activity
20082026
most citedIntroducing the Illustris Project: Simulating the coevolution of dark and visible matter in the Universe

2.3k citations · 36.1k across the 179 of their papers we have counts for

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Showing astro-ph.COShow all

70 papers · 1 filter

astro-ph.CO2026

BINDing the lightcone: A suite of astrophysical ray-traced weak lensing and SZ maps

Max E. Lee, Shy Genel, Zoltan Haiman +2

Recent multiwavelength observations of galaxy group and cluster gas suggest stronger baryonic feedback than our best-calibrated hydrodynamical simulations produce, while modeling t…

astro-ph.CO2026

Inductive Biases in Field-Level Cosmological Inference from Galaxy Catalogs

James O. Baldwin, Shy Genel, Francisco Villaescusa-Navarro

We perform field-level likelihood-free inference of the matter density parameter from simulated galaxy catalogs using machine learning models with differing inductive biases.…

astro-ph.CO2026

Learning the Universe with cosmological rescaling of merger trees and semi-analytic galaxy formation models

Richard Stiskalek, Lucia A. Perez, Shy Genel +3

Learning cosmology from galaxy surveys requires large suites of simulations spanning the cosmological and astrophysical parameter space, yet hydrodynamical simulations of galaxy fo…

astro-ph.CO2026

Learning the Universe with the 2nd Generation of CAMELS: Varying 35 parameters of the IllustrisTNG model in (50Mpc/h)^3 boxes

Shy Genel, Yongseok Jo, Boon Kiat Oh +10

We present a new set of 1,192 cosmological simulations as part of the CAMELS project, in which a space of 35 cosmological, astrophysical, and numerical parameters is explored aroun…

astro-ph.CO2026

Efficiently emulating distribution functions in gigaparsec volumes for varying cosmological parameters

Christopher C. Lovell, Max E. Lee, William J. Roper +4

We present a new method for emulating the halo mass function (HMF) and other distribution functions in large effective volumes, down to low halo masses, whilst simultaneously modif…

astro-ph.CO2026

The impact of baryons on weak lensing statistics as a function of halo mass and radius

Max E. Lee, Zoltan Haiman, Shy Genel

Upcoming weak lensing (WL) surveys such as those by {\it Euclid}, LSST, and {\it Roman} require percent-level control over systematic effects. A common approach to mitigating baryo…