150 citations · 513 across the 17 of their papers we have counts for
13 papers · 1 filter
Second public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation
Andrew Wetzel, Jenna Samuel, Pratik J. Gandhi +34
We describe the second data release (DR2) of the FIRE-2 cosmological zoom-in simulations of galaxy formation, from the Feedback In Realistic Environments (FIRE) project, available…
Evaluating Mass Outflow Rate Estimators in FIRE-2 Simulations: Towards a Self-Consistent Framework for Spectral Line Based Predictions
Cody A Carr, Aaron Smith, Viraj Pandya +4
$\require{mediawiki-texvc}$Galactic outflows shape galaxy evolution, but their mass, energy, and momentum transfer remain uncertain. High-resolution spectroscopy can help, but syst…
A Dusty Dawn: Galactic Dust Buildup at
Caleb R. Choban, Samir Salim, Dušan Kereš +2
Over the last decade, the Atacama Large Millimeter Array has revealed massive, dusty star-forming galaxies at , and the James Webb Space Telescope is primed to uncover e…
Host-galaxy stars can dominate the ionizing radiation field of the circumgalactic medium in galaxies at Cosmic Noon
Francisco Holguin, Christopher C. Hayward, Xiangcheng Ma +2
Elucidating the processes that shape the circumgalactic medium (CGM) is crucial for understanding galaxy evolution. Absorption and emission diagnostics can be interpreted using pho…
The impact of mass-dependent stochasticity at cosmic dawn
Viola Gelli, Charlotte Mason, Christopher C. Hayward
JWST is unveiling a surprising lack of evolution in the number densities of ultraviolet-selected (UV) galaxies at redshift . At the same time, observations and simulat…
Predictions for CO emission and the CO-to-H conversion factor in galaxy simulations with non-equilibrium chemistry
Oliver A. Thompson, Alexander J. Richings, Brad K. Gibson +3
Our ability to trace the star-forming molecular gas is important to our understanding of the Universe. We can trace this gas using CO emission, converting the observed CO intensity…