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Table 9.

Fraction of BH-NS mergers with detectable kilonova among LIGO/Virgo detectable (S/R > 8) events for assumed exposure times.

Model Subaru CFHT ATLAS
M230 0.004 0.002 < 10−5
M233 0.067 0.032 < 10−4
M280 0.004 0.002 < 10−5
M283 0.021 0.010 < 10−4
M383 0.064 0.038 < 10−4
M483 0.018 0.009 < 10−4

Notes. Kilonova detectability is assessed for three different instruments: Subaru, the Canada-France-Hawaii Telescope (CFHT) and ATLAS. The same results expressed in terms of merger rates can be found in the appendix; see Table A.3. See Eq. (16).

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