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Everything Every Band All at Once II: The Relationship Between Optical Size and Stellar Mass Over Eight Billion Years of Cosmic History
While the size-mass relation provides insight into the structural evolution of galaxies, the data available and methods employed have …
Evidence for Shallow Nebular Attenuation Curves and Patchy Dust Geometry at z~2 with Pa-beta/H-alpha Measurements from JWST-MegaScience Medium Band Photometry
We constrain the nebular attenuation curve and investigate dust geometry in star-forming galaxies at cosmic noon using photometric …
Water absorption confirms cool atmospheres in two little red dots
Little red dots (LRDs) are an abundant population of compact high- redshift sources with red rest-frame optical continua, discovered by …
UNCOVER/MegaScience Finds Uniform and Highly Bursty Star Formation at 3 < z < 9, consistent with the High-Redshift UV Luminosity Function
Star formation timescales are key to understanding fundamental physics like feedback mechanisms, as well as the abundance of bright …
JWST+ALMA reveal the build up of stellar mass in the cores of dusty star-forming galaxies at Cosmic Noon
Dusty star-forming galaxies have long been suspected to serve as the missing evolutionary bridge between the star-forming and quiescent …
MINERVA: A NIRCam Medium Band and MIRI Imaging Survey to Unlock the Hidden Gems of the Distant Universe
We present an overview of the MINERVA survey, a 259.8 hour (prime) and 127 hour (parallel) Cycle 4 treasury program on the James Webb …
An unambiguous AGN and a Balmer break in an Ultraluminous Little Red Dot at z=4.47 from Ultradeep UNCOVER and All the Little Things Spectroscopy
We present a detailed exploration of the most optically-luminous Little Red Dot (LHα=10⁴⁴erg/s, LV=10⁴⁵erg/s, F444W=22AB) found to …