UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10

Behroozi, Peter; Wechsler, Risa H; Hearin, Andrew P; Conroy, Charlie

doi:10.1093/mnras/stz1182

Cited by 1,243Galaxies: Formation, Evolution, PhenomenaStellar, planetary, and galactic studiesCosmology and Gravitation Theories

UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10

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Behroozi, Peter, Wechsler, Risa H, Hearin, Andrew P, Conroy, Charlie·2019·Monthly Notices of the Royal Astronomical Society

DOI 10.1093/mnras/stz1182

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Abstract

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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The total accreted stellar mass 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 Msun.
“(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
Section 4.8 (p. 19) predicts the fraction of stellar mass formed ex situ through mergers as a function of halo mass, and the Figure 27 caption (p. 19) identifies that fraction as merger-accreted mass. Our copy does not give the claimed total of 1–5 × 10^9 solar masses for Milky Way-mass galaxies, so it cannot verify that numerical prediction. (LLM, conf=0.81)
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Calzetti D., 2001, New Astronomy Review, 45, 601
Haario H., Saksman E., Tamminen J., 2001, Bernoulli, 7, pp. 223
Kravtsov A. V., Vikhlinin A. A., Meshcheryakov A. V., 2018, Astronomy Letters, 44, 8
Wechsler R. H., Tinker J. L., 2018, Annual Review of Astronomy and Astrophysics, 56, 435

