activity
19962023
most citedThe Second Data Release of the Sloan Digital Sky Survey

1.2k citations · 3.4k across the 64 of their papers we have counts for

collaborators

64 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★ 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…

astro-ph.CO2021★ 12 cited

An Optical Observational Cluster Mass Function at with the ORELSE Survey

D. Hung, B. C. Lemaux, R. R. Gal +11

We present a new mass function of galaxy clusters and groups using optical/near-infrared wavelength spectroscopic and photometric data from the Observations of Redshift Evolution i…

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…