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UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10
Open accessAbstract
We present a method to flexibly and self-consistently determine individual galaxies’ star formation rates (SFRs) from their host haloes’ potential well depths, assembly histories, and redshifts. The method is constrained by galaxies’ observed stellar mass functions, SFRs (specific and cosmic), quenched fractions, ultraviolet (UV) luminosity functions, UV–stellar mass relations, IRX–UV relations, auto- and cross-correlation functions (including quenched and star-forming subsamples), and quenching dependence on environment; each observable is reproduced over the full redshift range available, up to 0 < z < 10. Key findings include the following: galaxy assembly correlates strongly with halo assembly; quenching correlates strongly with halo mass; quenched fractions at fixed halo mass decrease with increasing redshift; massive quenched galaxies reside in higher-mass haloes than star-forming galaxies at fixed galaxy mass; star-forming and quenched galaxies’ star formation histories at fixed mass differ most at z < 0.5; satellites have large scatter in quenching time-scales after infall, and have modestly higher quenched fractions than central galaxies; Planck cosmologies result in up to 0.3 dex lower stellar – halo mass ratios at early times; and, none the less, stellar mass–halo mass ratios rise at z > 5. Also presented are revised stellar mass – halo mass relations for all, quenched, star-forming, central, and satellite galaxies; the dependence of star formation histories on halo mass, stellar mass, and galaxy SSFR; quenched fractions and quenching time-scale distributions for satellites; and predictions for higher-redshift galaxy correlation functions and weak lensing surface densities. The public data release (DR1) includes the massively parallel (>105 cores) implementation (the UniverseMachine), the newly compiled and remeasured observational data, derived galaxy formation constraints, and mock catalogues including lightcones.
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“(which is on the low side of, but consistent with the predictions for Milky Way-mass galaxies by Behroozi et al. 2019 and Moster et al. 2019, who find 1 5 10 9 M )”
From Kraken reveals itself – the merger history of the Milky Way reconstructed with the E-MOSAICS simulations (2020) · cites this paper as Behroozi et al. 2019
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Self-citationHalo Properties from Observable Measures of Environment: I. Halo and Subhalo Masses
Bowden, H., Behroozi, P., & Hearin, A. P. (2023) · The Open Journal of Astrophysics · doi:10.21105/astro.2307.07549 · Cited by 3
Self-citationCosmological prior for the J -factor estimation of dwarf spheroidal galaxies
Horigome, S.-I., Hayashi, K., & Ando, S. (2023) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.108.083530 · Cited by 3
O’Neil, S., Borrow, J., Vogelsberger, M., Zhao, H., & Wang, B. (2024) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stae990 · Cited by 3
Sabla, V. I., Bernal, J. L., Sato-Polito, G., & Kamionkowski, M. (2024) · Physical review. D/Physical review. D. · doi:10.1103/physrevd.110.023507 · Cited by 3
Momose, R., Lee, K., Ata, M., Horowitz, B., & Kartaltepe, J. S. (2024) · Publications of the Astronomical Society of Japan · doi:10.1093/pasj/psae076 · Cited by 3
The impact of large-scale structure on the anisotropic quenching of satellites
Zakharova, D., McGee, S., Vulcani, B., & Lucia, G. D. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202452296 · Cited by 3
Zhang, Z.-C., Bi, X.-J., & Yin, P. (2025) · Journal of Cosmology and Astroparticle Physics · doi:10.1088/1475-7516/2025/03/031 · Cited by 3
The impact of cosmic ray feedback during the epoch of reionisation
Farcy, M., Rosdahl, J., Dubois, Y., Blaizot, J., Martin-Alvarez, S., Haehnelt, M. G., Kimm, T., & Teyssier, R. (2025) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202553924 · Cited by 3
Contini, E., Yi, S. K., Rhee, J., & Jeon, S. (2025) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/addb4b · Cited by 3
