871 citations · 2.3k across the 14 of their papers we have counts for
13 papers
CLEAR: Survey Overview, Data Analysis and Products
Raymond C. Simons, Casey Papovich, Ivelina G. Momcheva +19
We present an overview of the CANDELS Lyman-a Emission At Reionization (CLEAR) survey. CLEAR is a 130 orbit program of the Hubble Space Telescope using the Wide Field Camera 3 (WFC…
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 Astropy Problem
Demitri Muna, Michael Alexander, Alice Allen +151
The Astropy Project (http://astropy.org) is, in its own words, "a community effort to develop a single core package for Astronomy in Python and foster interoperability between Pyth…
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…
On the importance of using appropriate spectral models to derive physical properties of galaxies at 0.7<z<2.8
Camilla Pacifici, Elisabete da Cunha, Stéphane Charlot +14
Interpreting observations of distant galaxies in terms of constraints on physical parameters - such as stellar mass, star-formation rate (SFR) and dust optical depth - requires spe…