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Table 2.
FWHM, luminosities, and MBH.
| Image | Line | FWHM [km s−1] | log10(Lref)[L⊙] (a) | log10(MBH) [M⊙] | log10 ( rs) [cm] (b) | S/N line (c) | S/N continuum |
|---|---|---|---|---|---|---|---|
| Mg II | 3914.52 ± 500.09 | 44.23 ± 0.19 | 8.25 ± 0.59 | 14.92 ± 0.31 | 30 | 5 | |
| A | Hβ | 4689.32 ± 42.96 | 44.29 ± 0.17 | 8.27 ± 0.24 | 15.26 ± 0.79 | 16 | 6 |
| Hα | 5595.68 ± 125.92 | 44.36 ± 0.23 | 8.57 ± 0.22 | 15.63 ± 0.83 | 73 | 11 | |
| Mg II | 4118.73 ± 921.90 | 44.23 ± 0.19 | 8.29 ± 0.88 | 14.95 ± 0.23 | 35 | 6 | |
| B | Hβ | 4817.63 ± 48.15 | 44.21 ± 0.16 | 8.24 ± 0.21 | 15.23 ± 0.85 | 19 | 6 |
| Hα | 6150.98 ± 133.39 | 44.29 ± 0.23 | 8.61 ± 0.27 | 15.66 ± 0.74 | 85 | 12 | |
Notes.
(a)
Lref = Luminosity ( L3000, L5100, L5100) for Mg II, Hα and Hβ respectively. The luminosity for Hα and Hβ is from the spectra and for Mg II is obtained from the SED.
(b)
rs is the accretion disk size obtained from Eq. (5) at the λrest of the emission line used for the MBH measurement.
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