The DOI matches its Crossref record; 100 of the 100 references it cites were found in a registry or an index.
SEMI-ANALYTIC GALAXY EVOLUTION (SAGE): MODEL CALIBRATION AND BASIC RESULTS
Open accessAbstract
This paper describes a new publicly available codebase for modeling galaxy formation in a cosmological context, the “Semi-Analytic Galaxy Evolution” model, or sage for short.5 sage is a significant update to the 2006 model of Croton et al. and has been rebuilt to be modular and customizable. The model will run on any N-body simulation whose trees are organized in a supported format and contain a minimum set of basic halo properties. In this work, we present the baryonic prescriptions implemented in sage to describe the formation and evolution of galaxies, and their calibration for three N-body simulations: Millennium, Bolshoi, and GiggleZ. Updated physics include the following: gas accretion, ejection due to feedback, and reincorporation via the galactic fountain; a new gas cooling–radio mode active galactic nucleus (AGN) heating cycle; AGN feedback in the quasar mode; a new treatment of gas in satellite galaxies; and galaxy mergers, disruption, and the build-up of intra-cluster stars. Throughout, we show the results of a common default parameterization on each simulation, with a focus on the local galaxy population.
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Planck 2015 results. XIII. Cosmological parameters
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The Sloan Digital Sky Survey: Technical Summary
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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
On the variation of the initial mass function
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The cosmological simulation code gadget-2
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FIVE-YEAR WILKINSON MICROWAVE ANISOTROPY PROBE OBSERVATIONS: COSMOLOGICAL INTERPRETATION
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THE SEVENTH DATA RELEASE OF THE SLOAN DIGITAL SKY SURVEY
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The Global Schmidt Law in Star‐forming Galaxies
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Simulations of the formation, evolution and clustering of galaxies and quasars
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Cited by
Simulating galaxy formation with the IllustrisTNG model
Pillepich, A., Springel, V., Nelson, D., Genel, S., Naiman, J., Pakmor, R., Hernquist, L., Torrey, P., Vogelsberger, M., Weinberger, R., et al. (2018) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx2656 · Cited by 2,007
UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
Behroozi, P., Wechsler, R. H., Hearin, A. P., & Conroy, C. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz1182 · Cited by 1,243
Metadata
- Authors
- Croton, D. J., Stevens, A. R. H., Tonini, C., Garel, T., Bernyk, M., Bibiano, A., Hodkinson, L., Mutch, S. J., Poole, G. B., & Shattow, G. M.
- Venue
- The Astrophysical Journal Supplement Series
- Publisher
- American Astronomical Society
- Published
- 2016-02-01
- Volume
- 222
- Issue
- 2
- Pages
- 22
- ISSN
- 0067-0049 (ISSN-L)
- 1538-4365
- OpenAlex
- W2268627276
- Cited by
- 264
- References
- 100
- FWCI
- 16.28
- Type
- journal article
- Language
- en
- Open access
- bronze
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- CoChat. (2026). Citation check: SEMI-ANALYTIC GALAXY EVOLUTION (SAGE): MODEL CALIBRATION AND BASIC RESULTS. https://app.cochat.ai/papers/10.3847/0067-0049/222/2/22
- The paper
- Croton, D. J., Stevens, A. R. H., Tonini, C., Garel, T., Bernyk, M., Bibiano, A., Hodkinson, L., Mutch, S. J., Poole, G. B., & Shattow, G. M. (2016). SEMI-ANALYTIC GALAXY EVOLUTION (SAGE): MODEL CALIBRATION AND BASIC RESULTS. The Astrophysical Journal Supplement Series. https://doi.org/10.3847/0067-0049/222/2/22
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