activity
20142024
most citedTwo Remarkably Luminous Galaxy Candidates at Revealed by JWST

441 citations · 1.5k across the 34 of their papers we have counts for

collaborators

34 papers

astro-ph.GA20241 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.GA20241 cited

UNCOVER: Significant Reddening in Cosmic Noon Quiescent Galaxies

Jared Siegel, David Setton, Jenny Greene +19

We explore the physical properties of five massive quiescent galaxies at , revealing the presence of non-negligible dust reservoirs. JWST NIRSpec observations were obtain…

astro-ph.GA202411 cited

Age and metal gradients in massive quiescent galaxies at : implications for quenching and assembly histories

Chloe M. Cheng, Mariska Kriek, Aliza G. Beverage +12

We present spatially resolved, simple stellar population equivalent ages, stellar metallicities, and abundance ratios for 456 massive ($10.3\lesssim\log(\mathrm{M}_*/\mathrm{M}_\od…

astro-ph.GA20241 cited

Medium Bands, Mega Science: a JWST/NIRCam Medium-Band Imaging Survey of Abell 2744

Katherine A. Suess, John R. Weaver, Sedona H. Price +39

In this paper, we describe the "Medium Bands, Mega Science" JWST Cycle 2 survey (JWST-GO-4111) and demonstrate the power of these data to reveal both the spatially-integrated and s…

astro-ph.GA2024

Estimating Galaxy Parameters with Self-Organizing Maps and the Effect of Missing Data

Valentina La Torre, Anna Sajina, Andy D. Goulding +4

The current and upcoming large data volume galaxy surveys require the use of machine learning techniques to maximize their scientific return. This study explores the use of Self-Or…

astro-ph.GA20241 cited

A Comparison of Star-Formation Histories Derived from UniverseMachine and LEGA-C at

Cecilia Steel, Alan Pearl, Yasha Kaushal +1

In this work, we compare star formation histories of massive (10.5 12) galaxies in the UniverseMachine model to those measured from the Large Ear…