Table 2.
Detection limits and predicted detection rates for NSNS and BHNS assuming different detector network configurations.
| GW ET | KN+GW | GRB afterglow+GW | GRB prompt+GW | ||||||
|---|---|---|---|---|---|---|---|---|---|
| J | z | g | Radio | Optical | X-rays | VHE | Fermi | ||
| NSNS | |||||||||
| Limit | 12 | 21 | 24.4 | 26 | 0.01 | 26 | 10−13 | CTA | 3.09 × 10−7 |
| ETΔ | |||||||||
| Rate | ![]() |
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| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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| ET2L | |||||||||
| Rate | ![]() |
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| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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| ETΔ+2CE | |||||||||
| Rate | ![]() |
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| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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| ET2L+2CE | |||||||||
| Rate | ![]() |
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| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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| BHNS | |||||||||
| Limit | 12 | 21 | 24.4 | 26 | 0.01 | 26 | 10−13 | CTA | 3.09 × 10−7 |
| ETΔ | |||||||||
| Rate | ![]() |
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| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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| ET2L | |||||||||
| Rate | ![]() |
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| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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| ETΔ+2CE | |||||||||
| Rate | ![]() |
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| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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| ET2L+2CE | |||||||||
| Rate | ![]() |
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< 10−3 | ![]() |
| (ΔΩ90% < 100 deg2) | ( ) |
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| (ΔΩ90% < 10 deg2) | ( ) |
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Notes. We report in parenthesis the detection rates assuming ΔΩ90% < 100 deg2 and ΔΩ90% < 10 deg2. The GW detection limits refer to the S/Nnet threshold. Near infrared and optical limiting magnitudes are in the AB system; radio limiting flux densities are in mJy @ 1.4 GHz; X-ray limiting flux densities are in erg cm−2 s−1 keV−1 @ 1 keV; gamma-ray limiting fluence is in erg cm−2 (Fermi/GBM). Detection rates are in yr−1. The reported errors, given at the 90% credible level, stem from the uncertainty on the overall merger rate, while systematic errors are not included.
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