The DOI matches its Crossref record; 129 of the 129 references it cites were found in a registry or an index.
The bahamas project: calibrated hydrodynamical simulations for large-scale structure cosmology
Open accessAbstract
The evolution of the large-scale distribution of matter is sensitive to a variety of fundamental parameters that characterize the dark matter, dark energy, and other aspects of our cosmological framework. Since the majority of the mass density is in the form of dark matter that cannot be directly observed, to do cosmology with large-scale structure, one must use observable (baryonic) quantities that trace the underlying matter distribution in a (hopefully) predictable way. However, recent numerical studies have demonstrated that the mapping between observable and total mass, as well as the total mass itself, are sensitive to unresolved feedback processes associated with galaxy formation, motivating explicit calibration of the feedback efficiencies. Here, we construct a new suite of large-volume cosmological hydrodynamical simulations (called bahamas, for BAryons and HAloes of MAssive Systems), where subgrid models of stellar and active galactic nucleus feedback have been calibrated to reproduce the present-day galaxy stellar mass function and the hot gas mass fractions of groups and clusters in order to ensure the effects of feedback on the overall matter distribution are broadly correct. We show that the calibrated simulations reproduce an unprecedentedly wide range of properties of massive systems, including the various observed mappings between galaxies, hot gas, total mass, and black holes, and represent a significant advance in our ability to mitigate the primary systematic uncertainty in most present large-scale structure tests.
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Cites
Galactic Stellar and Substellar Initial Mass Function
Chabrier, G. (2003) · Publications of the Astronomical Society of the Pacific · doi:10.1086/376392 · Cited by 9,071
STAR FORMATION IN GALAXIES ALONG THE HUBBLE SEQUENCE
Kennicutt, R. C. (1998) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev.astro.36.1.189 · Cited by 6,578
Planck 2013 results. XVI. Cosmological parameters
Planck Collaboration, Ade, P. A. R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A. J., et al. (2014) · Astronomy & Astrophysics · doi:10.1051/0004-6361/201321591 · Cited by 6,521
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
NINE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE ( WMAP ) OBSERVATIONS: COSMOLOGICAL PARAMETER RESULTS
Hinshaw, G., Larson, D., Komatsu, E., Spergel, D. N., Bennett, C. L., Dunkley, J., Nolta, M. R., Halpern, M., Hill, R. S., Odegard, N., et al. (2013) · The Astrophysical Journal Supplement Series · doi:10.1088/0067-0049/208/2/19 · Cited by 5,121
Galactic Stellar and Substellar Initial Mass FunctionPreprint
Chabrier, G. (2003) · Cited by 4,970
Lewis, A., Challinor, A., & Lasenby, A. (2000) · The Astrophysical Journal · doi:10.1086/309179 · Cited by 4,920
Astronomical Data Analysis Software and Systems
Argyle, R. W., Bunclark, P., & Lewis, J. R. (2008) · Cited by 4,399
The cosmological simulation code GADGET-2
Petkova, M., & Springel, V. (2005) · Cited by 3,918
Star Formation in Galaxies Along the Hubble Sequence
Kennicutt, R. C., & Words, K. (1998) · Cited by 3,712
Cited by
simba: Cosmological simulations with black hole growth and feedback
Davé, R., Anglés-Alcázar, D., Narayanan, D., Li, Q., Rafieferantsoa, M. H., & Appleby, S. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz937 · Cited by 1,111
Euclid: I. Overview of the Euclid mission
Euclid Collaboration, Mellier, Y., Abdurro’uf, Acevedo Barroso, J. A., Achúcarro, A., Adamek, J., Adam, R., Addison, G. E., Aghanim, N., Aguena, M., et al. (2025) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202450810 · Cited by 616
Self-citationThe CAMELS Project: Cosmology and Astrophysics with Machine-learning Simulations
Villaescusa-Navarro, F., Anglés-Alcázar, D., Genel, S., Spergel, D. N., S. Somerville, R., Dave, R., Pillepich, A., Hernquist, L., Nelson, D., Torrey, P., et al. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/abf7ba · Cited by 304
Davies, J. J., Crain, R. A., Oppenheimer, B. D., & Schaye, J. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz3201 · Cited by 167
Self-citationNelson, D., Pillepich, A., Ayromlou, M., Lee, W., Lehle, K., Rohr, E., & Truong, N. (2024) · Astronomy & Astrophysics · doi:10.1051/0004-6361/202348608 · Cited by 110
Metadata
- Authors
- McCarthy, I. G., Schaye, J., Bird, S., & Le Brun, A. M. C.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2016-10-30
- Volume
- 465
- Issue
- 3
- Pages
- 2936-2965
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2296455390
- Cited by
- 502
- References
- 129
- FWCI
- 14.00
- Type
- journal article
- Language
- en
- Open access
- green
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