Table 1.
Parameters and derived quantities for sources with reliable occultations detected.
| Source name | log |
Necl | ΣΔteff | log[RBLR(cm)] | log[ρXobs(cm−3)] | log[r2(cm)] | log |
Refs. for | |
|---|---|---|---|---|---|---|---|---|---|
| Ksec | log |
||||||||
| NGC 4395 | 5.14 ± 0.07 | 3 | 110 | 14.68 ± 0.27 | −39.30 ± 0.17 | 13.04 ± 0.19 | −3.67 ± 0.40 | (1) | |
| NGC 4051 | 6.13 ± 0.14 | 4 | 885 | 15.85 ± 0.13 | −42.15 ± 0.22 | 13.73 ± 0.11 | −0.63 ± 0.20 | (2) | |
| MCG 06-30-015 | 6.20 ± 0.10 | 13 | 1030 | 16.24 ± 0.14 | −42.01 ± 0.16 | 13.13 ± 0.11 | −0.46 ± 0.22 | (3) | |
| NGC 1365 | 6.65 ± 0.09 | 9 | 1388 | 16.20 ± 0.23 | −42.95 ± 0.18 | 13.66 ± 0.17 | −0.005 ± 0.35 | (1) | |
| Mrk 766 | 6.82 ± 0.05 | 6 | 881 | 16.15 ± 0.09 | −43.16 ± 0.09 | 13.76 ± 0.07 | 0.024 ± 0.132 | (2) | |
| NGC 5506 | 6.86 ± 0.09 | 3 | 315 | 16.83 ± 0.22 | −43.41 ± 0.18 | 13.29 ± 0.16 | 0.87 ± 0.34 | (1) | |
| NGC 3227 | 6.77 ± 0.10 | 3 | 245 | 16.00 ± 0.08 | −42.76 ± 0.15 | 13.55 ± 0.08 | −0.52 ± 0.14 | (2) | |
| NGC 4593 | 6.82 ± 0.09 | 1 | 235 | 16.34 ± 0.10 | −43.46 ± 0.15 | 13.86 ± 0.09 | 0.47 ± 0.16 | (2) | |
| IGR J21277+ | 7.18 ± 0.34 | 2 | 286 | 17.00 ± 0.22 | −44.11 ± 0.52 | 13.49 ± 0.23 | 1.43 ± 0.38 | (4) | |
| NGC 3516 | 7.39 ± 0.05 | 4 | 830 | 16.26 ± 0.12 | −44.22 ± 0.09 | 14.13 ± 0.09 | 0.59 ± 0.18 | (2) | |
| NGC 3783 | 7.37 ± 0.08 | 8 | 785 | 16.17 ± 0.11 | −43.81 ± 0.13 | 13.84 ± 0.09 | 0.11 ± 0.17 | (2) | |
| NGC 4151 | 7.55 ± 0.05 | 4 | 335 | 15.92 ± 0.13 | −43.90 ± 0.10 | 13.99 ± 0.10 | −0.24 ± 0.20 | (2) | |
| Mrk 79 | 7.61 ± 0.12 | 1 | 225 | 16.73 ± 0.04 | −44.82 ± 0.18 | 14.05 ± 0.07 | 1.43 ± 0.08 | (2) | |
| PG 1501+106 | 8.05 ± 0.02 | 2 | 859 | 16.68 ± 0.02 | −45.73 ± 0.03 | 14.569 ± 0.017 | 1.86 ± 0.03 | (5) |
Notes. For each source showing reliable occultations the following quantities are reported: the logarithm of mass of the central black hole MBH in solar mass units; the total number of eclipses detected in Paper I, Necl; the cumulative observational time ΣΔteff; the value of log(RBLR); the logarithm of the occulting cloud number density as derived from Eq. (5) for the case gex = 3.0, gin = 0.1; the logarithm of the radius of the largest cloud in the source, r2 (defined in Sect. 5.1); and the logarithm of the mass of the ensemble of clouds in the BLR, measured in units of the solar mass, 
(defined in Sect. 8). The last two quantities refer to the case w = 2 (see Sect. 4) and the same choice of of {gex, gin} parameters quoted above (see Sects. 5 and 7 for details). References for log
values are reported in the last column: (1) Ricci et al. (2017), (2) Bentz & Katz (2015), (3) Bentz et al. (2016), (4) Malizia et al. (2008), (5) Winter et al. (2010).
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