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ZENODO
Dataset . 2026
License: CC BY
Data sources: Datacite
ZENODO
Dataset . 2026
License: CC BY
Data sources: Datacite
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.Ini files for McFACTS v.0.3.0 to reproduce several Figures in the Ford & McKernan CQG review paper

Authors: McKernan, Barry; Ford, K.E.Saavik;

.Ini files for McFACTS v.0.3.0 to reproduce several Figures in the Ford & McKernan CQG review paper

Abstract

Input (.Ini) file for McFACTS v.0.3.0 to reproduce several of the Figures in the Ford & McKernan CQG review paper on the AGN channel for binary black hole mergers.Fig. 2 (CQG) is the equivalent of Fig. 9 in McFACTS1 except for M^-1 not M^-2.Fig. 3 (CQG) is the equivalent of Fig. 6 (LHS) in McFACTS1 except for M^-1 not M^-2.Fig.4 (CQG) is the equivalent of Fig.11 (LHS) in McFACTS1 except for M^-1 not M^-2.Fig. 8 (CQG) is the equivalent of Fig. 8 in McFACTS1 except for M^-1 not M^-2.Fig. 10(CQG) is the equivalent of Fig.10 (RHS) in McFACTS1 except for M^-1 not M^-2.

Keywords

gravitational waves, active galactic nuclei, binary black holes

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Powered by OpenAIRE graph
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average