181 citations · 1.3k across the 38 of their papers we have counts for
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Evolution of Gas, and Star Formation from z = 0 to 5
Nick Scoville, Andreas Faisst, John Weaver +20
ALMA observations of the long wavelength dust continuum are used to estimate the gas masses in a sample of 708 star-forming (SF) galaxies at z = 0.3 to 4.5. We determine the depend…
No Redshift Evolution of Dust Temperatures from
Patrick M. Drew, Caitlin M. Casey
Some recent literature has claimed there to be an evolution in galaxies' dust temperatures towards warmer (or colder) spectral energy distributions (SEDs) between low and high reds…
Searching Far and Long I: Pilot ALMA 2mm Follow-up of Bright Dusty Galaxies as a Redshift Filter
Olivia R. Cooper, Caitlin M. Casey, Jorge A. Zavala +5
A complete census of dusty star-forming galaxies (DSFGs) at early epochs is necessary to constrain the obscured contribution to the cosmic star formation rate density (CSFRD), howe…
Measurements of the dust properties in z~1-3 SMGs with ALMA
E. da Cunha, J. A. Hodge, C. M. Casey +13
We present Atacama Large Millimetre Array (ALMA) 2mm continuum observations of a complete and unbiased sample of 99 870micron-selected sub-millimeter galaxies (SMGs) in the Extende…
Comprehensive Gas Characterization of a Protocluster: A Cluster Core Caught in the Beginning of Virialization?
Jaclyn B. Champagne, Caitlin M. Casey, Jorge A. Zavala +6
In order to connect galaxy clusters to their progenitor protoclusters, we must constrain the star formation histories within their member galaxies and the timescale of virial colla…
The Physical Drivers of the Luminosity-Weighted Dust Temperatures in High-Redshift Galaxies
Anne D. Burnham, Caitlin M. Casey, Jorge A. Zavala +7
The underlying distribution of galaxies' dust SEDs (i.e., their spectra re-radiated by dust from rest-frame 3m-3mm) remains relatively unconstrained due to a dearth of FIR…