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 …

Numerical simulations have become a major tool for understanding galaxy formation and
evolution. Over the decades the field has made significant progress. It is now possible to …

The protagonists of the last great phase transition of the universe—cosmic reionization—
remain elusive. Faint star-forming galaxies are leading candidates because they are found …

We make use of sensitive (9.3 μJy beam− 1 rms) 1.2 mm continuum observations from the
Atacama Large Millimeter/submillimeter Array (ALMA) Spectroscopic Survey in the Hubble …

What are the faintest distant galaxies we can see with the Hubble Space Telescope (HST)
now, before the launch of the James Webb Space Telescope? This is the challenge taken …

We present specific star formation rates (sSFRs) for 40 ultraviolet (UV)-bright galaxies at z∼
7–8 observed as part of the Reionization Era Bright Emission Line Survey (REBELS) …

Context. How galaxies form, assemble, and cease their star formation is a central question
within the modern landscape of galaxy evolution studies. These processes are indelibly …

We present results from the Cosmic Evolution Early Release Survey on the stellar
population parameters for 28 galaxies with redshifts 4< z< 9 using imaging data from the …

We present a new flexible Bayesian framework for directly inferring the fraction of neutral
hydrogen in the intergalactic medium (IGM) during the Epoch of Reionization (EoR, z∼ 6 …

We present an analysis of the deepest Herschel images in four major extragalactic fields
GOODS–North, GOODS–South, UDS, and COSMOS obtained within the GOODS–Herschel …