Table 1
Summary of the results of GW detections relevant for the present work at the various considered detector networks.
Number of GW detections | |||||||
---|---|---|---|---|---|---|---|
Network | Θ ≤ 20° | Θ ≤ 33° | ∆ψ ≤ 30° | ∆ι ≤ 30° | Θ ≤ 20° & ∆ψ ≤ 30° | Θ ≤ 33° & ∆ψ ≤ 30° | Θ ≤ 33° & ∆ι ≤ 30° |
LVKIO5 | 2 | 7 | 3 | 5 | 0 | 0 | 0 |
LVKI Voyager | 74 | 148 | 100 | 78 | 8 | 26 | 1 |
ET | 1573 | 3774 | 1561 | 4007 | 26 | 63 | 54 |
ET+2CE | 4680 | 12 035 | 16 973 | 21 423 | 59 | 172 | 144 |
Notes. For each configuration, in the second and third column we report the number of detections of events with Θ ≤ 20° and Θ ≤ 33°, respectively. We use for convenience of notation the definition Θ = min(ι, 180° − ι}, thus, for example, Θ ≤ 20° is equivalent to ι ≤ 20° or ι ≥ 160°. The value Θ = 33° matches the one reconstructed for GW170817, which we take as a representative limit. In the fourth and fifth column we report the number of detected events with 1σ errors smaller than 30° on ψ and ι, respectively. In the sixth and seventh column we report the number of events matching both the criteria ∆ψ ≤ 30° and Θ ≤ 20° and Θ ≤ 33°, respectively, while in the last column the events having both Θ ≤ 33° and ∆ι ≤ 30° (no event is found with Θ ≤ 20° and ∆ι ≤ 30°, as can be seen from Fig. 10).
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