We describe a public data release of the FIRE-2 cosmological zoom-in simulations of galaxy
formation (available at http://flathub. flatironinstitute. org/fire) from the Feedback In Realistic …

As they grow, galaxies can transition from irregular/spheroidal with 'bursty'star formation
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …

We introduce a suite of cosmological volume simulations to study the evolution of galaxies
as part of the Feedback in Realistic Environments project. FIREbox, the principal simulation …

ABSTRACT JWST has revealed a large population of UV-bright galaxies at and possibly
overly massive galaxies at, challenging standard galaxy formation models in the ΛCDM …

Feedback from accreting supermassive black holes (SMBHs) is thought to be a primary
driver of quenching in massive galaxies, but how to best implement SMBH physics into …

Without active galactic nucleus (AGN) feedback, simulated massive, star-forming galaxies
become too compact relative to observed galaxies at z≲ 2. In this paper, we perform high …

The first stars, galaxies, star clusters, and direct-collapse black holes are expected to have
formed in low-mass (∼ 105–109 M⊙) haloes at Cosmic Dawn (z∼ 10–30) under conditions …

We present a detailed study of the cosmic star formation history over 90 per cent of cosmic
time (0≲ z≲ 4), using deep, radio continuum observations that probe star formation activity …

Abstract In the Λ-Cold Dark Matter model of the universe, galaxies form in part through
accreting satellite systems. Previous works have built an understanding of the signatures of …

Galaxies that are invisible in deep optical–near-infrared imaging but detected at longer
wavelengths have been the focus of several recent observational studies, with speculation …