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Table 3

Emission-line black hole mass.

Name zSDSS Line ID Lλ erg s−1 FWHM km s−1 Flux 10−17 erg s−1 cm−2 logLline erg s−1 log(MBH / Mθ) logLBLR erg s−1 logLγ erg s−1 δ
(1) (2) (3) (4) (5) (6) (7) (8) (9) (10) (11)
J0014.3-0500 0.7908 Mg II 45.18 ± 0.01 3008.97 ± 270.55 222.41 ± 13.61 42.81 ± 0.03 8.19 ± 0.08 44.03 ± 0.03 46.27 ± 0.05 15.97
J0024.5-0810 2.0709 C IV 45.63 ± 0.01 4471.36 ± 540.12 489.93 ± 74.55 44.19 ± 0.07 8.97 ±0.1 45.14 ± 0.07 46.91 ± 0.14 7.41
J0036.9+1832 1.5949 C IV 2882.85 ± 32.66 469.95 ± 23.08 43.89 ± 0.02 44.69 ± 0.04 46.94 ± 0.06 14.11
Mg II 45.47 ± 0.03 1573.64 ± 513.7 124.51 ± 20.19 43.31 ± 0.07 7.81 ± 0.28
J0040.9+3203 0.6319 Mg II 44.31 ± 0.01 3635.99 ± 2462.07 57.8 ± 14.17 41.99 ± 0.11 7.82 ± 0.59 43.2 ± 0.11 45.5 ±0.1 20.29

Notes. Column 1: 4FGL name. Column 2: redshift in SDSS. Column 3: emission line used for black hole mass estimation. Column 4: Lλ represents the continuum luminosity in erg s−1 associated with Col. 3. The typical continuum wavelengths are 5100 Å for Hβ, 3000 Å for Mg II, and 1350 Å for C IV. Column 5: full width at half maximum (FWHM) of the emission line in km s−1. Column 6: line flux in units of 10−17 erg s−1 cm−2. Column 7: logarithmic line luminosity in erg s−1. Column 8: logarithmic black hole mass in M derived from the line in Col. 3. Column 9: logarithmic γ-ray luminosity, logLγ(0.1∼100,GeV) (erg s−1). Column 10: Logarithmic broad-line region luminosity, log LBLR (erg s−1). Column 11: Doppler factor estimated in this work, δ. Full table available at the CDS.

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