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“…been identified), implying that the total accreted stellar mass is likely to be close to the sum of the five satellites discussed here (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× 109 M ).”
Result
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Key Physical Processes in the Circumgalactic Medium
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Angulo, R., & Hahn, O. (2021) · Living Reviews in Computational Astrophysics · doi:10.1007/s41115-021-00013-z · Cited by 119 · see citing works
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Bursty Star Formation Naturally Explains the Abundance of Bright Galaxies at Cosmic Dawn
Sun, G., Faucher‐Giguère, C., Hayward, C. C., Shen, X., Wetzel, A. R., & Cochrane, R. K. (2023) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/acf85a · Cited by 170 · see citing works
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Fujimoto, S., Haro, P. A., Dickinson, M., Finkelstein, S. L., Kartaltepe, J. S., Larson, R. L., Burgarella, D., Bagley, M. B., Behroozi, P., Chworowsky, K., et al. (2023) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/acd2d9 · Cited by 165 · see citing works
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The ALPINE-ALMA [C II] survey: Star-formation-driven outflows and circumgalactic enrichment in the early Universe
Ginolfi, M., Jones, G. C., Béthermin, M., Fudamoto, Y., Loiacono, F., Fujimoto, S., Fèvre, O. C. L., Faisst, A. L., Schaerer, D., Cassata, P., et al. (2019) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201936872 · Cited by 164 · see citing works
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Naidu, R. P., Conroy, C., Bonaca, A., Zaritsky, D., Weinberger, R., Ting, Y.-S., Caldwell, N., Tacchella, S., Han, J., Speagle, J. S., et al. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac2d2d · Cited by 164 · see citing works
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HERA Phase I Limits on the Cosmic 21 cm Signal: Constraints on Astrophysics and Cosmology during the Epoch of Reionization
Abdurashidova, Z., Aguirre, J., Alexander, P. E., Ali, Z. S., Balfour, Y., Barkana, R., Beardsley, A. P., Bernardi, G., Billings, T. S., Bowman, J. D., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac2ffc · Cited by 160 · see citing works
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A dark matter profile to model diverse feedback-induced core sizes of ΛCDM haloes
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Endsley, R., Stark, D. P., Chevallard, J., & Charlot, S. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa3370 · Cited by 156 · see citing works
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de Graaff, A., Rix, H., Carniani, S., Suess, K. A., Charlot, S., Curtis-Lake, E., Arribas, S., Baker, W. M., Boyett, K., Bunker, A. J., et al. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202347755 · Cited by 156 · see citing works
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Danieli, S., van Dokkum, P., Conroy, C., Abraham, R. G., & Romanowsky, A. J. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab0e8c · Cited by 150 · see citing works
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Evolution of the galaxy stellar mass functions and UV luminosity functions at z = 6−9 in the Hubble Frontier Fields
Bhatawdekar, R., Conselice, C. J., Margalef-Bentabol, B., & Duncan, K. J. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz866 · Cited by 149 · see citing works
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Simulating the interstellar medium and stellar feedback on a moving mesh: implementation and isolated galaxies
Marinacci, F., Sales, L., Vogelsberger, M., Torrey, P., & Springel, V. (2019) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2391 · Cited by 75 · see citing works
FIRE-3: updated stellar evolution models, yields, and microphysics and fitting functions for applications in galaxy simulations
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Hydrodynamical Simulations of the Galaxy Population: Enduring Successes and Outstanding Challenges
Crain, R. A., & van de Voort, F. (2023) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-041923-043618 · Cited by 138 · see citing works
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An observational determination of the evolving extragalactic background light from the multiwavelength HST /CANDELS survey in the Fermi and CTA era
Saldana-Lopez, A., Domínguez, A., Pérez‐González, P. G., Finke, J. D., Ajello, M., Primack, J. R., Paliya, V. S., & Desai, A. (2021) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stab2393 · Cited by 137 · see citing works
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The Universe at z > 10: predictions for JWST from the universemachine DR1
Behroozi, P., Conroy, C., Wechsler, R. H., Hearin, A. P., Williams, C. C., Moster, B. P., Yung, L. Y. A., Somerville, R. S., Gottlöber, S., Yepes, G., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa3164 · Cited by 134 · see citing works
