activity
20112021
most citedGalaxy Stellar Mass Functions from ZFOURGE/CANDELS: An Excess of Low-Mass Galaxies Since z=2 and the Rapid Buildup of Quiescent Galaxies

460 citations · 3k across the 47 of their papers we have counts for

collaborators

47 papers

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…

astro-ph.GA2020★ 70 cited

The VIMOS Ultra Deep Survey: The reversal of the star-formation rate density relation at

B. C. Lemaux, O. Cucciati, O. Le Fèvre +28

Utilizing spectroscopic observations taken for the VIMOS Ultra-Deep Survey (VUDS), new observations from Keck/DEIMOS, and publicly available observations of large samples of star-f…

astro-ph.GA2020★ 4 cited

Environmental impact on star-forming galaxies in a cluster during course of galaxy accretion

Tetsuro Asano, Tadayuki Kodama, Kentaro Motohara +18

Galaxies change their properties as they assemble into clusters. In order to understand the physics behind that, we need to go back in time and observe directly what is occurring i…

astro-ph.GA2020★ 24 cited

MOSEL: Strong [OIII]5007 Å Emitting Galaxies at (3<z<4) from the ZFOURGE Survey

Kim-Vy H. Tran, Ben Forrest, Leo Y. Alcorn +13

To understand how strong emission line galaxies (ELGs) contribute to the overall growth of galaxies and star formation history of the universe, we target Strong ELGs (SELGs) from t…