The DOI matches its Crossref record; 92 of the 92 references it cites were found in a registry or an index.
GALICS- I. A hybrid N-body/semi-analytic model of hierarchical galaxy formation
Open accessAbstract
This is the first paper of a series that describes the methods and basic results of the galics model (Galaxies In Cosmological Simulations). galics is a hybrid model for hierarchical galaxy formation studies, combining the outputs of large cosmological N-body simulations with simple, semi-analytic recipes to describe the fate of the baryons within dark matter haloes. The simulations produce a detailed merging tree for the dark matter haloes, including complete knowledge of the statistical properties arising from the gravitational forces. We intend to predict the overall statistical properties of galaxies, with special emphasis on the panchromatic spectral energy distribution emitted by galaxies in the ultraviolet/optical and infrared/submillimetre wavelength ranges. In this paper, we outline the physically motivated assumptions and key free parameters that go into the model, comparing and contrasting with other parallel efforts. We specifically illustrate the success of the model in comparison with several data sets, showing how it is able to predict the galaxy disc sizes, colours, luminosity functions from the ultraviolet to far infrared, the Tully–Fisher and Faber–Jackson relations, and the fundamental plane in the local Universe. We also identify certain areas where the model fails, or where the assumptions needed to succeed are at odds with observations, and pay special attention to understanding the effects of the finite resolution of the simulations on the predictions made. Other papers in this series will take advantage of different data sets available in the literature to extend the study of the limitations and predictive power of galics, with particular emphasis put on high-redshift galaxies.
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Cites
The Luminosity Function and Stellar Evolution.
Salpeter, E. E. (1955) · The Astrophysical Journal · doi:10.1086/145971 · Cited by 8,697
Formation of Galaxies and Clusters of Galaxies by Self-Similar Gravitational Condensation
Press, W. H., & Schechter, P. (1974) · The Astrophysical Journal · doi:10.1086/152650 · Cited by 4,916
The Demography of Massive Dark Objects in Galaxy Centers
Magorrian, J., Tremaine, S., Richstone, D., Bender, R., Bower, G., Dressler, A., Faber, S. M., Gebhardt, K., Green, R., Grillmair, C., et al. (1998) · The Astronomical Journal · doi:10.1086/300353 · Cited by 4,007
Core condensation in heavy halos: a two-stage theory for galaxy formation and clustering
White, S. D. M., & Rees, M. J. (1978) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/183.3.341 · Cited by 3,919
A hierarchical O(N log N) force-calculation algorithm
Barnes, J., & Hut, P. (1986) · Nature · doi:10.1038/324446a0 · Cited by 3,698
The evolution of large-scale structure in a universe dominated by cold dark matter
Davis, M., Efstathiou, G., Frenk, C. S., & White, S. D. M. (1985) · The Astrophysical Journal · doi:10.1086/163168 · Cited by 3,391
Optical properties of interstellar graphite and silicate grains
Draine, B. T., & Lee, H. M. (1984) · The Astrophysical Journal · doi:10.1086/162480 · Cited by 3,279
The statistics of peaks of Gaussian random fields
Bardeen, J. M., Bond, J. R., Kaiser, N., & Szalay, A. S. (1986) · The Astrophysical Journal · doi:10.1086/164143 · Cited by 3,270
An analytical model for spherical galaxies and bulges
Hernquist, L. (1990) · The Astrophysical Journal · doi:10.1086/168845 · Cited by 3,126
Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
Springel, V., White, S. D. M., Tormen, G., & Kauffmann, G. (2001) · Monthly Notices of the Royal Astronomical Society · doi:10.1046/j.1365-8711.2001.04912.x · Cited by 2,707
Cited by
The Epochs of Early‐Type Galaxy Formation as a Function of Environment
Thomas, D., Maraston, C., Bender, R., & de Oliveira, C. M. (2005) · The Astrophysical Journal · doi:10.1086/426932 · Cited by 1,620
The hierarchical formation of the brightest cluster galaxies
De Lucia, G., & Blaizot, J. (2007) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2006.11287.x · Cited by 1,613
Croton, D., Springel, V., White, S. D. M., Lucia, G. D., Frenk, C. S., Gao, L., Jenkins, A. R., Kauffmann, G., Navarro, J. F., & Yoshida, N. (2006) · Max Planck Digital Library · doi:10.25916/sut.26253068.v1 · Cited by 1,611
The EAGLE simulations of galaxy formation: calibration of subgrid physics and model variations
Crain, R. A., Schaye, J., Bower, R. G., Furlong, M., Schaller, M., Theuns, T., Dalla Vecchia, C., Frenk, C. S., McCarthy, I. G., Helly, J. C., et al. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv725 · Cited by 1,451
Galactic star formation and accretion histories from matching galaxies to dark matter haloes
Moster, B. P., Naab, T., & White, S. D. M. (2013) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/sts261 · Cited by 1,431
Metadata
- Authors
- Hatton, S., Devriendt, J. E. G., Ninin, S., Bouchet, F. R., Guiderdoni, B., & Vibert, D.
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2003-07-21
- Volume
- 343
- Issue
- 1
- Pages
- 75-106
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W1996522486
- Cited by
- 321
- References
- 92
- FWCI
- 15.08
- Type
- journal article
- Language
- en
- Open access
- hybrid
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- Hatton, S., Devriendt, J. E. G., Ninin, S., Bouchet, F. R., Guiderdoni, B., & Vibert, D. (2003). GALICS- I. A hybrid N-body/semi-analytic model of hierarchical galaxy formation. Monthly Notices of the Royal Astronomical Society. https://doi.org/10.1046/j.1365-8711.2003.05589.x
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Contains information from the Semantic Scholar Academic Graph Datasets, made available under the ODC Attribution License (ODC-BY 1.0).
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