activity
20202022
most citedThe Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years

181 citations · 183 across the 4 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2022

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…

astro-ph.GA20212 cited

Lower-Luminosity Obscured AGN Host Galaxies are Not Predominantly in Major-Merging Systems at Cosmic Noon

Erini Lambrides, Marco Chiaberge, Timothy Heckman +15

For over 60 years, the scientific community has studied actively growing central super-massive black holes (active galactic nuclei -- AGN) but fundamental questions on their genesi…

astro-ph.GA2021

Merger or Not: Accounting for Human Biases in Identifying Galactic Merger Signatures

Erini Lambrides, Duncan J. Watts, Marco Chiaberge +9

Significant galaxy mergers throughout cosmic time play a fundamental role in theories of galaxy evolution. The widespread usage of human classifiers to visually assess whether gala…

astro-ph.GA2021

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…

astro-ph.GA2021181 cited

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…

astro-ph.GA2020

Emergence of an Ultra-Red Ultra-Massive Galaxy Cluster Core at

Arianna S. Long, Asantha Cooray, Jingzhe Ma +6

Recent simulations and observations of massive galaxy cluster evolution predict that the majority of stellar mass build up happens within cluster members by , before cluster v…