The AGORA high-resolution galaxy simulations comparison project

Ji Hoon Kim, Tom Abel, Oscar Agertz, Greg L. Bryan, Daniel Ceverino, Charlotte Christensen, Charlie Conroy, Avishai Dekel, Nickolay Y. Gnedin, Nathan J. Goldbaum, Javiera Guedes, Oliver Hahn, Alexander Hobbs, Philip F. Hopkins, Cameron B. Hummels, Francesca Iannuzzi, Dusan Keres, Anatoly Klypin, Andrey V. Kravtsov, Mark R. KrumholzMichael Kuhlen, Samuel N. Leitner, Piero Madau, Lucio Mayer, Christopher E. Moody, Kentaro Nagamine, Michael L. Norman, Jose Onorbe, Brian W. O'Shea, Annalisa Pillepich, Joel R. Primack, Thomas Quinn, Justin I. Read, Brant E Robertson, Miguel Rocha, Douglas H. Rudd, Sijing Shen, Britton D. Smith, Alexander S. Szalay, Romain Teyssier, Robert Thompson, Keita Todoroki, Matthew J. Turk, James W. Wadsley, John H. Wise, Adi Zolotov

Research output: Contribution to journalArticle

128 Citations (Scopus)

Abstract

We introduce the Assembling Galaxies Of Resolved Anatomy (AGORA) project, a comprehensive numerical study of well-resolved galaxies within the ΛCDM cosmology. Cosmological hydrodynamic simulations with force resolutions of 100 proper pc or better will be run with a variety of code platforms to follow the hierarchical growth, star formation history, morphological transformation, and the cycle of baryons in and out of eight galaxies with halo masses M vir ≃ 1010, 1011, 1012, and 1013 M at z = 0 and two different ("violent" and "quiescent") assembly histories. The numerical techniques and implementations used in this project include the smoothed particle hydrodynamics codes GADGET and GASOLINE, and the adaptive mesh refinement codes ART, ENZO, and RAMSES. The codes share common initial conditions and common astrophysics packages including UV background, metal-dependent radiative cooling, metal and energy yields of supernovae, and stellar initial mass function. These are described in detail in the present paper. Subgrid star formation and feedback prescriptions will be tuned to provide a realistic interstellar and circumgalactic medium using a non-cosmological disk galaxy simulation. Cosmological runs will be systematically compared with each other using a common analysis toolkit and validated against observations to verify that the solutions are robust - i.e., that the astrophysical assumptions are responsible for any success, rather than artifacts of particular implementations. The goals of the AGORA project are, broadly speaking, to raise the realism and predictive power of galaxy simulations and the understanding of the feedback processes that regulate galaxy "metabolism." The initial conditions for the AGORA galaxies as well as simulation outputs at various epochs will be made publicly available to the community. The proof-of-concept dark-matter-only test of the formation of a galactic halo with a z = 0 mass of M vir ≃ 1.7 × 1011 M by nine different versions of the participating codes is also presented to validate the infrastructure of the project.

Original languageEnglish (US)
Article number14
JournalAstrophysical Journal, Supplement Series
Volume210
Issue number1
DOIs
StatePublished - Jan 2014

Fingerprint

anatomy
assembling
galaxies
high resolution
simulation
hydrodynamics
metal
astrophysics
star formation
cosmology
history
histories
artifact
metabolism
infrastructure
code
project
comparison
galactic halos
disk galaxies

Keywords

  • cosmology: theory
  • dark matter
  • galaxies: evolution
  • galaxies: formation
  • hydrodynamics
  • methods: numerical

ASJC Scopus subject areas

  • Space and Planetary Science
  • Astronomy and Astrophysics

Cite this

Kim, J. H., Abel, T., Agertz, O., Bryan, G. L., Ceverino, D., Christensen, C., ... Zolotov, A. (2014). The AGORA high-resolution galaxy simulations comparison project. Astrophysical Journal, Supplement Series, 210(1), [14]. https://doi.org/10.1088/0067-0049/210/1/14