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Public Data Release of the FIRE-2 Cosmological Zoom-in Simulations of Galaxy Formation
Wetzel, A. R., Hayward, C. C., Sanderson, R. E., Ma, X., Anglés‐Alcázar, D., Feldmann, R., Chan, T. K., El-Badry, K., Wheeler, C., Garrison-Kimmel, S., et al. (2023) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/acb99a · Cited by 134 · see citing works
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A massive galaxy that formed its stars at z ≈ 11
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Muñoz, J. B., Qin, Y., Mesinger, A., Murray, S., Greig, B., & Mason, C. A. (2021) · Research at the University of Copenhagen (University of Copenhagen) · doi:10.1093/mnras/stac185 · Cited by 123 · see citing works
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de Graaff, A., Setton, D., Brammer, G., Cutler, S. E., Suess, K., Labb'e, I., Leja, J., Weibel, A., Maseda, M., Whitaker, K., et al. (2024) · Nature Astronomy · doi:10.1038/s41550-024-02424-3 · Cited by 92 · see citing works
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The JWST-PRIMAL archival survey
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Yung, L. Y. A., Somerville, R., Popping, G., Finkelstein, S., Ferguson, H., & Dave, R. (2019) · Monthly notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2755 · Cited by 76 · see citing works
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Mirocha, J. T., & Furlanetto, S. R. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3578 · Cited by 114 · see citing works
CCAT-prime Collaboration: Science Goals and Forecasts with Prime-Cam on the Fred Young Submillimeter Telescope
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Iyer, K. G., Tacchella, S., Genel, S., Hayward, C. C., Hernquist, L., Brooks, A. M., Čaplar, N., Davé, R., Diemer, B., Forbes, J. C., et al. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2150 · Cited by 112 · see citing works
The evolution of the galaxy stellar-mass function over the last 12 billion years from a combination of ground-based and HST surveys
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Trebitsch, M., Dubois, Y., Volonteri, M., Pfister, H., Cadiou, C., Katz, H., Rosdahl, J., Kimm, T., Pichon, C., Beckmann, R. S., et al. (2021) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202037698 · Cited by 110 · see citing works
SILVERRUSH. VIII. Spectroscopic Identifications of Early Large-scale Structures with Protoclusters over 200 Mpc at z ∼ 6–7: Strong Associations of Dusty Star-forming Galaxies
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Quenching as a Contest between Galaxy Halos and Their Central Black Holes
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A Search for H-Dropout Lyman Break Galaxies at z ∼ 12–16
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LyC escape from sphinx galaxies in the Epoch of Reionization
Rosdahl, J., Blaizot, J., Katz, H., Kimm, T., Garel, T., Haehnelt, M. G., Keating, L. C., Martin-Alvarez, S., Michel-Dansac, L., & Ocvirk, P. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1942 · Cited by 107 · see citing works
The chemo-dynamical groups of Galactic globular clusters
Callingham, T. M., Cautun, M., Deason, A. J., Frenk, C. S., Grand, R. J. J., & Marinacci, F. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1145 · Cited by 102 · see citing works
A survey of high- z galaxies: SERRA simulations
Pallottini, A., Ferrara, A., Gallerani, S., Behrens, C., Kohandel, M., Carniani, S., Vallini, L., Salvadori, S., Gelli, V., Sommovigo, L., et al. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac1281 · Cited by 102 · see citing works
Cooling flow solutions for the circumgalactic medium
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Introducing the TNG-Cluster simulation: Overview and the physical properties of the gaseous intracluster medium
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The MillenniumTNG project: the galaxy population at z ≥ 8
Kannan, R., Springel, V., Hernquist, L., Pakmor, R., Delgado, A. M., Hadzhiyska, B., Hernández‐Aguayo, C., Barrera, M., Ferlito, F., Bose, S., et al. (2022) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stac3743 · Cited by 100 · see citing works
A Mass-dependent Slope of the Galaxy Size–Mass Relation out to z ∼ 3: Further Evidence for a Direct Relation between Median Galaxy Size and Median Halo Mass
Mowla, L., van der Wel, A., van Dokkum, P., & Miller, T. B. (2019) · The Astrophysical Journal Letters · doi:10.3847/2041-8213/ab0379 · Cited by 99 · see citing works
The BUFFALO HST Survey
Steinhardt, C. L., Jauzac, M., Acebrón, A., Atek, H., Capak, P. L., Davidzon, I., Eckert, D., Harvey, D., Koekemoer, A. M., Lagos, C. D. P., et al. (2020) · The Astrophysical Journal Supplement Series · doi:10.3847/1538-4365/ab75ed
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Font, A. S., McCarthy, I. G., Poole-McKenzie, R., Stafford, S. G., Brown, S. T., Schaye, J., Crain, R. A., Theuns, T., & Schaller, M. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa2463 · Cited by 99 · see citing works
