Galaxy Evolution

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. …
A galaxy group candidate at z ensuremath≈ 3.7 in the COSMOS field
We report a galaxy group candidate HPC1001 at z ensuremath≈ 3.7 in the COSMOS field. This structure was selected as a high galaxy …
Diagnosing deceivingly cold dusty galaxies at 3.5 < z < 6: A substantial population of compact starbursts with high infrared optical depths
Using NOEMA and ALMA 3mm line scans, we measured spectroscopic redshifts of six new dusty galaxies at 3.5 < z < 4.2 by solidly …
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 …