1k citations · 9.6k across the 67 of their papers we have counts for
67 papers
CLEAR I: Ages and Metallicities of Quiescent Galaxies at Derived from Deep Hubble Space Telescope Grism Data
Vicente Estrada-Carpenter, Casey Papovich, Ivelina Momcheva +14
We use deep \textit{Hubble Space Telescope} spectroscopy to constrain the metallicities and (\editone{light-weighted}) ages of massive () galaxies sel…
The Effects of Environment on the Evolution of the Galaxy Stellar Mass Function
Casey Papovich, Lalitwadee Kawinwanichakij, Ryan Quadri +8
We study the effects of galaxy environment on the evolution of the stellar-mass function (SMF) over 0.2 < z < 2.0 using the FourStar Galaxy Evolution (ZFOURGE) survey and NEWFIRM M…
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.…
Effect of local environment and stellar mass on galaxy quenching and morphology at
Lalitwadee Kawinwanichakij, Casey Papovich, Ryan F. Quadri +20
We study galactic star-formation activity as a function of environment and stellar mass over 0.5<z<2.0 using the FourStar Galaxy Evolution (ZFOURGE) survey. We estimate the galaxy…
A comparison of the most massive quiescent galaxies from to the present: slow evolution in size, and spheroid-dominated
Shannon G. Patel, Yu Xuan Hong, Ryan F. Quadri +2
We use Hubble Space Telescope imaging to study the structural properties of ten of the most massive ( Msun) quiescent galaxies (QGs) in the UKIDSS UDS at $2.5<z<…
Discovery of Extreme [OIII]+H Emitting Galaxies Tracing an Overdensity at z~3.5 in CDF-South
Ben Forrest, Kim-Vy H. Tran, Adam Broussard +12
Using deep multi-wavelength photometry of galaxies from ZFOURGE, we group galaxies at by the shape of their spectral energy distributions (SEDs). We identify a populati…