Correction to: Binary black hole mergers from population III stars: uncertainties from star formation and binary star properties

• Verfasst von: Santoliquido, Filippo [VerfasserIn]
• Verfasst von: Mapelli, Michela [VerfasserIn]
• Verfasst von: Iorio, Giuliano [VerfasserIn]
• Verfasst von: Costa, Guglielmo [VerfasserIn]
• Verfasst von: Glover, Simon [VerfasserIn]
• Verfasst von: Hartwig, Tilman [VerfasserIn]
• Verfasst von: Klessen, Ralf S. [VerfasserIn]
• Verfasst von: Merli, Lorenzo [VerfasserIn]
• Titel: Correction to: Binary black hole mergers from population III stars: uncertainties from star formation and binary star properties
• Verf.angabe: Filippo Santoliquido, Michela Mapelli, Giuliano Iorio, Guglielmo Costa, Simon C.O. Glover, Tilman Hartwig, Ralf S. Klessen and Lorenzo Merli
• E-Jahr: 2024
• Jahr: February 2024
• Umfang: 9 S.
• Illustrationen: Illustrationen
• Fussnoten: Gesehen am 28.06.2024
• Titel Quelle: Enthalten in: Royal Astronomical SocietyMonthly notices of the Royal Astronomical Society
• Ort Quelle: Oxford : Oxford Univ. Press, 1827
• Jahr Quelle: 2024
• Band/Heft Quelle: 528(2024), 1 vom: Feb., Seite 954-962
• ISSN Quelle: 1365-2966
• DOI: doi:10.1093/mnras/stad3969
• Datenträger: Online-Ressource
• Sprache: eng
• Bibliogr. Hinweis: Errata zu: Santoliquido, Filippo: Binary black hole mergers from population III stars
• K10plus-PPN: 189240477X

Abstract

Our paper ‘Binary black hole mergers from population III stars: uncertainties from star formation and binary star properties’ was published in MNRAS, 524, p. 307-324 (2023).After publication, we found a minor bug in cosmo$\mathcal {R}$ate, the code we used to produce the results shown in Figs 2, 3, 4, 5, 6, 7, 8, 9, 10, 12, 13, 14, 15, 17, 18, B1, and B2.In the following, we list the changes with respect to the published version of the paper. All of them are minor changes: the results and conclusions presented in the published article are not significantly affected by the bug.