We present the survey design, implementation, and outlook for COSMOS-Web, a 255 hr
treasury program conducted by the James Webb Space Telescope in its first cycle of …

Galaxy sizes and their evolution over cosmic time have been studied for decades and serve
as key tests of galaxy formation models. However, at z≳ 1 these studies have been limited …

We present the galaxy stellar mass–size relation in the rest-frame near-IR (1.5 μm) and its
evolution with redshift up to z= 2.5. Sérsic profiles are measured for∼ 26,000 galaxies with …

We analyse the joint distribution of dust attenuation and projected axis ratios, together with
galaxy size and surface brightness profile information, to infer lessons on the dust content …

The existence of massive quiescent galaxies at high redshift seems to require rapid
quenching, but it is unclear whether all quiescent galaxies have gone through this phase …

Abstract We use the Ultraviolet Imaging of the Cosmic Assembly Near-infrared Deep
Extragalactic Legacy Survey fields (UVCANDELS) to measure half-light radii in the rest …

MAGAZ3NE: High Stellar Velocity Dispersions for Ultramassive Quiescent Galaxies at z ≳ 3 -
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We present the results of a systematic study of the rest-frame optical morphology of
quiescent galaxies at z≥ 3 using the Near-Infrared Camera (NIRCam) on board the James …

We use the unprecedented resolution and depth of the JWST NIRCam Early Release
Observations at 1–5 μm to study the stellar mass, age, and metallicity of compact star …

We present spatially resolved, simple stellar population equivalent ages, stellar metallicities,
and abundance ratios for 456 massive () quiescent galaxies at from the Large Early Galaxy …