activity
20172026
most citedThe Evolution of the IR Luminosity Function and Dust-obscured Star Formation in the Last 13 Billion Years

181 citations · 512 across the 25 of their papers we have counts for

collaborators

29 papers

astro-ph.GA2026

CHAMPS: Data Reduction and Detection of ~3300 Dusty Galaxies at 1.2 mm

Felix Martinez, Jeyhan S. Karaltepe, Andreas L. Faisst +52

We present the reduction and source catalogs for the \textit{COSMOS High- ALMA-MIRI Population Survey} (CHAMPS), the largest Atacama Large (Sub)Millimeter Array (ALMA) blank fie…

astro-ph.GA2026

CHAMPS: The COSMOS High-Redshift ALMA-MIRI Population Survey - A New Census of the Dusty Early Universe

Andreas L. Faisst, Felix Martinez, Jeyhan S. Kartaltepe +86

Understanding how dust forms and evolves over cosmic time is a key open problem in extragalactic astrophysics. Galaxies in the early Universe were once thought to be mostly dust-po…

astro-ph.GA2026

Star Formation and Nebular Attenuation from Pa, Br, and Br in Massive Dust-obscured Galaxies at Cosmic Noon using JWST

Virginia Vanicek, Jed McKinney, Alexandra Pope +14

Near-infrared hydrogen recombination lines can provide robust star-formation rates if the effects of dust attenuation continue to diminish towards longer wavelengths. To quantify n…

astro-ph.GA2026

Dust in the Average Galaxy: Attenuation, Emission, and Opacity from

Caitlin M. Casey, Hollis B. Akins, Andrew J. Battisti +43

We present constraints on the dust emission and attenuation properties of galaxies across 0<z<7 using JWST imaging from the COSMOS-Web Survey combined with deep FIR/(sub)millimeter…

astro-ph.GA2026

PANORAMIC: The Dawn of Massive Quiescent Galaxies I. Number Density and Cosmic Variance from 1000 arcmin NIRCam Imaging

Zhiyuan Ji, Christina C. Williams, Peter Behroozi +13

We measure the number density and field-to-field variance of massive quiescent galaxies at - 8 using the JWST/NIRCam pure-parallel imaging survey PANORAMIC together with a…

astro-ph.GA2026

A PANORAMIC of UV-optical morphologies of "Little Red Dots": Two groups of LRDs distinguished by UV half-light radius

Aidan P. Cloonan, Katherine E. Whitaker, Sinclaire M. Manning +13

Among the most remarkable results from JWST is the discovery of abundant, compact, and very red sources in the early Universe known as "Little Red Dots" (LRDs). The relative degree…

astro-ph.GA2025

ALMA and JWST Identification of Faint Dusty Star-Forming Galaxies up to z~8

Jorge A. Zavala, Andreas L. Faisst, Manuel Aravena +44

We exploit a new sample of around 400 bright dusty galaxies from the ALMA CHAMPS Large Program, together with the rich JWST multi-band data products in the COSMOS field, to explore…

astro-ph.GA2025★ 1 cited

JWST+ALMA reveal the ISM kinematics and stellar structure of MAMBO-9, a merging pair of DSFGs in an overdense environment at

Hollis B. Akins, Caitlin M. Casey, Jaclyn B. Champagne +14

We present high-resolution ALMA [CII] 158 micron observations and JWST/NIRCam+MIRI imaging of MAMBO-9, a pair of optically-dark, dusty star-forming galaxies at . MAMBO-9 is…

astro-ph.GA2025

JWST+ALMA reveal the build up of stellar mass in the cores of dusty star-forming galaxies at Cosmic Noon

Sarah Bodansky, Katherine E. Whitaker, Ayesha Abdullah +14

Dusty star-forming galaxies have long been suspected to serve as the missing evolutionary bridge between the star-forming and quiescent phases of massive galaxy evolution. With the…

astro-ph.GA2025

An upper limit of 10 M in dust from ALMA observations in 60 Little Red Dots

Caitlin M. Casey, Hollis B. Akins, Steven L. Finkelstein +9

By virtue of their red color, the dust in little red dots (LRDs) has been thought to be of appreciable influence, whether that dust is distributed in a torus around a compact activ…

astro-ph.GA2025

SCUBADive II: Searching for Dust-Obscured Galaxies via F150W-Dropouts in COSMOS-Web

