The DOI matches its Crossref record; 8 of the 8 references it cites were found in a registry or an index.
THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT
Open accessAbstract
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 ≃ 10 10 , 10 11 , 10 12 , and 10 13 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 × 10 11 M ☉ by nine different versions of the participating codes is also presented to validate the infrastructure of the project.
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Citations
Cites
A Universal Density Profile from Hierarchical Clustering
Navarro, J. F., Frenk, C. S., & White, S. D. M. (1997) · The Astrophysical Journal · doi:10.1086/304888 · Cited by 9,917
The cosmological simulation code gadget-2
Springel, V. (2005) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09655.x · Cited by 6,368
THE AVERAGE STAR FORMATION HISTORIES OF GALAXIES IN DARK MATTER HALOS FROM z = 0-8
Behroozi, P. S., Wechsler, R. H., & Conroy, C. (2013) · The Astrophysical Journal · doi:10.1088/0004-637x/770/1/57 · Cited by 2,167
Self-citationInterstellar bubbles. II - Structure and evolution
Weaver, R., McCray, R., Castor, J., Shapiro, P., & Moore, R. (1977) · The Astrophysical Journal · doi:10.1086/155692 · Cited by 1,736 · cited 1×
“…clouds (Whitworth 1979; Matzner 2002; Dale et al. 2012), fast stellar winds that shock-heat the ISM and produce expanding bubbles (Castor et al. 1975; Weaver et al. 1977; Chevalier & Clegg 1985), the pressure of both direct starlight and dust-reprocessed radiation (Krumholz & Matzner 2009; Murray…”
BackgroundContraction of dark matter galactic halos due to baryonic infall
Blumenthal, G. R., Faber, S. M., Flores, R., & Primack, J. R. (1986) · The Astrophysical Journal · doi:10.1086/163867 · Cited by 1,213 · cited 1×
“It appears that compression of the central dark matter due to baryonic infall (e.g., Blumenthal et al. 1986; Gnedin et al. 2004, 2011) is an important effect in early-type galaxies, but this is apparently largely offset by other effects in late-type galaxies (e.g., Dutton et al. 2007;…”
BackgroundSelf-citationCastor, J., Weaver, R., & McCray, R. (1975) · The Astrophysical Journal · doi:10.1086/181908 · Cited by 670
The Initial‐Final Mass Relation: Direct Constraints at the Low‐Mass End
Kalirai, J. S., Hansen, B. M. S., Kelson, D. D., Reitzel, D. B., Rich, R. M., & Richer, H. B. (2008) · The Astrophysical Journal · doi:10.1086/527028 · Cited by 327
The H I halo in the inner galaxy
Lockman, F. J. (1984) · The Astrophysical Journal · doi:10.1086/162277 · Cited by 200 · cited 1×
“Yet, even at Eris’s resolution one barely resolves the vertical disk structure of the Milky Way since the Milky Way H I disk scale height is about 120 pc (Lockman 1984) and the H2 scale height is about 50 pc inside the solar circle (Sanders et al. 1984; Narayan & Jog 2002).”
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Cited by
Theoretical Challenges in Galaxy Formation
Naab, T., & Ostriker, J. P. (2017) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081913-040019 · Cited by 722
Read, J. I. (2014) · Journal of Physics G: Nuclear and Particle Physics · doi:10.1088/0954-3899/41/6/063101 · Cited by 489
Self-citationWainer, T. M., Williams, B. F., Johnson, L. C., Weisz, D. R., Dalcanton, J. J., Seth, A. C., Dolphin, A., Durbin, M. J., Bell, E. F., Chen, Z., et al. (2024) · The Astronomical Journal · doi:10.3847/1538-3881/ad5a6e · Cited by 4
Metadata
- Authors
- Kim, J.-H., Abel, T., Agertz, O., Bryan, G. L., Ceverino, D., Christensen, C., Conroy, C., Dekel, A., Gnedin, N. Y., Goldbaum, N. J., Guedes, J., Hahn, O., Hobbs, A., Hopkins, P. F., Hummels, C. B., Iannuzzi, F., Keres, D., Klypin, A., Kravtsov, A. V., Krumholz, M. R., Kuhlen, M., Leitner, S. N., Madau, P., Mayer, L., Moody, C. E., Nagamine, K., Norman, M. L., Onorbe, J., O'Shea, B. W., Pillepich, A., Primack, J. R., Quinn, T., Read, J. I., Robertson, B. E., Rocha, M., Rudd, D. H., Shen, S., Smith, B. D., Szalay, A. S., Teyssier, R., Thompson, R., Todoroki, K., Turk, M. J., Wadsley, J. W., Wise, J. H., Zolotov, A. A., & Collaboration29, F. T. A.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2013-12-24
- Volume
- 210
- Issue
- 1
- Pages
- 14
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2114564796
- Cited by
- 280
- References
- 8
- FWCI
- 15.86
- Type
- journal article
- Language
- en
- Open access
- bronze
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- Kim, J.-H., Abel, T., Agertz, O., Bryan, G. L., Ceverino, D., Christensen, C., Conroy, C., Dekel, A., Gnedin, N. Y., Goldbaum, N. J., Guedes, J., Hahn, O., Hobbs, A., Hopkins, P. F., Hummels, C. B., Iannuzzi, F., Keres, D., Klypin, A., Kravtsov, A. V., . . . Collaboration29, F. T. A. (2013). THE AGORA HIGH-RESOLUTION GALAXY SIMULATIONS COMPARISON PROJECT. The Astrophysical Journal Supplement Series. https://doi.org/10.1088/0067-0049/210/1/14
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