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Table 4.

Physical quantities of PJ308-21 derived from line fitting.

PJ308-21
Lλ(5100 Å) ( 4 . 9 0.2 + 0.4 ) × 10 42 erg s 1 Å 1 $ (4.9^{+0.4}_{-0.2}) \times 10^{42}\,\mathrm{erg\,s}^{-1}\,\AA^{-1} $
L(Hα) (1.84 ± 0.01)×1045 erg s−1
FWHM(Hβ) 4616 61 + 63 km s 1 $ 4616^{+63}_{-61}\,\mathrm{km\,s}^{-1} $
FWHM(Hα) 3739 ± 26 km s−1
FWHM([O III]) 2776 74 + 75 $ 2776^{+75}_{-74} $ km s−1
ΔvHβ 87 ± 15 km s−1
ΔvHα −149 ± 7 km s−1
Δv[O III] −1922 ± 39 km s−1
MBH, Hβ (2.7 ± 0.2)×109M
MBH, Hα (1.93 ± 0.03)×109M
Lbol ( 2 . 3 0.1 + 0.2 ) × 10 47 erg s 1 $ (2.3^{+0.2}_{-0.1}) \times 10^{47}\,\mathrm{erg\,s}^{-1} $
λEdd, Hβ 0 . 67 0.05 + 0.12 $ 0.67^{+0.12}_{-0.05} $
λEdd, Hα 0 . 96 0.06 + 0.10 $ 0.96^{+0.10}_{-0.06} $
EW[O III] 19 ± 2 Å
EWHβ 118 11 + 8 Å $ 118^{+8}_{-11}\,\AA $
EWFe II 43 3 + 2 Å $ 43^{+2}_{-3}\,\AA $
RFe II 0 . 36 0.06 + 0.04 $ 0.36^{+0.04}_{-0.06} $

Notes. We report the random errors from the MCMC fit. The statistical uncertainty, due to object-to-object differences, on the black hole mass estimates is ∼0.5 dex (Vestergaard & Peterson 2006) and affects also the Eddington ratios.

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