Dark-ages Reionization and Galaxy Formation Simulation - X. The small contribution of quasars to reionization

Autor: Chuanwu Liu, Alan R. Duffy, Paul W. Angel, Andrei Mesinger, Paul M. Geil, J. Stuart B. Wyithe, Gregory B. Poole, Yuxiang Qin, Simon J. Mutch
Přispěvatelé: Qin, Yuxiang, Mutch, Simon J., Poole, Gregory B., Liu, Chuanwu, Angel, Paul W., Duffy, Alan R., Geil, Paul M., Mesinger, Andrei, Wyithe, J. Stuart B.
Jazyk: angličtina
Rok vydání: 2017
Předmět:
Cosmology and Nongalactic Astrophysics (astro-ph.CO)
Active galactic nucleus
Stellar mass
Astrophysics::High Energy Astrophysical Phenomena
FOS: Physical sciences
Astrophysics
Astrophysics::Cosmology and Extragalactic Astrophysics
01 natural sciences
high-redshift [Galaxies]
0103 physical sciences
supermassive black hole [Quasars]
010303 astronomy & astrophysics
Reionization
Astrophysics::Galaxy Astrophysics
Luminosity function (astronomy)
Physics
Supermassive black hole
numerical [Methods]
010308 nuclear & particles physics
Astronomy
Astronomy and Astrophysics
Quasar
Astronomy and Astrophysic
formation [Galaxies]
Astrophysics - Astrophysics of Galaxies
Redshift
Galaxy
13. Climate action
Space and Planetary Science
Astrophysics of Galaxies (astro-ph.GA)
Astrophysics - Cosmology and Nongalactic Astrophysics
Zdroj: Monthly Notices of the Royal Astronomical Society
Popis: Motivated by recent measurements of the number density of faint AGN at high redshift, we investigate the contribution of quasars to reionization by tracking the growth of central supermassive black holes in an update of the Meraxes semi-analytic model. The model is calibrated against the observed stellar mass function at $z\sim0.6-7$, the black hole mass function at $z\lesssim0.5$, the global ionizing emissivity at $z\sim2-5$ and the Thomson scattering optical depth. The model reproduces a Magorrian relation in agreement with observations at $z
21 pages, 12 figures; Updated to match the published version. All results and conclusions remain unchanged
Databáze: OpenAIRE