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Rest-frame Near-infrared Sizes of Galaxies at Cosmic Noon: Objects in JWST's Mirror Are Smaller than They Appeared
Galaxy sizes and their evolution over cosmic time have been studied for decades and serve as key tests of galaxy formation models. …
Implications of a Temperature-dependent Initial Mass Function. III. Mass Growth and Quiescence
The stellar initial mass function (IMF) is predicted to depend upon the temperature of gas in star-forming molecular clouds. The …
Implications of a Temperature-dependent Initial Mass Function. II. An Updated View of the Star-forming Main Sequence
The stellar initial mass function (IMF) is predicted to depend upon the temperature of gas in star-forming molecular clouds. The …
COSMOS2020: Ubiquitous AGN Activity of Massive Quiescent Galaxies at 0 < z < 5 Revealed by X-Ray and Radio Stacking
We characterize the average X-ray and radio properties of quiescent galaxies (QGs) with $mathrmlog(M_⋆ /M_ødot ) 10$ at 0 < z < …
The Archival Discovery of a Strong Lyensuremathα and [C II] Emitter at z = 7.677
We report the archival discovery of Lyensuremathα emission from the bright ultraviolet galaxy Y002 at z = 7.677, spectroscopically …
COSMOS2020: A Panchromatic View of the Universe to z 10 from Two Complementary Catalogs
The Cosmic Evolution Survey (COSMOS) has become a cornerstone of extragalactic astronomy. Since the last public catalog in 2015, a …
Extensive Lensing Survey of Optical and Near-infrared Dark Objects (El Sonido): HST H-faint Galaxies behind 101 Lensing Clusters
We present a Spitzer/IRAC survey of H-faint (H $_160$ ensuremathgtrsim 26.4, < 5ensuremathσ) sources in 101 lensing cluster fields. …
The BUFFALO HST Survey
The Beyond Ultra-deep Frontier Fields and Legacy Observations (BUFFALO) is a 101 orbit + 101 parallel Cycle 25 Hubble Space Telescope …