The DOI matches its Crossref record; 338 of the 338 references it cites were found in a registry or an index.
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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Items 201–338 of 338
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Self-citationTHE IMPOSSIBLY EARLY GALAXY PROBLEM
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Self-citationIs main-sequence galaxy star formation controlled by halo mass accretion?
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THE SUBHALO-SATELLITE CONNECTION AND THE FATE OF DISRUPTED SATELLITE GALAXIES
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RAPID ENVIRONMENTAL QUENCHING OF SATELLITE DWARF GALAXIES IN THE LOCAL GROUP
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Self-citationCOSMOLOGICAL EVOLUTION OF LONG GAMMA-RAY BURSTS AND THE STAR FORMATION RATE
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The most massive galaxies and black holes allowed by ΛCDM
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Self-citationConnecting stellar mass and star-formation rate to dark matter halo mass out to z ∼ 2
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AN UNEXPECTEDLY LOW-REDSHIFT EXCESS OF SWIFT GAMMA-RAY BURST RATE
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Evolution of the atomic and molecular gas content of galaxies in dark matter haloes
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Self-citationA Theory for the Variation of Dust Attenuation Laws in Galaxies
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RECONCILING THE OBSERVED STAR-FORMING SEQUENCE WITH THE OBSERVED STELLAR MASS FUNCTION
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GAS LOSS BY RAM PRESSURE STRIPPING AND INTERNAL FEEDBACK FROM LOW-MASS MILKY WAY SATELLITES
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THE STELLAR MASS GROWTH OF BRIGHTEST CLUSTER GALAXIES IN THE IRAC SHALLOW CLUSTER SURVEY
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Demographics of Star-forming Galaxies since z ∼ 2.5. I. The UVJ Diagram in CANDELS
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Self-citationMajor mergers going Notts: challenges for modern halo finders
Behroozi, P., Knebe, A., Pearce, F. R., Elahi, P. J., Han, J., Lux, H., Mao, Y.-Y., Muldrew, S. I., Potter, D., & Srisawat, C. (2015) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stv2046 · Cited by 75
Self-citationELUCID. IV. Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias
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The Implications of a High Allelic Frequency of CYP2B6 G516T in Ethnic Chinese Persons
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Demographics of Star-forming Galaxies since z similar to 2.5. I. The UVJ Diagram in CANDELS
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An empirical model for the star formation history in dark matter haloes
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On the physical origin of galactic conformity
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Self-citationPRIMUS: GALAXY CLUSTERING AS A FUNCTION OF LUMINOSITY AND COLOR AT 0.2 <z< 1
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Self-citationAN INCREASING STELLAR BARYON FRACTION IN BRIGHT GALAXIES AT HIGH REDSHIFT
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Self-citationThe massive end of the stellar mass function
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AN HST /WFC3-UVIS VIEW OF THE STARBURST IN THE COOL CORE OF THE PHOENIX CLUSTER
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Self-citationPredicting galaxy star formation rates via the co-evolution of galaxies and haloes
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Self-citationEnvironmental quenching of low-mass field galaxies
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Subhalo demographics in the Illustris simulation: effects of baryons and halo-to-halo variation
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THE PHYSICAL NATURE OF THE COSMIC ACCRETION OF BARYONS AND DARK MATTER INTO HALOS AND THEIR GALAXIES
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HIERARCHICAL GALAXY GROWTH AND SCATTER IN THE STELLAR MASS–HALO MASS RELATION
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Self-citationThe agora high-resolution galaxy simulations comparison project. Ii. Isolated disk test
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A SIMPLE MODEL LINKING GALAXY AND DARK MATTER EVOLUTION
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THE PHYSICAL NATURE OF THE COSMIC ACCRETION OF BARYONS AND DARK MATTER INTO HALOS AND THEIR GALAXIES
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GLOBAL STAR FORMATION RATE DENSITY OVER 0.7 <z< 1.9
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- Silk, 1998, A&A, 331, L1
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Harikane, Y., Ouchi, M., Oguri, M., Ono, Y., Nakajima, K., Isobe, Y., Umeda, H., Mawatari, K., & Zhang, Y. (2023) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/acaaa9 · Cited by 651
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Naidu, R. P., Tacchella, S., Mason, C. A., Bose, S., Oesch, P. A., & Conroy, C. (2020) · The Astrophysical Journal · doi:10.3847/1538-4357/ab7cc9 · Cited by 310
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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
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