I present a comprehensive review of the evolution of galaxy structure in the Universe from
the first galaxies currently observable at z∼ 6 down to galaxies observable in the local …

We present the results of a size and structural analysis of 1395 galaxies at 0.5≤ z≲ 8 with
stellar masses log (M*/M⊙)> 9.5 within the James Webb Space Telescope Public CEERS …

Galaxy morphology is a product of how galaxies formed, how they interacted with their
environment, how they were influenced by internal perturbations, AGN, and dark matter, and …

We present an early analysis on the search for high-redshift galaxies using the deepest
public JWST imaging to date, the NGDEEP field. These data consist of six-band NIRCam …

We measure the sizes of 82 massive (M\geq 10^{11}\, M_ {\odot}) galaxies at 1.7\leq z\leq 3
utilizing deep HST NICMOS data taken in the GOODS North and South fields. Our sample is …

This paper begins a series in which we examine the structures of distant galaxies to directly
determine the history of their formation modes. We start this series by examining the …

We perform a comprehensive estimate of the frequency of galaxy mergers and their impact
on star formation over z∼ 0.24–0.80 (lookback time T b∼ 3–7 Gyr) using∼ 3600 (M⩾ 1× 10 …

We analyze 347 galaxies at redshift 4< z< 9.5 using JWST observations from the Cosmic
Evolution Early Release Science (CEERS) program by simultaneously fitting a two …

High-resolution imaging of galaxies in rest-frame UV has revealed the existence of giant star-
forming clumps prevalent in high-redshift galaxies. Studying these substructures provides …

Clumpy galaxies in the Galaxy Evolution from Morphology and SEDs and Great
Observatories Origins Deep Survey fields are examined for clues to their evolution into …