activity
19932023
most citedThe afterglow, the redshift, and the extreme energetics of the gamma-ray burst 990123

424 citations · 4.6k across the 90 of their papers we have counts for

collaborators

89 papers

astro-ph.GA2023★ 27 cited

Elentári: A Proto-Supercluster in COSMOS

Ben Forrest, Brian C. Lemaux, Ekta Shah +25

Motivated by spectroscopic confirmation of three overdense regions in the COSMOS field at , we analyze the uniquely deep multi-wavelength photometry and extensive spectr…

astro-ph.GA2022★ 37 cited

Investigating the Effect of Galaxy Interactions on Star Formation at 0.5<z<3.0

Ekta A. Shah, Jeyhan S. Kartaltepe, Christina T. Magagnoli +24

Observations and simulations of interacting galaxies and mergers in the local universe have shown that interactions can significantly enhance the star formation rates (SFR) and fue…

astro-ph.GA2022★ 35 cited

MAGAZ3NE: High Stellar Velocity Dispersions for Ultra-Massive Quiescent Galaxies at

Ben Forrest, Gillian Wilson, Adam Muzzin +17

In this work we publish stellar velocity dispersions, sizes, and dynamical masses for 8 ultra-massive galaxies (UMGs; log(/M, ) from the Massive Ancient Ga…

astro-ph.GA2022★ 3 cited

The ALPINE-ALMA [CII] survey: The infrared-radio correlation and AGN fraction of star-forming galaxies at z 4.4-5.9

Lu Shen, Brian C. Lemaux, Lori M. Lubin +26

We present the radio properties of 66 spectroscopically-confirmed normal star-forming galaxies (SFGs) at in the COSMOS field that were [C II] detected in the Atacama La…

astro-ph.GA2022★ 15 cited

The ALPINE-ALMA [CII] Survey: Investigation of 10 Galaxies at with [OII] and [CII] Line Emission ISM Properties and [OII]SFR Relation

Brittany N. Vanderhoof, A. L. Faisst, L. Shen +23

We present main-sequence ALPINE galaxies (log() = 9.2-11.1 and ) at with optical [OII] measurements from Ke…

astro-ph.GA2021★ 26 cited

Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z3.3

Lu Shen, Brian C. Lemaux, Lori M. Lubin +15

Radio Active Galactic Nuclei (RAGNs) are mainly found in dense structures (i.e., clusters/groups) at redshifts of z2 and are commonly used to detect protoclusters at higher reds…