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20072024
most citedA Multi-Code Analysis Toolkit for Astrophysical Simulation Data

1.2k citations · 5.9k across the 39 of their papers we have counts for

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Showing astro-ph.COShow all

12 papers · 1 filter

astro-ph.CO2016★ 343 cited

Grackle: a Chemistry and Cooling Library for Astrophysics

Britton D. Smith, Greg L. Bryan, Simon C. O. Glover +11

We present the Grackle chemistry and cooling library for astrophysical simulations and models. Grackle provides a treatment of non-equilibrium primordial chemistry and cooling for…

astro-ph.CO2014★ 84 cited

Dark Sky Simulations: Early Data Release

Samuel W. Skillman, Michael S. Warren, Matthew J. Turk +3

The Dark Sky Simulations are an ongoing series of cosmological N-body simulations designed to provide a quantitative and accessible model of the evolution of the large-scale Univer…

astro-ph.CO2014★ 392 cited

The Birth of a Galaxy - III. Propelling reionisation with the faintest galaxies

John H. Wise, Vasiliy G. Demchenko, Martin T. Halicek +4

Starlight from galaxies plays a pivotal role throughout the process of cosmic reionisation. We present the statistics of dwarf galaxy properties at z > 7 in haloes with masses up t…

astro-ph.CO2013★ 38 cited

Population III Star Formation In Large Cosmological Simulations I. Halo Temporal and Physical Environment

Brian D. Crosby, Brian W. O'Shea, Britton D. Smith +2

We present a semi-analytic, computationally inexpensive model to identify halos capable of forming a Population III star in cosmological simulations across a wide range of times an…

astro-ph.CO2012★ 176 cited

The Birth of a Galaxy. II. The Role of Radiation Pressure

John H. Wise, Tom Abel, Matthew J. Turk +2

Massive stars provide feedback that shapes the interstellar medium of galaxies at all redshifts and their resulting stellar populations. Here we present three adaptive mesh refinem…

astro-ph.CO2011★ 160 cited

Magnetic Fields in Population III Star Formation

Matthew J. Turk, Jeffrey S. Oishi, Tom Abel +1

We study the buildup of magnetic fields during the formation of Population III star-forming regions, by conducting cosmological simulations from realistic initial conditions and va…