A survey of high-z galaxies: serra simulations
We introduce serra, a suite of zoom-in high-resolution (, at z= 7.7) cosmological simulations
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
including non-equilibrium chemistry and on-the-fly radiative transfer. The outputs are post …
FIRE-2 simulations: physics versus numerics in galaxy formation
PF Hopkins, A Wetzel, D Kereš… - Monthly Notices of …, 2018 - academic.oup.com
ABSTRACT The Feedback In Realistic Environments (FIRE) project explores feedback in
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …
cosmological galaxy formation simulations. Previous FIRE simulations used an identical …
Ultrafaint dwarfs in a Milky Way context: introducing the Mint condition DC Justice League simulations
E Applebaum, AM Brooks, CR Christensen… - The Astrophysical …, 2021 - iopscience.iop.org
We present results from the" Mint" resolution DC Justice League suite of Milky Way–like
zoom-in cosmological simulations, which extend our study of nearby galaxies down into the …
zoom-in cosmological simulations, which extend our study of nearby galaxies down into the …
Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation
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 …
formation (available at http://flathub. flatironinstitute. org/fire) from the Feedback In Realistic …
Reconciling dwarf galaxies with ΛCDM cosmology: simulating a realistic population of satellites around a Milky Way–mass galaxy
Low-mass" dwarf" galaxies represent the most significant challenges to the cold dark matter
(CDM) model of cosmological structure formation. Because these faint galaxies are (best) …
(CDM) model of cosmological structure formation. Because these faint galaxies are (best) …
The cosmic baryon cycle and galaxy mass assembly in the FIRE simulations
D Anglés-Alcázar, CA Faucher-Giguère… - Monthly Notices of …, 2017 - academic.oup.com
We use cosmological simulations from the FIRE (Feedback In Realistic Environments)
project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo …
project to study the baryon cycle and galaxy mass assembly for central galaxies in the halo …
What causes the formation of discs and end of bursty star formation?
PF Hopkins, AB Gurvich, X Shen… - Monthly Notices of …, 2023 - academic.oup.com
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 …
histories (SFHs), to discy with smooth SFHs. But even in simulations, the direct physical …
Galaxies on FIRE (Feedback In Realistic Environments): stellar feedback explains cosmologically inefficient star formation
PF Hopkins, D Kereš, J Oñorbe… - Monthly Notices of …, 2014 - academic.oup.com
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 …
0, spanning halo masses∼ 108–1013 M⊙, and stellar masses∼ 104–1011 M⊙. Our …
Not so lumpy after all: modelling the depletion of dark matter subhaloes by Milky Way-like galaxies
Among the most important goals in cosmology is detecting and quantifying small () dark
matter (DM) subhaloes. Current probes around the Milky Way (MW) are most sensitive to …
matter (DM) subhaloes. Current probes around the Milky Way (MW) are most sensitive to …
The origin and evolution of the galaxy mass–metallicity relation
X Ma, PF Hopkins, CA Faucher-Giguère… - Monthly Notices of …, 2016 - academic.oup.com
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 …
Environment (FIRE) project to study the galaxy mass–metallicity relations (MZR) from z= 0 …