Table 1
Simulated values of the rate R for the old LISA configuration.
j | eLSO | t0 | Tmission | p/10-2 | R [yr-1] |
|
|||||
0.1 | 0.1 | 5 yr | 5 yr | 1.06 | 400 (4700) |
0.1 | 0.3 | 5 yr | 5 yr | 1.06 | 300 (4500) |
0.1 | 0.5 | 5 yr | 5 yr | 1.06 | 200 (3100) |
0.1 | 0.7 | 5 yr | 5 yr | 1.06 | 80 (1200) |
0.5 | 0.1 | 5 yr | 5 yr | 1.06 | 500 (4700) |
0.5 | 0.3 | 5 yr | 5 yr | 1.06 | 300 (4700) |
0.5 | 0.5 | 5 yr | 5 yr | 1.06 | 200 (3600) |
0.5 | 0.7 | 5 yr | 5 yr | 1.06 | 100 (1500) |
1 | 0.1 | 5 yr | 5 yr | 1.06 | 500 (4900) |
1 | 0.1 | 5 yr | 5 yr | 5.04 | 2200 (19900) |
1 | 0.1 | 5 yr | 5 yr | 0.281 | 100 (1400) |
1 | 0.3 | 5 yr | 5 yr | 1.06 | 400 (5300) |
1 | 0.5 | 5 yr | 5 yr | 1.06 | 300 (4300) |
1 | 0.7 | 5 yr | 5 yr | 1.06 | 100 (1900) |
1 | 0.5 | 6 yr | 5 yr | 1.06 | 100 (1700) |
1 | 0.5 | 10 yr | 5 yr | 1.06 | 20 (300) |
1 | 0.5 | 15 yr | 5 yr | 1.06 | 8 (100) |
1 | 0.5 | 5 yr | 2 yr | 1.06 | 20 (300) |
1 | 0.5 | 6 yr | 2 yr | 1.06 | 10 (200) |
Notes. The tabulated values of R depend on the spin parameter (j), on the eccentricity at the last stable orbit (eLSO), on the initial time of observations, defined as time before the plunge-in (t0), on the expected duration of the mission (Tmission), on p ≡ msph/mh (see Sect. 2.1 and Appendix B), and on fBH (i.e. the adopted mSMBH − msph relation). The value of R out of (inside) parentheses refers to fBH from G12a (MH03). Tabulated rates are for and tloss = 107 yr.
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