159 citations · 1.1k across the 29 of their papers we have counts for
6 papers · 1 filter
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.…
Deep CO(1-0) Observations of z=1.62 Cluster Galaxies with Substantial Molecular Gas Reservoirs and Normal Star Formation Efficiencies
Gregory Rudnick, Jacqueline Hodge, Fabian Walter +9
We present an extremely deep CO(1-0) observation of a confirmed galaxy cluster. We detect two spectroscopically confirmed cluster members in CO(1-0) with . Both gal…
The Ages of Passive Galaxies in a z=1.62 Protocluster
Donald B. Lee-Brown, Gregory H. Rudnick, Ivelina G. Momcheva +9
We present a study of the relation between galaxy stellar age and mass for 14 members of the protocluster IRC 0218, using multiband imaging and HST G102 and G141 grism spe…
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…
Survival of Massive Star-forming Galaxies in Cluster Cores Drives Gas-Phase Metallicity Gradients : The Effects of Ram Pressure Stripping
Anshu Gupta, Tiantian Yuan, Davide Martizzi +2
Recent observations of galaxies in a cluster at z=0.35 show that their integrated gas-phase metallicities increase with decreasing cluster-centric distance. To test if ram pressure…
SG1120-1202: Mass-Quenching as Tracked by UV Emission in the Group Environment at z=0.37
Jonathan T. Monroe, Kim-Vy H. Tran, Anthony H. Gonzalez
We use the Hubble Space Telescope to obtain WFC3/F390W imaging of the supergroup SG1120-1202 at z=0.37, mapping the UV emission of 138 spectroscopically confirmed members. We measu…