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

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,...

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Bibliographische Detailangaben
Hauptverfasser: Santoliquido, Filippo (VerfasserIn) , Mapelli, Michela (VerfasserIn) , Iorio, Giuliano (VerfasserIn) , Costa, Guglielmo (VerfasserIn) , Glover, Simon (VerfasserIn) , Hartwig, Tilman (VerfasserIn) , Klessen, Ralf S. (VerfasserIn) , Merli, Lorenzo (VerfasserIn)
Dokumenttyp: Article (Journal)
Sprache:Englisch
Veröffentlicht: February 2024
In: Monthly notices of the Royal Astronomical Society
Year: 2024, Jahrgang: 528, Heft: 1, Pages: 954-962
ISSN:1365-2966
DOI:10.1093/mnras/stad3969
Online-Zugang:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stad3969
Volltext
Verfasserangaben:Filippo Santoliquido, Michela Mapelli, Giuliano Iorio, Guglielmo Costa, Simon C.O. Glover, Tilman Hartwig, Ralf S. Klessen and Lorenzo Merli
Beschreibung
Zusammenfassung: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.
Beschreibung:Gesehen am 28.06.2024
Beschreibung:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stad3969

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