The AGORA high-resolution galaxy simulations comparison project. / Kim, Ji Hoon; Abel, Tom; Agertz, Oscar; Bryan, Greg L.; Ceverino, Daniel; Christensen, Charlotte; Conroy, Charlie; Dekel, Avishai; Gnedin, Nickolay Y.; Goldbaum, Nathan J.; Guedes, Javiera; Hahn, Oliver; Hobbs, Alexander; Hopkins, Philip F.; Hummels, Cameron B.; Iannuzzi, Francesca; Keres, Dusan; Klypin, Anatoly; Kravtsov, Andrey V.; Krumholz, Mark R.; Kuhlen, Michael; Leitner, Samuel N.; Madau, Piero; Mayer, Lucio; Moody, Christopher E.; Nagamine, Kentaro; Norman, Michael L.; Onorbe, Jose; O'Shea, Brian W.; Pillepich, Annalisa; Primack, Joel R.; Quinn, Thomas; Read, Justin I.; Robertson, Brant E; Rocha, Miguel; Rudd, Douglas H.; Shen, Sijing; Smith, Britton D.; Szalay, Alexander S.; Teyssier, Romain; Thompson, Robert; Todoroki, Keita; Turk, Matthew J.; Wadsley, James W.; Wise, John H.; Zolotov, Adi.

In: Astrophysical Journal, Supplement Series, Vol. 210, No. 1, 14, 01.2014.

Research output: Contribution to journalArticle

Kim, JH, Abel, T, Agertz, O, Bryan, GL, Ceverino, D, Christensen, C, Conroy, C, Dekel, A, Gnedin, NY, Goldbaum, NJ, Guedes, J, Hahn, O, Hobbs, A, Hopkins, PF, Hummels, CB, Iannuzzi, F, Keres, D, Klypin, A, Kravtsov, AV, Krumholz, MR, Kuhlen, M, Leitner, SN, Madau, P, Mayer, L, Moody, CE, Nagamine, K, Norman, ML, Onorbe, J, O'Shea, BW, Pillepich, A, Primack, JR, Quinn, T, Read, JI, Robertson, BE, Rocha, M, Rudd, DH, Shen, S, Smith, BD, Szalay, AS, Teyssier, R, Thompson, R, Todoroki, K, Turk, MJ, Wadsley, JW, Wise, JH & Zolotov, A 2014, 'The AGORA high-resolution galaxy simulations comparison project', Astrophysical Journal, Supplement Series, vol. 210, no. 1, 14. https://doi.org/10.1088/0067-0049/210/1/14
Kim, Ji Hoon ; Abel, Tom ; Agertz, Oscar ; Bryan, Greg L. ; Ceverino, Daniel ; Christensen, Charlotte ; Conroy, Charlie ; Dekel, Avishai ; Gnedin, Nickolay Y. ; Goldbaum, Nathan J. ; Guedes, Javiera ; Hahn, Oliver ; Hobbs, Alexander ; Hopkins, Philip F. ; Hummels, Cameron B. ; Iannuzzi, Francesca ; Keres, Dusan ; Klypin, Anatoly ; Kravtsov, Andrey V. ; Krumholz, Mark R. ; Kuhlen, Michael ; Leitner, Samuel N. ; Madau, Piero ; Mayer, Lucio ; Moody, Christopher E. ; Nagamine, Kentaro ; Norman, Michael L. ; Onorbe, Jose ; O'Shea, Brian W. ; Pillepich, Annalisa ; Primack, Joel R. ; Quinn, Thomas ; Read, Justin I. ; Robertson, Brant E ; Rocha, Miguel ; Rudd, Douglas H. ; Shen, Sijing ; Smith, Britton D. ; Szalay, Alexander S. ; Teyssier, Romain ; Thompson, Robert ; Todoroki, Keita ; Turk, Matthew J. ; Wadsley, James W. ; Wise, John H. ; Zolotov, Adi. / The AGORA high-resolution galaxy simulations comparison project. In: Astrophysical Journal, Supplement Series. 2014 ; Vol. 210, No. 1.
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AU - Christensen, Charlotte

AU - Conroy, Charlie

AU - Dekel, Avishai

AU - Gnedin, Nickolay Y.

