73 citations · 207 across the 6 of their papers we have counts for
8 papers
Bright z~9 Galaxies in Parallel: The Bright End of the Rest-UV Luminosity Function from HST Parallel Programs
Micaela B. Bagley, Steven L. Finkelstein, Sofía Rojas-Ruiz +7
The abundance of bright galaxies at z>8 can provide key constraints on models of galaxy formation and evolution, as the predicted abundance varies greatly when different physical p…
Texas Spectroscopic Search for Ly Emission at the End of Reionization III. the Ly Equivalent-width Distribution and Ionized Structures at
Intae Jung, Steven L. Finkelstein, Mark Dickinson +11
Ly emission from galaxies can be utilized to characterize the ionization state in the intergalactic medium (IGM). We report our search for Ly emission at using a compre…
The VIRUS-P Exploration of Nearby Galaxies (VENGA): The stellar populations and assembly of NGC 2903's bulge, bar, and outer disc
Andreia Carrillo, Shardha Jogee, Niv Drory +5
We study the stellar populations and assembly of the nearby spiral galaxy NGC 2903's bulge, bar, and outer disc using the VIRUS-P Exploration of Nearby Galaxies IFS survey. We obse…
Near-Infrared Spectroscopy of Galaxies During Reionization: Measuring CIII] in a Galaxy at
Taylor A. Hutchison, Casey Papovich, Steven L. Finkelstein +9
We present Keck/MOSFIRE -band spectroscopy targeting CIII] 1907,1909 in a galaxy previously identified via Ly emission. We detect strong line emission at $1…
Texas Spectroscopic Search for Ly Emission at the End of Reionization II. The Deepest Near-Infrared Spectroscopic Observation at
Intae Jung, Steven L. Finkelstein, Mark Dickinson +12
Realizing the utility of Ly emission to trace the evolution of the intergalactic medium (IGM) during the epoch of reionization requires deep spectroscopy across the boundary of…
Texas Spectroscopic Search for Ly Emission at the End of Reionization I. Constraining the Ly Equivalent Width Distribution at 6.0 < < 7.0
Intae Jung, Steven L. Finkelstein, Rachael C. Livermore +6
The distribution of Ly emission is an presently accessible method for studying the state of the intergalactic medium (IGM) into the reionization era. We carried out deep spectro…