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Table 4

Median bolometric luminosity, black hole mass, and Eddington ratio.

Sp. type BC only Whole profile


L bol a M BH b M BH b L/LEddc L/LEddc M BH b M BH b L/LEddc L/LEddc
Hβ Mgiiλ2800 Hβ Mgiiλ2800 Hβ Mgiiλ2800 Hβ Mgiiλ2800

Pop. A Full Sample
A1 46.18 8.61 8.62 –0.54 –0.56 8.61 8.71 –0.54 –0.64
A2 46.16 8.52 8.45 –0.47 –0.40 8.52 8.57 –0.47 –0.52
A3 46.15 8.27 8.41 –0.23 –0.37 8.39 8.53 –0.35 –0.49
A4 46.20 8.21 8.56 –0.13 –0.47 8.42 8.66 –0.33 –0.57
Pop. B Full Sample
B1 46.13 9.09 8.98 –1.07 –0.96 9.27 9.08 –1.25 –1.06
B1+ 45.96 9.24 9.06 –1.39 –1.21 9.40 9.18 –1.55 –1.33
B1++ 45.96 9.47 9.14 –1.62 –1.29 9.70 9.35 –1.84 –1.50
B2 46.23 8.93 8.74 –0.81 –0.62 9.12 8.89 –1.00 –0.77

Notes.

(a)

Decimal logarithm of bolometric luminosity in units of erg s-1. A bolometric correction computed following Nemmen & Brotherton (2010) was applied to the 5100 Å specific luminosity.

(b)

Decimal logarithm of black hole mass in solar units. MBH has been estimated from the relation of Shen & Liu (2012) for Mgiiλ2800 and from the relation Assef et al. (2011) for Hβ.

(c)

Decimal logarithm of Eddington ratio.

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