gillian Wilson, Ben Forrest +16

We examine the quiescent fractions of massive galaxies in six spectroscopically-confirmed protoclusters in the COSMOS field, one of which is newly confirmed and present…

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.GA2024★ 9 cited

MAGAZ3NE: Massive, Extremely Dusty Galaxies at Lead to Photometric Overestimation of Number Densities of the Most Massive Galaxies at

Ben Forrest, M. C. Cooper, Adam Muzzin +17

We present rest-frame optical spectra from Keck/MOSFIRE and Keck/NIRES of 16 candidate ultramassive galaxies targeted as part of the Massive Ancient Galaxies at Near-Infrared…

astro-ph.GA2024★ 20 cited

Spectroscopic Confirmation of an Ultra-Massive Galaxy in a Protocluster at

Stephanie M. Urbano Stawinski, M. C. Cooper, Ben Forrest +8

We present spectroscopic confirmation of an ultra-massive galaxy (UMG) with at in the Extended Groth Strip (EGS)…

astro-ph.GA2024

Resolved UV and optical color gradients reveal environmental influence on galaxy evolution at redshift z1.6

William J. Cramer, A. G. Noble, G. Rudnick +13

The changes in colors across a galaxy are intimately connected to the galaxy's formation, growth, quenching history, and dust content. A particularly important epoch in the growth…

astro-ph.GA2024★ 1 cited

The first quenched galaxies, when and how?

Lizhi Xie, Gabriella De Lucia, Fabio Fontanot +11

Many quiescent galaxies discovered in the early Universe by \textit{JWST} raise fundamental questions on when and how these galaxies became and stayed quenched. Making use of the l…

astro-ph.CO2024

LoVoCCS. II. Weak Lensing Mass Distributions, Red-Sequence Galaxy Distributions, and Their Alignment with the Brightest Cluster Galaxy in 58 Nearby X-ray-Luminous Galaxy Clusters

Shenming Fu, Ian Dell'Antonio, Zacharias Escalante +31

The Local Volume Complete Cluster Survey (LoVoCCS) is an on-going program to observe nearly a hundred low-redshift X-ray-luminous galaxy clusters (redshifts and X-ray…

astro-ph.GA2024★ 6 cited

-selected protocluster candidates in the LSST Deep Drilling Fields

Harry Gully, Nina Hatch, Yannick Bahé +8

We have identified 189 candidate protoclusters and clusters in the LSST Deep Drilling Fields. This sample will enable the measurement of the metal enrichment and star for…