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 …

In the past five years, deep imaging campaigns conducted with the Hubble Space
Telescope (HST) and ground-based observatories have delivered large samples of galaxies …

Galaxies with stellar masses as high as roughly 1011 solar masses have been identified,–
out to redshifts z of roughly 6, around 1 billion years after the Big Bang. It has been difficult to …

Abstract The GLASS-JWST Early Release Science (hereafter GLASS-JWST-ERS) Program
will obtain and make publicly available the deepest extragalactic data of the ERS campaign …

One of the main goals of the JWST is to study the first galaxies in the Universe. We present a
systematic photometric analysis of very distant galaxies in the first JWST deep field towards …

We present the JWST cycle 1 53.8 h medium program FRESCO, short for 'First Reionization
Epoch Spectroscopically Complete Observations'. FRESCO covers 62 arcmin2 in each of …

ABSTRACT Spitzer/Infrared Array Camera (IRAC) imaging has revealed that the brightest
z∼ 7− 8 galaxies often exhibit young ages and strong nebular line emission, hinting at high …

We present the first constraints on the prevalence of z> 10 galaxies in the Hubble Ultra Deep
Field (HUDF) leveraging new NIRCam observations from JEMS (JWST Extragalactic …

Here we provide the most comprehensive determinations of the rest-frame UV luminosity
function (LF) available to date with the Hubble Space Telescope (HST) at z∼ 2–9 …

JWST has revolutionized the field of extragalactic astronomy with its sensitive and high-
resolution infrared view of the distant Universe. Adding to the new legacy of JWST …