181 citations · 763 across the 14 of their papers we have counts for
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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…
Characterization of Two 2mm-detected Optically-Obscured Dusty Star-Forming Galaxies
Sinclaire M. Manning, Caitlin M. Casey, Jorge A. Zavala +22
The 2mm Mapping Obscuration to Reionization with ALMA (MORA) Survey was designed to detect high redshift (), massive, dusty star-forming galaxies (DSFGs). Here we presen…
Mapping Obscuration to Reionization with ALMA (MORA): 2mm Efficiently Selects the Highest-Redshift Obscured Galaxies
Caitlin M. Casey, Jorge A. Zavala, Sinclaire M. Manning +24
We present the characteristics of 2mm-selected sources from the largest Atacama Large Millimeter and submillimeter Array (ALMA) blank-field contiguous survey conducted to-date, the…
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…
SuperCLASS -- II: Photometric Redshifts and Characteristics of Spatially-Resolved Jy Radio Sources
Sinclaire M. Manning, Caitlin M. Casey, Chao-Ling Hung +12
We present optical and near-infrared imaging covering a 1.53 deg region in the Super-Cluster Assisted Shear Survey (SuperCLASS) field, which aims to make the first robust…
Three Dusty Star Forming Galaxies at : Mergers and Disks on the Main Sequence
Patrick M. Drew, Caitlin M. Casey, Asantha Cooray +1
The main sequence of galaxies, a correlation between the star formation rates and stellar masses of galaxies, has been observed out to . Galaxies within the scatter of the…
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…
Physical Characterization of an Unlensed Dusty Star-Forming Galaxy at
Caitlin M. Casey, Jorge A. Zavala, Manuel Aravena +23
We present a physical characterization of MMJ100026.36+021527.9 (a.k.a. ``MAMBO-9''), a dusty star-forming galaxy (DSFG) at . This is the highest redshift unlensed…
Taking Census of Massive, Star-Forming Galaxies formed <1 Gyr After the Big Bang
Caitlin M. Casey, Peter Capak, Johannes Staguhn +24
Two decades of effort have been poured into both single-dish and interferometric millimeter-wave surveys of the sky to infer the volume density of dusty star-forming galaxies (DSFG…
Evidence of a Flat Outer Rotation Curve in a Starbursting Disk Galaxy at
Patrick M. Drew, Caitlin M. Casey, Anne D. Burnham +4
Observations of the baryon to dark matter fraction in galaxies through cosmic time are a fundamental test for galaxy formation models. Recent observational studies have suggested t…
Constraining the volume density of Dusty Star-Forming Galaxies through the first 3mm Number Counts from ALMA
J. A. Zavala, C. M. Casey, E. da Cunha +4
We carry out a blind search of 3mm continuum sources using the ALMA Science Archive to derive the first galaxy number counts at this wavelength. The analyzed data are drawn from ob…
An Analysis of ALMA Deep Fields and the Perceived Dearth of High-z Galaxies
Caitlin M. Casey, Jacqueline Hodge, Jorge A. Zavala +5
Deep, pencil-beam surveys from ALMA at 1.1-1.3mm have uncovered an apparent absence of high-redshift dusty galaxies, with existing redshift distributions peaking around $z\sim1.5-2…
The Brightest Galaxies in the Dark Ages: Galaxies' Dust Continuum Emission During the Reionization Era
Caitlin M. Casey, Jorge A. Zavala, Justin Spilker +6
Though half of cosmic starlight is absorbed by dust and reradiated at long wavelengths (3m-3mm), constraints on the infrared through millimeter galaxy luminosity function (the `…