Hagimoto, M., Tamura, Y., Inoue, A. K., Umehata, H., Bakx, T. J. L. C., Hashimoto, T., Mawatari, K., Sugahara, Y., Fudamoto, Y., Harikane, Y., et al. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/ade87e · Cited by 3
The Diversity of Environments around Luminous Quasars at Redshift z ∼ 6
Ren, K., Trenti, M., Marshall, M. A., Matteo, T. D., & Ni, Y. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac0ae2 · Cited by 3
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Cosmic Distributions of Stellar Tidal Disruptions by Massive Black Holes at Galactic Centers
Chen, Y., Yu, Q., & Lu, Y. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/aba950 · Cited by 3
O’Donnell, C., Behroozi, P., & More, S. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab3170 · Cited by 3
Self-citationEmpirical scenarios of galaxy evolution
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JWST reveals a possible z ∼ 11 galaxy merger in triply-lensed MACS0647–JDPreprint
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The Critical Role of Dark Matter Halos in Driving Star Formation*
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The dynamical evolution of the stellar clumps in the Sparkler galaxy
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Extended Star Formation in Luminous Infrared Galaxies at z ∼ 1 in the SMILES Field
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DESI Emission-line Galaxies: Clustering Dependence on Stellar Mass and [O II ] Luminosity
Hagen, T., Dawson, K., Zheng, Z., Aguilar, J., Ahlen, S. P., BenZvi, S., Bianchi, D., Brooks, D., Castander, F. J., Claybaugh, T., et al. (2025) · The Astrophysical Journal · doi:10.3847/1538-4357/ae0036 · Cited by 2
Metadata
- Authors
- Behroozi, P., Wechsler, R. H., Hearin, A. P., & Conroy, C.
- Affiliations
- University of Arizona (US)
- SLAC National Accelerator Laboratory (US)
- Argonne National Laboratory (US)
- Harvard University (US)
- Corresponding author
- Behroozi, Peter
- Venue
- Monthly Notices of the Royal Astronomical Society
- Publisher
- Oxford University Press (OUP)
- Published
- 2019-05-02
- Volume
- 488
- Issue
- 3
- Pages
- 3143-3194
- ISSN
- 0035-8711 (ISSN-L)
- 1365-2966
- OpenAlex
- W2809045192
- Cited by
- 1,243
- References
- 337
- Citations by year
- 2026: 111 · 2025: 222 · 2024: 207 · 2023: 170 · 2022: 187 · 2021: 145 · 2020: 133 · 2019: 66
- FWCI
- 70.86
- Type
- journal article
- Language
- en
- Open access
- green
- arxiv.org
- Licence
- academic.oup.com/journals/pages/open_access/funder_policies/chorus/standard_publication_model (vor)
- Locations
- Monthly Notices of the Royal Astronomical Society (publishedVersion)
- UA Campus Repository (The University of Arizona) (acceptedVersion)
- arXiv (Cornell University) (submittedVersion)
- OSTI OAI (U.S. Department of Energy Office of Scientific and Technical Information) (submittedVersion)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration (NAS5-26555)
- Space Telescope Science Institute (HST-HF2-51353.001-A)
- National Science Foundation (1066293, PHY11-25915)
- Deutsche Forschungsgemeinschaft (DE-AC02-76SF00515)
- U.S. Department of Energy (DE-AC02-05CH11231)
- University of Arizona
- University of California
- Alfred P. Sloan Foundation
- Brookhaven National Laboratory
- Carnegie Mellon University
- University of Florida
- Harvard University
- Johns Hopkins University
- Lawrence Berkeley National Laboratory
- New Mexico State University
- New York University
- Ohio State University
- Pennsylvania State University
- University of Portsmouth
- Princeton University
- University of Tokyo
- University of Utah
- Vanderbilt University
- University of Virginia
- University of Washington
- Yale University
- Science and Technology Facilities Council
- Australian Respiratory Council
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Galaxies: Formation, Evolution, Phenomena
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Cosmology and Gravitation Theories
- Keywords
- galaxy growth, star formation rate, galaxy quenching, stellar mass-halo mass relation, galaxy correlation function, stellar mass function, quenched fraction, star formation history, stellar mass surface density, high-redshift galaxy evolution
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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