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Toward Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-early Star Formation Tensions
The discovery of a population of massive, ancient quiescent galaxies within the first 2 Gyr of the Universe’s history has led to …
Toward Unbreaking the Universe: MINERVA Measurements of Color Gradients in Massive Quiescent Galaxies Can Help Ease Too-early Star Formation Tensions
Everything Every Band All at Once. I. A Global Morphology Catalog in A2744 Based on UNCOVER/MegaScience
We present spectrally resolved structural parameter measurements of 28,274 sources from the legacy lensing field of A2744, quantifying …
Discovery of Red Galaxy Candidates at z ~ 12: Early Dust Growth or Significant Nebular Emission with High-temperature Stars?
We report the discovery of two z ~ 12 galaxy candidates with unusually red UV slopes (βUV ≳ -1.5), and probe the origin of such colors …
Discovery of Ancient Globular Cluster Candidates in the Relic, a Quiescent Galaxy at z = 2.5
Globular clusters (GCs) are some of the oldest bound structures in the Universe, holding clues to the earliest epochs of star formation …
JWST+ALMA Reveal the Buildup of Stellar Mass in the Cores of Dusty Star-forming Galaxies at Cosmic Noon
Dusty star-forming galaxies (DSFGs) have long been suspected to serve as the missing evolutionary bridge between the star-forming and …
RUBIES Spectroscopically Confirms the High Number Density of Quiescent Galaxies from 2 < z< 5
We present the number density of massive (log(M*/M☉)>10.3) quiescent galaxies at 2 < z < 5 using JWST NIRSpec PRISM spectra. …
Taking a Break at Cosmic Noon: Continuum-selected Low-mass Galaxies Require Long Burst Cycles
While bursty star formation in low-mass galaxies has been observed in local populations and reproduced in simulations, the dormant …
What You See Is What You Get: Empirically Measured Bolometric Luminosities of Little Red Dots
New populations of red active galactic nuclei (known as “little red dots”) discovered by JWST exhibit remarkable spectral energy …
The Evolution of Half-mass Radii and Color Gradients for Young and Old Quiescent Galaxies at 0.5 < z < 3 with JWST/PRIMER
We present a study of the size growth of the red sequence between 0.5 < z < 3, tracing the evolution of quiescent galaxies in …
The Structure and Formation Histories of Low-mass Quiescent Galaxies in the A2744 Cluster Environment
Low-mass quiescent galaxies are thought to predominantly reside in overdense regions, as environmental effects are often invoked to …
The Structure and Formation Histories of Low-mass Quiescent Galaxies in the A2744 Cluster Environment