Table 3.
KERRBB results derived from the best-fit peak position.
| a | Rin/Rg |
 |
 |
 |
Ld/LEdd |
|---|---|---|---|---|---|
| SDSS J0100+2802 | |||||
| 0 | 6 | 9.78 | 28.00 | 47.71 | 0.66 |
| 0.998 | 1.24 | 10.24 | 27.48 | 47.94 | 0.39 |
| –0.998 | 9 | 9.62 | 28.16 | 47.69 | 0.90 |
| SDSS J0306+1853 | |||||
| 0 | 6 | 9.64 | 27.92 | 47.63 | 0.75 |
| 0.998 | 1.24 | 10.10 | 27.40 | 47.86 | 0.44 |
| –0.998 | 9 | 9.48 | 28.08 | 47.61 | 1.03 |
| B2 1023+25 | |||||
| 0 | 6 | 9.26 | 27.04 | 46.75 | 0.24 |
| 0.998 | 1.24 | 9.66 | 26.56 | 47.02 | 0.18 |
| –0.998 | 9 | 9.11 | 27.19 | 46.73 | 0.32 |
Notes. The columns are the black hole spin, the inner radius in units of the gravitational radius, the logarithmic values of the black hole mass (per solar mass), the accretion rate (in units of g s−1), the disc luminosity in units of erg s−1, and the Eddington ratio defined in terms of luminosities.
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