Table 2.
Relative number of GW-detectable systems with detectable GRB afterglows (radio band), with and without detectable KN, for our fiducial population model, in an O5-type run, and the two jet opening angle hypotheses.
| Fractions of GW triggers with | θj = 3.4° | θj = 15° |
|---|---|---|
| detectable radio afterglow, among which: | O5 | O5 |
| KN detectable | 67% | 74% |
| KN undetectable | 33% | 26% |
| KN undetectable & GRB prompt undetectable | 12% | 15% |
Notes. The threshold for GRB radio afterglow detection considered was 0.01 mJy. KN detection is defined by detection in g (24) or in z (22.5), see text for more details.
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