Spurred by rich, multiwavelength observations and enabled by new simulations, ranging
from cosmological to subparsec scales, the past decade has seen major theoretical …

The bulk of cosmic matter resides in a dilute reservoir that fills the space between galaxies,
the intergalactic medium (IGM). The history of this reservoir is intimately tied to the cosmic …

ABSTRACT The Feedback In Realistic Environments (FIRE) project explores feedback in
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …

We present a series of high-resolution cosmological simulations1 of galaxy formation to z=
0, spanning halo masses∼ 108–1013 M⊙, and stellar masses∼ 104–1011 M⊙. Our …

We present an analysis of the galaxy-scale gaseous outflows from the Feedback in Realistic
Environments (FIRE) simulations. This suite of hydrodynamic cosmological zoom …

We present the mufasa suite of cosmological hydrodynamic simulations, which employs the
gizmo meshless finite mass (MFM) code including H 2-based star formation, nine-element …

We use high-resolution cosmological zoom-in simulations from the Feedback in Realistic
Environment (FIRE) project to study the galaxy mass–metallicity relations (MZR) from z= 0 …

We present an updated model of the cosmic ionizing background from the UV to the X-rays.
Relative to our previous model, the new model provides a better match to a large number of …

We study the distribution of cold dark matter (CDM) in cosmological simulations from the
FIRE (Feedback In Realistic Environments) project, for M*∼ 104–11 M⊙ galaxies in M h∼ …

We report the detection of extended Lyα haloes around 145 individual star-forming galaxies
at redshifts 3≤ z≤ 6 in the Hubble Ultra Deep Field observed with the Multi-Unit …