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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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Main Authors: Santoliquido, Filippo (Author) , Mapelli, Michela (Author) , Iorio, Giuliano (Author) , Costa, Guglielmo (Author) , Glover, Simon (Author) , Hartwig, Tilman (Author) , Klessen, Ralf S. (Author) , Merli, Lorenzo (Author)
Format: Article (Journal)
Language:English
Published: February 2024
In: Monthly notices of the Royal Astronomical Society
Year: 2024, Volume: 528, Issue: 1, Pages: 954-962
ISSN:1365-2966
DOI:10.1093/mnras/stad3969
Online Access:Verlag, lizenzpflichtig, Volltext: https://doi.org/10.1093/mnras/stad3969
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Author Notes:Filippo Santoliquido, Michela Mapelli, Giuliano Iorio, Guglielmo Costa, Simon C.O. Glover, Tilman Hartwig, Ralf S. Klessen and Lorenzo Merli
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Summary: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.
Item Description:Gesehen am 28.06.2024
Physical Description:Online Resource
ISSN:1365-2966
DOI:10.1093/mnras/stad3969

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