734 citations · 3.1k across the 27 of their papers we have counts for
28 papers
3D-Herschel: Constraining Dust Emission with Panchromatic Modeling of 3D-HST Galaxies
Seamus McNulty, Mimi Song, Katherine E. Whitaker +9
We present 3D-Herschel, a new publicly released 0.3-350m photometric catalog that combines deblended Herschel far-infrared (FIR) imaging with the CANDELS/3D-HST legacy fields to…
New Lyman-alpha Emitters in EGS: Evidence of an Extended Ionized Structure at
Intae Jung, Steven L. Finkelstein, Rebecca L. Larson +21
We perform a ground-based near-infrared spectroscopic survey using the Keck/MOSFIRE spectrograph to target Ly emission at from 61 galaxies to trace the ionization st…
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…
REQUIEM-2D: A diversity of formation pathways in a sample of spatially-resolved massive quiescent galaxies at z~2
Mohammad Akhshik, Katherine E. Whitaker, Joel Leja +16
REQUIEM-2D (REsolving QUIEscent Magnified galaxies with 2D grism spectroscopy) is comprised of a sample of 8 massive () strongly lensed quiescent galaxies…
Diagnosing DASH: A Catalog of Structural Properties for the COSMOS-DASH Survey
Sam E. Cutler, Katherine E. Whitaker, Lamiya A. Mowla +16
We present the morphological catalogs for the COSMOS-DASH survey, the largest area near-IR survey using HST-WFC3 to date. Utilizing the "Drift And SHift" observing techni…
On the Stellar Populations of Galaxies at z=9-11: The Growth of Metals and Stellar Mass at Early Times
Sandro Tacchella, Steven L. Finkelstein, Micaela Bagley +18
We present a detailed stellar population analysis of 11 bright () galaxies at (three spectroscopically confirmed) to constrain the chemical enrichment and growth o…
A Census of the Bright z=8.5-11 Universe with the Hubble and Spitzer Space Telescopes in the CANDELS Fields
Steven L. Finkelstein, Micaela Bagley, Mimi Song +21
We present the results from a new search for candidate galaxies at z ~ 8.5-11 discovered over the 850 arcmin^2 area probed by the Cosmic Assembly Near-Infrared Deep Extragalactic L…
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…
Evidence for Reduced Specific Star Formation Rates in the Centers of Massive Galaxies at z = 4
Intae Jung, Steven L. Finkelstein, Mimi Song +11
We perform the first spatially-resolved stellar population study of galaxies in the early universe (z = 3.5 - 6.5), utilizing the Hubble Space Telescope Cosmic Assembly Near-infrar…
The VIRUS-P Exploration of Nearby Galaxies (VENGA): Spatially Resolved Gas-Phase Metallicity Distributions in Barred and Unbarred Spirals
Kyle F. Kaplan, Shardha Jogee, Lisa Kewley +6
We present a study of the excitation conditions and metallicity of ionized gas (Z_gas) in eight nearby barred and unbarred spiral galaxies from the VIRUS-P Exploration of Nearby Ga…
Keck/MOSFIRE Spectroscopy of z=7-8 Galaxies: Ly Emission from a Galaxy at z=7.66
Mimi Song, Steven L. Finkelstein, Rachael C. Livermore +3
We report the results from some of the deepest Keck/Multi-Object Spectrometer For Infra-Red Exploration data yet obtained for candidate galaxies. Our data show one si…
The Evolution of the Galaxy Stellar Mass Function at z= 4-8: A Steepening Low-mass-end Slope with Increasing Redshift
Mimi Song, Steven L. Finkelstein, Matthew L. N. Ashby +16
We present galaxy stellar mass functions (GSMFs) at 4-8 from a rest-frame ultraviolet (UV) selected sample of 4500 galaxies, found via photometric redshifts over an area…
An Increasing Stellar Baryon Fraction in Bright Galaxies at High Redshift
Steven L. Finkelstein, Mimi Song, Peter Behroozi +12
Recent observations have shown that the characteristic luminosity of the rest-frame ultraviolet (UV) luminosity function does not significantly evolve at 4 < z < 7 and is approxima…
The galaxy stellar mass function at 3.5<z<7.5 in the CANDELS/UDS, GOODS-South, and HUDF fields
A. Grazian, A. Fontana, P. Santini +38
The galaxy stellar mass function (GSMF) at high-z provides key information on star-formation history and mass assembly in the young Universe. We aimed to use the unique combination…
The Evolution of the Galaxy Rest-Frame Ultraviolet Luminosity Function Over the First Two Billion Years
Steven L. Finkelstein, Russell E. Ryan, Casey Papovich +26
We present a robust measurement and analysis of the rest-frame ultraviolet (UV) luminosity function at z=4-8. We use deep Hubble Space Telescope imaging over the CANDELS/GOODS fiel…
The HETDEX Pilot Survey V: The Physical Origin of Lyman-alpha Emitters Probed by Near-infrared Spectroscopy
Mimi Song, Steven L. Finkelstein, Karl Gebhardt +19
We present the results from a VLT/SINFONI and Keck/NIRSPEC near-infrared spectroscopic survey of 16 Lyman-alpha emitters (LAEs) at = 2.1 - 2.5 in the COSMOS and GOODS-N fields…
Rapid Decline of Lyman-alpha Emission Toward the Reionization Era
Vithal Tilvi, Casey Papovich, Steven L. Finkelstein +7
The observed deficit of strongly Lyman-alpha emitting galaxies at z>6.5 is attributed to either increasing neutral hydrogen in the intergalactic medium (IGM) and/or to the evolving…
Spectral Energy Distribution Fitting of HETDEX Pilot Survey Lyman-alpha Emitters in COSMOS and GOODS-N
Alex Hagen, Robin Ciardullo, Caryl Gronwall +15
We use broadband photometry extending from the rest-frame UV to the near-IR to fit the individual spectral energy distributions (SEDs) of 63 bright (L(Ly-alpha) > 10^43 ergs/s) Ly-…
A Rapidly Star-forming Galaxy 700 Million Years After the Big Bang at z=7.51
S. L. Finkelstein, C. Papovich, M. Dickinson +18
Out of several dozen z > 7 candidate galaxies observed spectroscopically, only five have been confirmed via Lyman-alpha emission, at z=7.008, 7.045, 7.109, 7.213 and 7.215. The sma…
The Spectrally Resolved Lyman-alpha Emission of Three Lyman-alpha Selected Field Galaxies at z~2.4 from the HETDEX Pilot Survey
Taylor S. Chonis, Guillermo A. Blanc, Gary J. Hill +11
We present new results on the spectrally resolved Lyman-alpha (LyA) emission of three LyA emitting field galaxies at z~2.4 with high LyA equivalent width (>100 Angstroms) and LyA l…