activity
20142026
most citedThe Cosmic Baryon Cycle and Galaxy Mass Assembly in the FIRE Simulations

425 citations · 1.7k across the 43 of their papers we have counts for

collaborators
Showing 2021Show all

9 papers · 1 filter

astro-ph.GA2021★ 1 cited

Weighing the Milky Way and Andromeda with Artificial Intelligence

Pablo Villanueva-Domingo, Francisco Villaescusa-Navarro, Shy Genel +6

We present new constraints on the masses of the halos hosting the Milky Way and Andromeda galaxies derived using graph neural networks. Our models, trained on thousands of state-of…

astro-ph.GA2021★ 72 cited

Supermassive black holes in cosmological simulations II: the AGN population and predictions for upcoming X-ray missions

Melanie Habouzit, Rachel S. Somerville, Yuan Li +13

In large-scale hydrodynamical cosmological simulations, the fate of massive galaxies is mainly dictated by the modeling of feedback from active galactic nuclei (AGN). The amount of…

astro-ph.GA2021★ 27 cited

From EMBER to FIRE: predicting high resolution baryon fields from dark matter simulations with Deep Learning

Mauro Bernardini, Robert Feldmann, Daniel Anglés-Alcázar +4

Hydrodynamic simulations provide a powerful, but computationally expensive, approach to study the interplay of dark matter and baryons in cosmological structure formation. Here we…

astro-ph.CO2021★ 26 cited

HIFlow: Generating Diverse HI Maps and Inferring Cosmology while Marginalizing over Astrophysics using Normalizing Flows

Sultan Hassan, Francisco Villaescusa-Navarro, Benjamin Wandelt +11

A wealth of cosmological and astrophysical information is expected from many ongoing and upcoming large-scale surveys. It is crucial to prepare for these surveys now and develop to…

astro-ph.CO2021★ 19 cited

Multifield Cosmology with Artificial Intelligence

Francisco Villaescusa-Navarro, Daniel Anglés-Alcázar, Shy Genel +10

Astrophysical processes such as feedback from supernovae and active galactic nuclei modify the properties and spatial distribution of dark matter, gas, and galaxies in a poorly und…

astro-ph.GA2021★ 11 cited

Running Late: Testing Delayed Supermassive Black Hole Growth Models Against the Quasar Luminosity Function

Megan Taylor Tillman, Sarah Wellons, Claude-André Faucher-Giguère +2

Observations of massive galaxies at low redshift have revealed approximately linear scaling relations between the mass of a supermassive black hole (SMBH) and properties of its hos…

astro-ph.GA2021★ 3 cited

The origin of galaxy colour bimodality in the scatter of the Stellar-to-Halo Mass Relation

Weiguang Cui, Romeel Davé, John A. Peacock +2

Recent observations reveal that, at a given stellar mass, blue galaxies tend to live in haloes with lower mass while red galaxies live in more massive host haloes. The physical dri…

astro-ph.GA2021

IQ Collaboratory III: The Empirical Dust Attenuation Framework -- Taking Hydrodynamical Simulations with a Grain of Dust

ChangHoon Hahn, Tjitske K. Starkenburg, Daniel Anglés-Alcázar +8

We present the Empirical Dust Attenuation (EDA) framework -- a flexible prescription for assigning realistic dust attenuation to simulated galaxies based on their physical properti…

astro-ph.GA2021★ 82 cited

Which AGN Jets Quench Star Formation in Massive Galaxies?

Kung-Yi Su, Philip F. Hopkins, Greg L. Bryan +12

Without additional heating, radiative cooling of gas in the halos of massive galaxies (Milky Way and above) produces cold gas or stars in excess of that observed. Previous work sug…