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Table 1.
Horizon distances assumed for the various GW observing runs, as used in the detection criterion in Eq. (1), and parameters for the kilonova peak absolute AB magnitude dependence on the viewing angle, as given in Eq. (4).
Run | DH [Mpc] | Band | Mλ, 0 | ΔMλ |
---|---|---|---|---|
O3 | 157 | g | −16.3 | 7 |
O4 | 229 | r | −16.3 | 4 |
O5 | 472 | i | −16.4 | 3.5 |
O3@GW190425 | 181 | z | −16.5 | 2.5 |
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