75 citations · 173 across the 5 of their papers we have counts for
9 papers
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…
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…
Reconstructing the observed ionizing photon production efficiency at z~2 using stellar population models
Themiya Nanayakkara, Jarle Brinchmann, Karl Glazebrook +8
The ionizing photon production efficiency, , is a critical parameter that provides a number of physical constraints to the nature of the early Universe, including the cont…
ZFOURGE: Using Composite Spectral Energy Distributions to Characterize Galaxy Populations at 1<z<4
Ben Forrest, Kim-Vy H. Tran, Adam Broussard +12
We investigate the properties of galaxies as they shut off star formation over the 4 billion years surrounding peak cosmic star formation. To do this we categorize galax…
ZFIRE: 3D Modeling of Rotation, Dispersion, and Angular Momentum of Star-Forming Galaxies at z~2
Leo Y. Alcorn, Kim-Vy Tran, Karl Glazebrook +10
We perform a kinematic and morphological analysis of 44 star-forming galaxies at in the COSMOS legacy field using near-infrared spectroscopy from Keck/MOSFIRE and F160W im…
Decoupled Black Hole Accretion and Quenching: The Relationship Between BHAR, SFR, and Quenching in Milky Way and Andromeda-mass Progenitors Since z = 2.5
Michael J. Cowley, Lee R. Spitler, Ryan F. Quadri +13
We investigate the relationship between the black hole accretion rate (BHAR) and star-formation rate (SFR) for Milky Way (MW) and Andromeda (M31)-mass progenitors from z = 0.2 - 2.…