Table A.1.
Observational and physical parameters derived from the optical spectra.
| Source | Lbolm | Lbold | L[O III]λ5007 | R5007 | Rsub | Rout | RNLR | MBH* |
|---|---|---|---|---|---|---|---|---|
| (1) | (2) | (3) | (4) | (5) | (6) | (7) | (8) | (9) |
| J1029 | 8.39× 1044 | 3.81× 1044 | 1.23× 1041 | 0.12 | 0.25 | 7.50 | 906.05 | 9.32× 107 |
| J1228 | 1.12× 1045 | 1.35× 1044 | 3.08× 1041 | 0.72 | 0.16 | 4.79 | 1459.28 | 2.23× 107 |
| J1232 | 1.35× 1045 | 5.51× 1044 | 2.34× 1041 | 0.13 | 0.32 | 9.63 | 1263.67 | 5.99× 107 |
| J1509 | 3.40× 1044 | 1.15× 1044 | 4.86× 1040 | 0.19 | 0.13 | 3.74 | 558.36 | 3.97× 107 |
| J1510 | 2.64× 1044 | 5.45× 1043 | 8.61× 1040 | 0.71 | 0.09 | 2.55 | 751.76 | 1.22× 107 |
| J1522 | 1.56× 1044 | 9.08× 1042 | 1.02× 1040 | 0.52 | 0.04 | 1.05 | 248.59 | 6.94× 106 |
| J1641 | 3.81× 1044 | 2.57× 1043 | 7.33× 1040 | 1.12 | 0.06 | 1.89 | 691.75 | 1.80× 107 |
Notes. Columns: (1) Source name; (2) bolometric luminosity calculated using the measured 5100Åcontinuum luminosity [erg s−1] (Eq. 10); (3) bolometric luminosity calculated using the derived 5100Åcontinuum luminosity [erg s−1] (Eq. 10 and Eq. 12); (4) [O III]λ5007 luminosity [erg s−1]; (5) flux ratio between [O III]λ5007 line and Hβ; (6) dust sublimation radius (i.e. boundary between the BLR and the molecular torus) [pc] (Foschini et al. 2019); (7) outer radius of the molecular torus [pc] (Foschini et al. 2019); (8) maximum extension of the NLR [pc] (Foschini et al. 2019); (9) black hole mass [M⊙] calculated using Eq. 2 in Shen et al. (2024).
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