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HST Hα grism spectroscopy of ROLES: a flatter low-mass slope for the z~1 SSFR--mass relation
Riona Ramraj, David G. Gilbank, Sarah-Louise Blyth +4
We present measurements of star formation rates (SFRs) for dwarf galaxies (M*~10^8.5 Msun ) at z~1 using near-infrared slitless spectroscopy from the Hubble Space Telescope (HST) b…
Galaxy environment in the 3D-HST fields. Witnessing the onset of satellite quenching at z ~ 1-2
M. Fossati, D. J. Wilman, J. T. Mendel +25
We make publicly available a catalog of calibrated environmental measures for galaxies in the five 3D-HST/CANDELS deep fields. Leveraging the spectroscopic and grism redshifts from…
The Number Density Evolution of Extreme Emission Line Galaxies in 3D-HST: Results from a Novel Automated Line Search Technique for Slitless Spectroscopy
Michael V. Maseda, Arjen van der Wel, Hans-Walter Rix +6
The multiplexing capability of slitless spectroscopy is a powerful asset in creating large spectroscopic datasets, but issues such as spectral confusion make the interpretation of…
The Evolution of the Fractions of Quiescent and Star-forming Galaxies as a Function of Stellar Mass Since z=3: Increasing Importance of Massive, Dusty Star-forming Galaxies in the Early Universe
Nicholas S. Martis, Danilo Marchesini, Gabriel B. Brammer +7
Using the UltraVISTA DR1 and 3D-HST catalogs, we construct a stellar-mass-complete sample, unique for its combination of surveyed volume and depth, to study the evolution of the fr…
Predicting Quiescence: The Dependence of Specific Star Formation Rate on Galaxy Size and Central Density at 0.5<z<2.5
Katherine E. Whitaker, Rachel Bezanson, Pieter G. van Dokkum +9
In this paper, we investigate the relationship between star formation and structure, using a mass-complete sample of 27,893 galaxies at selected from 3D-HST. We confirm…
The Relation Between [OIII]/H and Specific Star Formation Rate in Galaxies at
Claire Mackay Dickey, Pieter van Dokkum, Pascal Oesch +7
Recent surveys have identified a seemingly ubiquitous population of galaxies with elevated [OIII]/H emission line ratios at , though the nature of this phenomenon continu…