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Table 3.
Main properties of our models.
Instrument | MSBH | zmax | MIMBH, max | Γ1 | Γ2 | Γ3 | ΔΓ1 | ΔΓ2 | ΔΓ3 |
---|---|---|---|---|---|---|---|---|---|
( M⊙) | ( M⊙) | (yr−1) | (yr−1) | (yr−1) | (yr−1) | (yr−1) | (yr−1) | ||
LIGO | 10 | 0.38 | 200 | 0.04 | 0.04 | 0.04 | 0.003 − 0.54 | 0.003 − 0.59 | 0.003 − 0.54 |
LIGO | 30 | 0.57 | 200 | 0.09 | 0.11 | 0.11 | 0.006 − 1.3 | 0.008 − 1.6 | 0.008 − 1.6 |
LISA | 10 | 0.70 | 46240 | 0.35 | 0.45 | 0.45 | 0.024 − 5.1 | 0.031 − 6.5 | 0.031 − 6.5 |
LISA | 30 | 1.78 | 46240 | 3.9 | 3.5 | 4.1 | 0.27 − 56.2 | 0.24 − 50.0 | 0.28 − 59.3 |
ET | 10 | 6.00 | 2000 | 27.7 | 10.9 | 13.5 | 1.9 − 399.7 | 0.75 − 157.2 | 0.94 − 195.5 |
ET | 30 | 6.00 | 2000 | 41.3 | 15.5 | 19.2 | 2.8 − 596.5 | 1.1 − 224.0 | 1.3 − 278.1 |
DECIGO | 10 | 6.00 | 46240 | 217.2 | 85.5 | 103.2 | 15.0 − 3139 | 5.9 − 1235 | 7.1 − 1492 |
DECIGO | 30 | 6.00 | 46240 | 217.2 | 85.5 | 103.2 | 15.0 − 3139 | 5.9 − 1235 | 7.1 − 1492 |
Notes. Column 1: Instrument name. Column 2: Mass of the IMRI secondary. Column 3: Horizon redshift. Column 4: Maximum IMBH mass visible. Columns 5–7: Average merger rate obtained with models GAL, CFR, CSFE. Columns 8 and 9: Boundaries of the inferred merger rate for models GAL, CFR, CSFE.
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