D. Hung

activity

20182025

most citedConditional Quenching: A detailed look at the SFR-Density Relation at z ~ 0.9 from ORELSE

41 citations · 114 across the 17 of their papers we have counts for

collaborators

Showing 2021Show all

2 papers · 1 filter

astro-ph.GA2021

Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z $\sim$ 3.3

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 z $<$ 2 and are commonly used to detect protoclusters at higher reds…

astro-ph.CO2021★ 12 cited

An Optical Observational Cluster Mass Function at $z \sim 1$ 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…

Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z∼3.3

An Optical Observational Cluster Mass Function at z∼1 with the ORELSE Survey

Implications of the Environments of Radio-detected AGN in a Complex Protostructure at z $\sim$ 3.3

An Optical Observational Cluster Mass Function at $z \sim 1$ with the ORELSE Survey