Table 4
Summary table of the significant quantitative findings.
| Galactic DWD (spiraling) | Extragalactic DWD (merging) | ||||
|---|---|---|---|---|---|
| Quantity | Value | Ref. in text | Value | Ref. in text | |
| Detectable (S/N > 8) | 30 ± 5(stat) ± 6(sys) | Sect. 5.1 | 10 ± 3(stat) ± 2(sys) | Sect. 5.3 | |
| Total abundance | (5.5 ± 0.007(stat) ± 1(sys)) · 105 | ||||
| Super-Ch. abundance | (2 ± 0.01 (stat) ± 0.4(sys)) · 104 | Sect. 3.1 | 50 ± 7(stat) ± 9(sys) | ||
| 90% sky area [deg2] | Median | 8.6 · 10−3 | |||
| 95% interval | [3.6 · 10−4,1.5 · 10−1] | Sect. 5.3, Fig. 6 | |||
| dL relative error | Median | 4.9 · 10−1 | |||
| 95% interval | [6.3 · 10−2,1.5 · 101] | ||||
| Fiducial volume [Mpc3] | Median | 1.5 · 10−3 | |||
| 95% interval | [2.9 · 10−7,2.6 · 10−1] | ||||
Notes. The merging case refers to the contact scenario, as in the (very conservative) Roche scenario the extragalactic detection rate is negligible. The total and super-Chandrasekhar abundances refer to the systems with f > 1 mHz and dL < 30 Mpc. The observation time is 10 years in both cases.
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