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  • 1806.08370v2

    Rights statement: This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version Andrew J Griffin, Cedric G Lacey, Violeta Gonzalez-Perez, Claudia del P Lagos, Carlton M Baugh, Nikos Fanidakis, The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation, Monthly Notices of the Royal Astronomical Society, Volume 487, Issue 1, July 2019, Pages 198–227, https://doi.org/10.1093/mnras/stz1216 is available online at: https://academic.oup.com/mnras/article/487/1/198/5485649

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The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation

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The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation. / Griffin, Andrew J.; Lacey, Cedric G.; Gonzalez-Perez, Violeta et al.
In: Monthly Notices of the Royal Astronomical Society, Vol. 487, No. 1, 01.07.2019, p. 198-227.

Research output: Contribution to Journal/MagazineJournal articlepeer-review

Harvard

Griffin, AJ, Lacey, CG, Gonzalez-Perez, V, Lagos, CDP, Baugh, CM & Fanidakis, N 2019, 'The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation', Monthly Notices of the Royal Astronomical Society, vol. 487, no. 1, pp. 198-227. https://doi.org/10.1093/mnras/stz1216

APA

Griffin, A. J., Lacey, C. G., Gonzalez-Perez, V., Lagos, C. D. P., Baugh, C. M., & Fanidakis, N. (2019). The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation. Monthly Notices of the Royal Astronomical Society, 487(1), 198-227. https://doi.org/10.1093/mnras/stz1216

Vancouver

Griffin AJ, Lacey CG, Gonzalez-Perez V, Lagos CDP, Baugh CM, Fanidakis N. The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation. Monthly Notices of the Royal Astronomical Society. 2019 Jul 1;487(1):198-227. Epub 2019 May 4. doi: 10.1093/mnras/stz1216

Author

Griffin, Andrew J. ; Lacey, Cedric G. ; Gonzalez-Perez, Violeta et al. / The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation. In: Monthly Notices of the Royal Astronomical Society. 2019 ; Vol. 487, No. 1. pp. 198-227.

Bibtex

@article{329a77cf1d774e79baceb3726e815041,
title = "The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation",
abstract = " Understanding how Active Galactic Nuclei (AGN) evolve through cosmic time allows us to probe the physical processes that control their evolution. We use an updated model for the evolution of masses and spins of supermassive black holes (SMBHs), coupled to the latest version of the semi-analytical model of galaxy formation GALFORM using the Planck cosmology and a high resolution Millennium style dark matter simulation to make predictions for AGN and SMBH properties for $0 <z <6$. We compare the model to the observed black hole mass function and the SMBH versus galaxy bulge mass relation at $z=0$, and compare the predicted bolometric, hard X-ray, soft X-ray and optical AGN luminosity functions to observations at $z <6$, and find that the model is in good agreement with the observations. The model predicts that at $z",
keywords = "galaxies: active, galaxies: high-redshift, quasars: general",
author = "Griffin, {Andrew J.} and Lacey, {Cedric G.} and Violeta Gonzalez-Perez and Lagos, {Claudia del P.} and Baugh, {Carlton M.} and Nikos Fanidakis",
note = "This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version Andrew J Griffin, Cedric G Lacey, Violeta Gonzalez-Perez, Claudia del P Lagos, Carlton M Baugh, Nikos Fanidakis, The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation, Monthly Notices of the Royal Astronomical Society, Volume 487, Issue 1, July 2019, Pages 198–227, https://doi.org/10.1093/mnras/stz1216 is available online at: https://academic.oup.com/mnras/article/487/1/198/5485649",
year = "2019",
month = jul,
day = "1",
doi = "10.1093/mnras/stz1216",
language = "English",
volume = "487",
pages = "198--227",
journal = "Monthly Notices of the Royal Astronomical Society",
issn = "0035-8711",
publisher = "OXFORD UNIV PRESS",
number = "1",

}

RIS

TY - JOUR

T1 - The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation

AU - Griffin, Andrew J.

AU - Lacey, Cedric G.

AU - Gonzalez-Perez, Violeta

AU - Lagos, Claudia del P.

AU - Baugh, Carlton M.

AU - Fanidakis, Nikos

N1 - This is a pre-copy-editing, author-produced PDF of an article accepted for publication in Monthly Notices of the Royal Astronomical Society following peer review. The definitive publisher-authenticated version Andrew J Griffin, Cedric G Lacey, Violeta Gonzalez-Perez, Claudia del P Lagos, Carlton M Baugh, Nikos Fanidakis, The evolution of SMBH spin and AGN luminosities for z < 6 within a semi-analytic model of galaxy formation, Monthly Notices of the Royal Astronomical Society, Volume 487, Issue 1, July 2019, Pages 198–227, https://doi.org/10.1093/mnras/stz1216 is available online at: https://academic.oup.com/mnras/article/487/1/198/5485649

PY - 2019/7/1

Y1 - 2019/7/1

N2 - Understanding how Active Galactic Nuclei (AGN) evolve through cosmic time allows us to probe the physical processes that control their evolution. We use an updated model for the evolution of masses and spins of supermassive black holes (SMBHs), coupled to the latest version of the semi-analytical model of galaxy formation GALFORM using the Planck cosmology and a high resolution Millennium style dark matter simulation to make predictions for AGN and SMBH properties for $0 <z <6$. We compare the model to the observed black hole mass function and the SMBH versus galaxy bulge mass relation at $z=0$, and compare the predicted bolometric, hard X-ray, soft X-ray and optical AGN luminosity functions to observations at $z <6$, and find that the model is in good agreement with the observations. The model predicts that at $z

AB - Understanding how Active Galactic Nuclei (AGN) evolve through cosmic time allows us to probe the physical processes that control their evolution. We use an updated model for the evolution of masses and spins of supermassive black holes (SMBHs), coupled to the latest version of the semi-analytical model of galaxy formation GALFORM using the Planck cosmology and a high resolution Millennium style dark matter simulation to make predictions for AGN and SMBH properties for $0 <z <6$. We compare the model to the observed black hole mass function and the SMBH versus galaxy bulge mass relation at $z=0$, and compare the predicted bolometric, hard X-ray, soft X-ray and optical AGN luminosity functions to observations at $z <6$, and find that the model is in good agreement with the observations. The model predicts that at $z

KW - galaxies: active

KW - galaxies: high-redshift

KW - quasars: general

U2 - 10.1093/mnras/stz1216

DO - 10.1093/mnras/stz1216

M3 - Journal article

VL - 487

SP - 198

EP - 227

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

SN - 0035-8711

IS - 1

ER -