What causes the formation of discs and end of bursty star formation?
Hopkins, P. F., Gurvich, A. B., Shen, X., Hafen, Z., Grudić, M. Y., Kurinchi-Vendhan, S., Hayward, C. C., Jiang, F., Orr, M. E., Wetzel, A. R., et al. (2023) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stad1902 · Cited by 99 · see citing works
Revealing the galaxy–halo connection in IllustrisTNG
Bose, S., Eisenstein, D. J., Hernquist, L., Pillepich, A., Nelson, D., Marinacci, F., Springel, V., & Vogelsberger, M. (2019) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stz2546 · Cited by 97 · see citing works
Spectral Templates Optimal for Selecting Galaxies at z > 8 with the JWST
Larson, R. L., Hutchison, T. A., Bagley, M. B., Finkelstein, S. L., Yung, L. Y. A., Somerville, R. S., Hirschmann, M., Brammer, G., Holwerda, B. W., Papovich, C., et al. (2023) · The Astrophysical Journal · doi:10.3847/1538-4357/acfed4 · Cited by 98 · see citing works
Feedback-free starbursts at cosmic dawn
Li, Z., Dekel, A., Sarkar, K. C., Aung, H. H., Giavalisco, M., Mandelker, N., & Tacchella, S. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202348727 · Cited by 98 · see citing works
Spectroscopic Confirmation of a Protocluster at z = 3.37 with a High Fraction of Quiescent Galaxies
McConachie, I., Wilson, G., Forrest, B., Marsan, Z. C., Muzzin, A., Cooper, M. C., Annunziatella, M., Marchesini, D., Chan, J., Gómez, P., et al. (2022) · The Astrophysical Journal · doi:10.3847/1538-4357/ac2b9f · Cited by 96 · see citing works
FLAMINGO: calibrating large cosmological hydrodynamical simulations with machine learning
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Instability of supersonic cold streams feeding galaxies – IV. Survival of radiatively cooling streams
Mandelker, N., Nagai, D., Aung, H., Dekel, A., Birnboim, Y., & van den Bosch, F. C. (2020) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/staa812 · Cited by 95 · see citing works
COSMOS2020: Cosmic evolution of the stellar-to-halo mass relation for central and satellite galaxies up to z ∼ 5
Shuntov, M., McCracken, H. J., Gavazzi, R., Laigle, C., Weaver, J. R., Davidzon, I., Ilbert, O., Kauffmann, O. B., Faisst, A. L., Dubois, Y., et al. (2022) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202243136 · Cited by 94 · see citing works
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Carniani, S., Venturi, G., Parlanti, E., de Graaff, A., Maiolino, R., Arribas, S., Bonaventura, N., Boyett, K., Bunker, A. J., Cameron, A. J., et al. (2024) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202347230 · Cited by 94 · see citing works
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Has JWST Already Falsified Dark-matter-driven Galaxy Formation?
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The GOGREEN Survey: A deep stellar mass function of cluster galaxies at 1.0 < z < 1.4 and the complex nature of satellite quenching
van der Burg, R. F. J., Rudnick, G., Balogh, M. L., Muzzin, A., Lidman, C. E., Old, L. J., Shipley, H., Gilbank, D., McGee, S., Biviano, A., et al. (2020) · Astronomy and Astrophysics · doi:10.1051/0004-6361/202037754 · Cited by 89 · see citing works
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Predicting galaxy star formation rates via the co-evolution of galaxies and haloes
Watson, D. F., Hearin, A. P., Berlind, A. A., Becker, M. R., Behroozi, P., Skibba, R., Reyes, R., Zentner, A. R., & van den Bosch, F. C. (2014) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stu2065 · Cited by 60 · see citing works
Self-citation
Star-forming and quiescent central galaxies cluster similarly: implications for the galaxy–halo connection
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Self-citation
CONSTRAINING THE STAR FORMATION HISTORIES IN DARK MATTER HALOS. I. CENTRAL GALAXIES
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UniverseMachine: Predicting Galaxy Star Formation over Seven Decades of Halo Mass with Zoom-in Simulations
Wang, Y., Nadler, E. O., Mao, Y.-Y., Adhikari, S., Wechsler, R. H., & Behroozi, P. (2021) · The Astrophysical Journal · doi:10.3847/1538-4357/ac024a · Cited by 24 · see citing works
Self-citation
Constraining the galaxy–halo connection over the last 13.3 Gyr: star formation histories, galaxy mergers and structural properties
Rodríguez-Puebla, A., Primack, J., Avila-Reese, V., & Faber, S. M. (2017) · Monthly Notices of the Royal Astronomical Society · doi:10.1093/mnras/stx1172 · Cited by 162 · see citing works

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
ORCID: Behroozi, Peter
Wechsler, Risa H
Hearin, Andrew P
Conroy, Charlie
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
DOI: 10.1093/mnras/stz1182
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 · 2018: 2
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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UniverseMachine: The correlation between galaxy growth and dark matter halo assembly from z = 0−10

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