activity
20162021
most citedGalaxy Merger Fractions in Two Clusters at Using the Hubble Space Telescope

36 citations · 96 across the 6 of their papers we have counts for

collaborators

12 papers

astro-ph.GA20214 cited

ZFIRE: The Beginning of the End for Massive Galaxies at z ~ 2 and Why Environment Matters

Anishya Harshan, Anshu Gupta, Kim-Vy Tran +6

We use ZFIRE and ZFOURGE observations with the Spectral Energy Distribution (SED) fitting tool Prospector to reconstruct the star formation histories (SFHs) of proto-cluster and fi…

astro-ph.GA202113 cited

SITELLE Hα Imaging Spectroscopy of z~0.25 Clusters: Emission Line Galaxy Detection and Ionized Gas Offset in Abell 2390 & Abell 2465

Qing Liu, Howard Yee, Laurent Drissen +9

Environmental effects are crucial to the understanding of the evolution of galaxies in dense environments, such as galaxy clusters. Using the large field-of-view of SITELLE, the un…

astro-ph.GA202014 cited

A giant galaxy in the young Universe with a massive ring

Tiantian Yuan, Ahmed Elagali, Ivo Labbe +12

In the local (redshift z~0) Universe, collisional ring galaxies make up only ~0.01% of galaxies and are formed by head-on galactic collisions that trigger radially propagating dens…

astro-ph.GA202024 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…

astro-ph.GA2020

MOSEL Survey: Tracking the Growth of Massive Galaxies at 2<z<4 using Kinematics and the IllustrisTNG Simulation

Anshu Gupta, Kim-Vy Tran, Jonathan Cohn +13

We use K-band spectroscopic data from the Multi-Object Spectroscopic Emission Line (MOSEL) survey to analyze the kinematic properties of galaxies at z>3. Our sample consists of 34…

astro-ph.GA2020

ZFIRE: Measuring Electron Density with [OII] as a function of environment at z = 1.62

Anishya Harshan, Anshu Gupta, Kim-Vy Tran +8

The global star formation rates (SFR) of galaxies at fixed stellar masses increase with redshift and are known to vary with environment unto z~2. We explore here whether the change…