activity
20242026
collaborators

8 papers

astro-ph.GA2026

Discovery of Ancient Globular Cluster Candidates in the Relic, a Quiescent Galaxy at

Katherine E. Whitaker, Sam E. Cutler, Rupali Chandar +31

Globular clusters (GCs) are some of the oldest bound structures in the Universe, holding clues to the earliest epochs of star formation and galaxy assembly. However, accurate age m…

astro-ph.GA2025

Overview of the JWST Advanced Deep Extragalactic Survey (JADES)

Daniel J. Eisenstein, Chris Willott, Stacey Alberts +75

We present an overview of the James Webb Space Telescope (JWST) Advanced Deep Extragalactic Survey (JADES), an ambitious program of infrared imaging and spectroscopy in the GOODS-S…

astro-ph.GA2025

The JADES Origins Field: A New JWST Deep Field in the JADES Second NIRCam Data Release

Daniel J. Eisenstein, Benjamin D. Johnson, Brant Robertson +58

We summarize the properties and initial data release of the JADES Origins Field (JOF), the longest single pointing yet imaged with the James Webb Space Telescope (JWST). This field…

astro-ph.GA2025

The Structure and Formation Histories of Low-Mass Quiescent Galaxies in the Abell 2744 Cluster Environment

Sam E. Cutler, John R. Weaver, Katherine E. Whitaker +21

Low-mass quiescent galaxies are thought to predominantly reside in overdense regions, as environmental effects are often invoked to explain their shutdown of star formation. These…

astro-ph.GA2025

DUALZ: Deep UNCOVER-ALMA Legacy High-Z Survey

Seiji Fujimoto, Rachel Bezanson, Ivo Labbe +29

We present the survey design and initial results of the ALMA Cycle 9 program of DUALZ, which aims to establish a joint ALMA and JWST public legacy field targeting the massive galax…

astro-ph.GA2025

UNCOVER: The rest ultraviolet to near infrared multiwavelength structures and dust distributions of sub-millimeter-detected galaxies in Abell 2744

Sedona H. Price, Katherine A. Suess, Christina C. Williams +18

With the wavelength coverage, sensitivity, and high spatial resolution of JWST, it is now possible to peer through the dust attenuation to probe the rest-frame near infrared (NIR)…