Sinclaire M. Manning, Jed McKinney, Katherine E. Whitaker +24

The relative fraction of obscured galaxies at compared to lower redshifts remains highly uncertain as accurate bookkeeping of the dust-obscured component proves difficult. We…

astro-ph.GA2024

RUBIES: JWST/NIRSpec resolves evolutionary phases of dusty star-forming galaxies at

Olivia R. Cooper, Gabriel Brammer, Kasper E. Heintz +24

The dearth of high quality spectroscopy of dusty star-forming galaxies (DSFGs) -- the main drivers of the assembly of dust and stellar mass at the peak of activity in the Universe…

astro-ph.GA2024★ 1 cited

The PANORAMIC Survey: Pure Parallel Wide Area Legacy Imaging with JWST/NIRCam

Christina C. Williams, Pascal A. Oesch, Andrea Weibel +15

We present the PANORAMIC survey, a pure parallel extragalactic imaging program with NIRCam observed during JWST Cycle 1. The survey obtained 530 sq arcmin of NIRCam imaging f…

astro-ph.GA2024★ 4 cited

The Extended Mapping Obscuration to Reionization with ALMA (Ex-MORA) Survey: 5 Source Catalog and Redshift Distribution

Arianna S. Long, Caitlin M. Casey, Jed McKinney +41

One of the greatest challenges in galaxy evolution over the last decade has been constraining the prevalence of heavily dust-obscured galaxies in the early Universe. At , thes…

astro-ph.GA2024★ 2 cited

SCUBADive I: JWST+ALMA Analysis of 289 sub-millimeter galaxies in COSMOS-Web

Jed McKinney, Caitlin M. Casey, Arianna S. Long +36

JWST has enabled detecting and spatially resolving the heavily dust-attenuated stellar populations of sub-millimeter galaxies, revealing detail that was previously inaccessible. In…

astro-ph.GA2024★ 2 cited

Dust in Little Red Dots

Caitlin M. Casey, Hollis B. Akins, Vasily Kokorev +5

JWST has revealed a ubiquitous population of ``little red dots'' (LRDs) at , selected via their red rest-frame optical emission and compact morphologies. They are though…

astro-ph.GA2023

Uncovering a Massive z~7.7 Galaxy Hosting a Heavily Obscured Radio-Loud QSO Candidate in COSMOS-Web

Erini Lambrides, Marco Chiaberge, Arianna Long +47

In this letter, we report the discovery of the highest redshift, heavily obscured, radio-loud AGN candidate selected using JWST NIRCam/MIRI, mid-IR, sub-mm, and radio imaging in th…

astro-ph.GA2023★ 2 cited

A Near-Infrared Faint, Far-Infrared-Luminous Dusty Galaxy at z~5 in COSMOS-Web

Jed McKinney, Sinclaire M. Manning, Olivia R. Cooper +32

A growing number of far-infrared bright sources completely invisible in deep extragalactic optical surveys hint at an elusive population of z>4 dusty, star-forming galaxies. Cycle…

astro-ph.GA2022★ 13 cited

COSMOS-Web: An Overview of the JWST Cosmic Origins Survey

Caitlin M. Casey, Jeyhan S. Kartaltepe, Nicole E. Drakos +82

We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hour treasury program conducted by the James Webb Space Telescope in its first cycle of observations…

astro-ph.GA2022★ 25 cited

Probing cold gas in a massive, compact star-forming galaxy at z=6

Jorge A. Zavala, Caitlin M. Casey, Justin Spilker +7

Observations of low order CO transitions represent the most direct way to study galaxies' cold molecular gas, the fuel of star formation. Here we present the first detection of CO(…

astro-ph.GA2021★ 52 cited

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…

astro-ph.GA2021★ 76 cited

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…

astro-ph.GA2021★ 13 cited

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…

astro-ph.GA2021★ 181 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…