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20132025
most citedFIRE-2 Simulations: Physics versus Numerics in Galaxy Formation

1.1k citations · 5.7k across the 75 of their papers we have counts for

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Showing 2022Show all

14 papers · 1 filter

astro-ph.CO2022★ 20 cited

Calibrating cosmological simulations with implicit likelihood inference using galaxy growth observables

Yongseok Jo, Shy Genel, Benjamin Wandelt +7

In a novel approach employing implicit likelihood inference (ILI), also known as likelihood-free inference, we calibrate the parameters of cosmological hydrodynamic simulations aga…

astro-ph.GA2022★ 23 cited

Predicting sub-millimeter flux densities from global galaxy properties

R. K. Cochrane, C. C. Hayward, D. Angles-Alcazar +1

Recent years have seen growing interest in post-processing cosmological simulations with radiative transfer codes to predict observable fluxes for simulated galaxies. However, this…

astro-ph.GA2022★ 28 cited

Dust temperature uncertainties hamper the inference of dust and molecular gas masses from the dust continuum emission of quiescent high-redshift galaxies

R. K. Cochrane, C. C. Hayward, D. Anglés-Alcázar

Single flux density measurements at observed-frame sub-millimeter and millimeter wavelengths are commonly used to probe dust and gas masses in galaxies. In this Letter, we explore…

astro-ph.GA2022★ 1 cited

A unified model for the co-evolution of galaxies and their circumgalactic medium: the relative roles of turbulence and atomic cooling physics

Viraj Pandya, Drummond B. Fielding, Greg L. Bryan +7

The circumgalactic medium (CGM) plays a pivotal role in regulating gas flows around galaxies and thus shapes their evolution. However, the details of how galaxies and their CGM co-…

astro-ph.GA2022★ 32 cited

Stellar feedback-regulated black hole growth: driving factors from nuclear to halo scales

Lindsey Byrne, Claude-André Faucher-Giguère, Jonathan Stern +4

Several recent simulations of galaxy formation predict two main phases of supermassive black hole (BH) accretion: an early, highly intermittent phase (during which BHs are under-ma…

astro-ph.CO2022★ 1 cited

Robust field-level inference with dark matter halos

Helen Shao, Francisco Villaescusa-Navarro, Pablo Villanueva-Domingo +13

We train graph neural networks on halo catalogues from Gadget N-body simulations to perform field-level likelihood-free inference of cosmological parameters. The catalogues contain…

astro-ph.GA2022

Exploring supermassive black hole physics and galaxy quenching across halo mass in FIRE cosmological zoom simulations

Sarah Wellons, Claude-André Faucher-Giguère, Philip F. Hopkins +7

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

astro-ph.GA2022★ 139 cited

FIRE-3: Updated Stellar Evolution Models, Yields, & Microphysics and Fitting Functions for Applications in Galaxy Simulations

Philip F. Hopkins, Andrew Wetzel, Coral Wheeler +18

Increasingly, uncertainties in predictions from galaxy formation simulations (at sub-Milky Way masses) are dominated by uncertainties in stellar evolution inputs. In this paper, we…

astro-ph.GA2022★ 70 cited

Galaxies lacking dark matter produced by close encounters in a cosmological simulation

Jorge Moreno, Shany Danieli, James S. Bullock +18

The standard cold dark matter plus cosmological constant model predicts that galaxies form within dark-matter haloes, and that low-mass galaxies are more dark-matter dominated than…

astro-ph.GA2022★ 137 cited

Public data release of the FIRE-2 cosmological zoom-in simulations of galaxy formation

Andrew Wetzel, Christopher C. Hayward, Robyn E. Sanderson +23

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 R…

astro-ph.CO2022★ 69 cited

Co-evolution of massive black holes and their host galaxies at high redshift: discrepancies from six cosmological simulations and the key role of JWST

Melanie Habouzit, Masafusa Onoue, Eduardo Banados +7

The James Webb Space Telescope will have the power to characterize high-redshift quasars at z>6 with an unprecedented depth and spatial resolution. While the brightest quasars at s…

astro-ph.CO2022★ 2 cited

The Circumgalactic Medium from the CAMELS Simulations: Forecasting Constraints on Feedback Processes from Future Sunyaev-Zeldovich Observations

Emily Moser, Nicholas Battaglia, Daisuke Nagai +9

The cycle of baryons through the circumgalactic medium (CGM) is important to understand in the context of galaxy formation and evolution. In this study we forecast constraints on t…

astro-ph.GA2022

The black hole population in low-mass galaxies in large-scale cosmological simulations

Houda Haidar, Melanie Habouzit, Marta Volonteri +8

Recent systematic searches for massive black holes (BHs) in local dwarf galaxies led to the discovery of a population of faint Active Galactic Nuclei (AGN). We investigate the agre…

astro-ph.GA2022★ 95 cited

Hot-mode accretion and the physics of thin-disk galaxy formation

Zachary Hafen, Jonathan Stern, James Bullock +16

We use FIRE simulations to study disk formation in z~0, Milky Way-mass galaxies, and conclude that a key ingredient for the formation of thin stellar disks is the ability for accre…