380 citations · 2.8k across the 17 of their papers we have counts for
16 papers
The Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years
J. A. Zavala, C. M. Casey, S. M. Manning +25
We present the first results from the 2mm Mapping Obscuration to Reionization (MORA) survey, the largest ALMA contiguous blank-field survey to-date with a total area of 184 sq. arc…
On the Gas Content, Star Formation Efficiency, and Environmental Quenching of Massive Galaxies in Proto-Clusters at z~2.0-2.5
Jorge A. Zavala, C. M. Casey, J. B. Champagne +9
We present ALMA Band 6 (nu=233GHz, lambda=1.3mm) continuum observations towards 68 'normal' star-forming galaxies within two Coma-like progenitor structures at z=2.10 and 2.47, fro…
The VIMOS Ultra Deep Survey First Data Release: spectra and spectroscopic redshifts of 698 objects up to z~6 in CANDELS
L. A. M. Tasca, O. Le Fevre, B. Ribeiro +45
This paper describes the first data release (DR1) of the VIMOS Ultra Deep Survey (VUDS). The DR1 includes all low-resolution spectroscopic data obtained in 276.9 arcmin2 of the CAN…
A Turnover in the Galaxy Main Sequence of Star Formation at for Redshifts
Nicholas Lee, D. B. Sanders, Caitlin M. Casey +14
The relationship between galaxy star formation rates (SFR) and stellar masses () is re-examined using a mass-selected sample of 62,000 star-forming galaxies at $z \le…
Quest for COSMOS submillimeter galaxy counterparts using CARMA and VLA: Identifying three high-redshift starburst galaxies
V. Smolcic, F. Navarrete, M. Aravena +16
We report on interferometric observations at 1.3 mm at 2"-3" resolution using the Combined Array for Research in Millimeter-wave Astronomy (CARMA). We identify multi-wavelength cou…
Molecular Gas in a Submillimeter Galaxy at z=4.5: Evidence for a Major Merger at 1 Billion Years after the Big Bang
E. Schinnerer, C. L. Carilli, P. Capak +8
We report the detection of CO molecular line emission in the z=4.5 millimeter-detected galaxy COSMOS_J100054+023436 (hereafter: J100+0234) using the IRAM Plateau de Bure interferom…