Galaxy formation is at the heart of our understanding of cosmic evolution. Although there is a
consensus that galaxies emerged from the expanding matter background by gravitational …

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 early results regarding the morphological and structural properties of galaxies
seen with the James Webb Space Telescope (JWST) at z> 3 in the Early Release …

We present an overview of galaxy evolution across cosmic time in the Illustris simulation.
Illustris is an N-body/hydrodynamical simulation that evolves 2× 18203 resolution elements …

We present results on the morphological and structural evolution of a total of 3956 galaxies
observed with JWST at 1.5< z< 6.5 in the JWST CEERS observations that overlap with the …

The evolution of the number density of galaxies in the universe, and thus also the total
number of galaxies, is a fundamental question with implications for a host of astrophysical …

We present the redshift evolution of the galaxy effective radius re obtained from the Hubble
Space Telescope (HST) samples of∼ 190,000 galaxies at z= 0–10. Our HST samples …

Galaxy mergers are expected to have a significant role in the mass assembly of galaxies in
the early universe, but there are very few observational constraints on the merger history of …

Star-forming galaxies can exhibit strong morphological differences between the rest-frame
far-UV and optical, reflecting inhomogeneities in star formation and dust attenuation. We …

Abstract We present new Hubble Space Telescope/Wide Field Camera 3 (HST/WFC3)
imaging of 25 extremely luminous (− 23.2≤ M UV≲− 21.2) Lyman-break galaxies (LBGs) at …