Table 3: Black hole mass ( $M_{\rm BH}$), monochromatic luminosity $\nu $$L_{\nu }$(5100 Å), bolometric luminosity ( $L_{\rm bol}$), and accretion rate with respect to Eddington. (*) $L_{\rm bol}\simeq 9 \times \nu L_{\nu }$(5100 Å). (**) using the relation (3) given by Woo & Urry et al. (2002) between $M_{\rm BH}$ and $\nu L_{\nu }$(5100 Å). (a) Kaspi et al. (2000), (b) Vestergaard (2002), and (c) Shields et al. (2003), (d) Grupe et al. (2004), and (e) Woo & Urry (2002).

Source		 log  $M_{\rm BH}$ log $\nu $$L_{\nu }$ (5100Å) log  $L_{\rm bol}$ ${\dot{m}}$
  ($M_{\odot}$) (erg s-1) (erg s-1)  

I Zw1		 $7.26\pm0.11$(b) 44.52 $\pm$ 0.12(b) 45.47 $\pm$ 0.12(*) 1.30
PG 0804+761 8.31 $\pm$ 0.04(a) 44.82+0.07-0.09(a) 45.93(e) 0.33
PG 0947+396 8.54(c) 44.94(c) 45.89(*) 0.18
PG 0953+414 $\rm 8.27^{+0.06}_{-0.09}$(a) $\rm 45.08^{+0.05}_{-0.07}$(a) 46.16(e) 0.62
PG 1048+342 8.25(c) 44.86(c) 45.81(*) 0.29
PG 1114+445 8.41 $\pm$ 0.09(b) 44.59 $\pm$ 0.07(b) 45.54(*) 0.11
PG 1115+407 7.66(**) 44.51(d) 45.83(d) 0.51
PG 1116+215 8.50 $\pm$ 0.10(b) 45.27 $\pm$ 0.07(b) 46.02(e) 0.26
PG 1202+281 8.12 $\pm$ 0.09(b) 44.42 $\pm$ 0.07 (b) 45.26(d) 0.14
PG 1244+026 6.29 $\pm$ 0.10(b) 43.67 $\pm$ 0.08(b) 44.75(d) 1.71
PG 1307+085 8.73 $\pm$ 0.10(b) 44.86 $\pm$ 0.07(b) 45.83(e) 0.10
PG 1309+355 8.21 $\pm$ 0.13(b) 44.84 $\pm$ 0.07(b) 45.82 $\pm$ 0.07(*) 0.31
PG 1322+659 8.09(c) 44.98(c) 45.93(*) 0.55
PG 1352+183 8.30(c) 44.97(c) 45.92(*) 0.33
PG 1402+261 7.29(e)   45.13(e) 0.55
Mrk 1383 $\rm 8.67^{+0.13}_{-0.24}$(a) $\rm 44.61^{+0.06}_{-0.07}$(a) 45.19(e) 0.03
PG 1427+480 7.99(c) 44.95(c) 45.90(*) 0.65
Mrk 478 7.30 $\pm$ 0.10(b) 44.42 $\pm$ 0.07(b) 45.88(d) 0.94
PG 1512+370 8.95 $\pm$ 0.10(b) 45.41 $\pm$ 0.06(b) 46.36 $\pm$ 0.06(*) 0.21
Mrk 876 $\rm 8.38^{+0.18}_{-0.20}$(a) 44.84 $\pm$ 0.06(a) 45.66(e) 0.15
PG 1626+554 8.37(c) 44.72(c) 45.67(d) 0.16


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