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Table 7.

Accretion parameters.

Line/continuum log L log r Method MBH Lbol/LEdd Refs.
(1) (2) (3) (4) (5) (6) (7)
L(Hβ)(a) 43.33 17.70 Vir 7.89E+09 0.036 1
L(5100) 45.22 17.60 Vir 6.26E+09 0.045 2
L(5100) 45.22 17.59 Vir 6.08E+09 0.047 3
L(3000) 45.42 17.63 Vir 5.42E+09 0.052 4
L(3000) 45.42 17.72 Vir 6.65E+09 0.043 5
L(3000) 45.42 18.06 Vir 1.46E+10 0.019 2
Average 6.46E+09 0.040
St.dev. 9.14E+08 0.012
L(Hα) 44.12 ... SL 8.04E+09 0.035 6
L(5100) 45.22 ... SL 9.14E+09 0.031 7
L(5100) 45.22 ... SL 7.96E+09 0.036 2
L(Hβ) 43.43 ... SL 5.18E+09 0.055 8
L(3000) 45.42 ... SL 9.33E+09 0.030 4
L(3000) 45.42 ... SL 8.31E+09 0.034 9
L(MgII) 43.69 ... SL 1.23E+10 0.023 7
L(3000)(b) 45.42 ... SL 5.34E+10 0.005 2
Average 8.61E+09 0.035
St.dev. 2.12E+09 0.010

Notes. Column 2 in ergs s−1, Col. 3 in cm, and Col. 5 in M.

(a)

For the same flux, the luminosity was scaled to H0 = 75 km s−1 Mpc−1 as used in the Wu et al. (2004) relation.

(b)

MBH and Lbol/LEdd excluded from average and standard deviation as they are outliers above a 3σ confidence level.

References. (1) Wu et al. 2004; (2) Shen et al. 2023; (3) Bentz et al. 2013; (4) Trakhtenbrot & Netzer 2012; (5) Panda et al. 2019a; (6) Shen et al. 2011; (7) Vestergaard & Peterson 2006; (8) Greene & Ho 2005; and (9) Vestergaard & Osmer 2009.

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