Hydrogen Lyman-α (Lyα) emission has been one of the major observational probes for the
high-redshift Universe since the first discoveries of high-z Lyα-emitting galaxies in the late …

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 …

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 describe new JWST/NIRSpec observations of galaxies at z≳ 7 taken from the CEERS
survey. Previous observations of this area have revealed associations of Lyα emitters at …

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 …

We introduce the thesan project, a suite of large volume () radiation-magnetohydrodynamic
simulations that simultaneously model the large-scale statistical properties of the …

We have derived luminosity functions and set constraints on the UV luminosity and SFR
density from z∼ 17 to z∼ 8, using the three most-studied JWST/NIRCam data sets, the …

Abstract The Reionization Era Bright Emission Line Survey (REBELS) is a cycle-7 ALMA
Large Program (LP) that is identifying and performing a first characterization of many of the …

The ultraviolet (UV) continuum slope (β, where f λ∝ λ β) of galaxies is sensitive to a variety
of properties, from the metallicity and age of the stellar population to dust attenuation …