The new capabilities that JWST offers in the near-and mid-infrared (IR) are used to
investigate in unprecedented detail the nature of optical/near-IR-faint, mid-IR-bright sources …

We investigate the stellar populations for a sample of 24 quiescent galaxies at 1.5< z< 2.5
using deep rest-frame optical spectra obtained with Keck MOSFIRE. By fitting templates …

Structural and Star-forming Relations since z ∼ 3: Connecting Compact Star-forming and
Quiescent Galaxies - IOPscience This site uses cookies. By continuing to use this site you …

We study a new population of extremely red objects (EROs) recently discovered by the
James Webb Space Telescope (JWST) based on their NIRCam colors F277W− F444W> 1.5 …

The diffuse extragalactic background light (EBL) is formed by ultraviolet (UV), optical, and
infrared (IR) photons mainly produced by star formation processes over the history of the …

Hyper Suprime-Cam Subaru Strategic Program: A Mass-dependent Slope of the Galaxy
Size−Mass Relation at z < 1 - IOPscience This site uses cookies. By continuing to use this site …

The star formation histories (SFHs) of galaxies contain imprints of the physical processes
responsible for regulating star formation during galaxy growth and quenching. We improve …

We show how the interplay between active galactic nuclei (AGNs) and merger history
determines whether a galaxy quenches star formation (SF) at high redshift. We first simulate …

The most massive galaxies in the Universe stopped forming stars due to the time-integrated
feedback from central supermassive black holes (SMBHs). However, the exact quenching …

We investigate the assembly history of massive disk galaxies and describe how they shape
their morphology through cosmic time. Using SHARDS and HST data, we modeled the …