AU - Goldbaum, Nathan J.

AU - Guedes, Javiera

AU - Hahn, Oliver

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AU - Robertson, Brant E

AU - Rocha, Miguel

AU - Rudd, Douglas H.

AU - Shen, Sijing

AU - Smith, Britton D.

AU - Szalay, Alexander S.

AU - Teyssier, Romain

AU - Thompson, Robert

AU - Todoroki, Keita

AU - Turk, Matthew J.

AU - Wadsley, James W.

AU - Wise, John H.

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N2 - We introduce the Assembling Galaxies Of Resolved Anatomy (AGORA) project, a comprehensive numerical study of well-resolved galaxies within the ΛCDM cosmology. Cosmological hydrodynamic simulations with force resolutions of 100 proper pc or better will be run with a variety of code platforms to follow the hierarchical growth, star formation history, morphological transformation, and the cycle of baryons in and out of eight galaxies with halo masses M vir ≃ 1010, 1011, 1012, and 1013 M at z = 0 and two different ("violent" and "quiescent") assembly histories. The numerical techniques and implementations used in this project include the smoothed particle hydrodynamics codes GADGET and GASOLINE, and the adaptive mesh refinement codes ART, ENZO, and RAMSES. The codes share common initial conditions and common astrophysics packages including UV background, metal-dependent radiative cooling, metal and energy yields of supernovae, and stellar initial mass function. These are described in detail in the present paper. Subgrid star formation and feedback prescriptions will be tuned to provide a realistic interstellar and circumgalactic medium using a non-cosmological disk galaxy simulation. Cosmological runs will be systematically compared with each other using a common analysis toolkit and validated against observations to verify that the solutions are robust - i.e., that the astrophysical assumptions are responsible for any success, rather than artifacts of particular implementations. The goals of the AGORA project are, broadly speaking, to raise the realism and predictive power of galaxy simulations and the understanding of the feedback processes that regulate galaxy "metabolism." The initial conditions for the AGORA galaxies as well as simulation outputs at various epochs will be made publicly available to the community. The proof-of-concept dark-matter-only test of the formation of a galactic halo with a z = 0 mass of M vir ≃ 1.7 × 1011 M by nine different versions of the participating codes is also presented to validate the infrastructure of the project.

AB - We introduce the Assembling Galaxies Of Resolved Anatomy (AGORA) project, a comprehensive numerical study of well-resolved galaxies within the ΛCDM cosmology. Cosmological hydrodynamic simulations with force resolutions of 100 proper pc or better will be run with a variety of code platforms to follow the hierarchical growth, star formation history, morphological transformation, and the cycle of baryons in and out of eight galaxies with halo masses M vir ≃ 1010, 1011, 1012, and 1013 M at z = 0 and two different ("violent" and "quiescent") assembly histories. The numerical techniques and implementations used in this project include the smoothed particle hydrodynamics codes GADGET and GASOLINE, and the adaptive mesh refinement codes ART, ENZO, and RAMSES. The codes share common initial conditions and common astrophysics packages including UV background, metal-dependent radiative cooling, metal and energy yields of supernovae, and stellar initial mass function. These are described in detail in the present paper. Subgrid star formation and feedback prescriptions will be tuned to provide a realistic interstellar and circumgalactic medium using a non-cosmological disk galaxy simulation. Cosmological runs will be systematically compared with each other using a common analysis toolkit and validated against observations to verify that the solutions are robust - i.e., that the astrophysical assumptions are responsible for any success, rather than artifacts of particular implementations. The goals of the AGORA project are, broadly speaking, to raise the realism and predictive power of galaxy simulations and the understanding of the feedback processes that regulate galaxy "metabolism." The initial conditions for the AGORA galaxies as well as simulation outputs at various epochs will be made publicly available to the community. The proof-of-concept dark-matter-only test of the formation of a galactic halo with a z = 0 mass of M vir ≃ 1.7 × 1011 M by nine different versions of the participating codes is also presented to validate the infrastructure of the project.

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