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The Grism lens-amplified survey from space (GLASS). VII. The diversity of the distribution of star formation in cluster and field galaxies at 0.3<z<0.7
Benedetta Vulcani, Tommaso Treu, Kasper B. Schmidt +10
Exploiting the slitless spectroscopy taken as part of the Grism Lens-Amplified Survey from Space (GLASS), we present an extended analysis of the spatial distribution of star format…
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…
Ultra-deep Ks-band Imaging of the Hubble Frontier Fields
Gabriel B. Brammer, Danilo Marchesini, Ivo Labbé +16
We present an overview of the "KIFF" project, which provides ultra-deep Ks-band imaging of all six of the Hubble Frontier Fields clusters Abell 2744, MACS-0416, Abell S1063, Abell…
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…