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Table 1.

Our estimates for the BH mass M and Eddington ratio λ of J1342, J1120, and J0038 considering spin a = 0 (M0, λ0) and a = 0.9982 (M1, λ1), and different viewing angles (θv = 0 ° −30 ° −45°).

Model Source θv M0 λ0 M1 λ1
KERRBB J1342 8.94 ± 0.10 (9.16) 0.51 ± 0.10 (0.26) 9.34 ± 0.10 0.38 ± 0.10
30° 9.00 ± 0.10 (9.19) 0.49 ± 0.10 (0.28) 9.46 ± 0.10 0.29 ± 0.10
45° 9.07 ± 0.10 (9.23) 0.48 ± 0.10 (0.31) 9.64 ± 0.10 0.19 ± 0.10
J1120 9.13 ± 0.10 (9.35) 0.29 ± 0.10 (0.16) 9.53 ± 0.10 0.22 ± 0.10
30° 9.19 ± 0.10 (9.38) 0.28 ± 0.10 (0.17) 9.65 ± 0.10 0.17 ± 0.10
45° 9.26 ± 0.10 (9.42) 0.27 ± 0.10 (0.19) 9.82 ± 0.10 0.13 ± 0.10
J0038 9.13 ± 0.10 (9.35) 0.45 ± 0.10 (0.23) 9.53 ± 0.10 0.34 ± 0.10
30° 9.19 ± 0.10 (9.38) 0.44 ± 0.10 (0.25) 9.65 ± 0.10 0.26 ± 0.10
45° 9.26 ± 0.10 (9.42) 0.42 ± 0.10 (0.25) 9.84 ± 0.10 0.17 ± 0.10

SLIMBH J1342 8.95 ± 0.10 0.53 ± 0.10 9.41 ± 0.10 0.50 ± 0.10
30° 9.01 ± 0.10 0.51 ± 0.10 9.53 ± 0.10 0.37 ± 0.10
45° 9.08 ± 0.10 0.48 ± 0.10 9.70 ± 0.10 0.23 ± 0.10
J1120 9.14 ± 0.10 0.29 ± 0.10 9.60 ± 0.10 0.28 ± 0.10
30° 9.19 ± 0.10 0.29 ± 0.10 9.72 ± 0.10 0.21 ± 0.10
45° 9.26 ± 0.10 0.28 ± 0.10 9.89 ± 0.10 0.15 ± 0.10
J0038 9.14 ± 0.10 0.47 ± 0.10 9.60 ± 0.10 0.44 ± 0.10
30° 9.20 ± 0.10 0.45 ± 0.10 9.72 ± 0.10 0.33 ± 0.10
45° 9.27 ± 0.10 0.42 ± 0.10 9.89 ± 0.10 0.21 ± 0.10

Notes. The ±0.10 dex error comes from the small uncertainty on the spectrum peak position on which these estimates are based. For a = 0, the two models give almost the same results (i.e. disk thickness and relativistic effects are negligible); for a = 0.9982, the two models give different results by a factor of ∼1.2 − 1.3. For comparison, we show in brackets also the SS results.

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