Table 2
Mass and accretion luminosity estimated from optical data.
| Source | σline | FWHM | LHβ | M | Ldisk | Ldisk/LEdd | Method |
|
|
|||||||
| J0100 − 0200 | 982 | 920 | − | 4.0 | 25.2 | 0.49 | M |
| J0134 − 4258 | 1632 | 1241 | 2.77 | 7.1 | 8.61 | 0.09 | L (Grupe et al. 2000) |
| J0324 + 3410 | 1791 | 1868 | 0.53 | 3.6 | 1.50 | 0.03 | A |
| J0706 + 3901 | 1839 | 1402 | 0.16 | 2.0 | 0.43 | 0.02 | N |
| J0713 + 3820 | 2041 | 1901 | 9.28 | 21.2 | 31.0 | 0.11 | N |
| J0744 + 5149 | 2122 | 1989 | − | 26.5 | 49.2 | 0.14 | M |
| J0804 + 3853 | 1588 | 1523 | 2.74 | 6.7 | 8.51 | 0.10 | S |
| J0814 + 5609 | 2759 | 2777 | 6.10 | 31.0 | 19.9 | 0.05 | S |
| J0849 + 5108 | 1330 | 2490 | 1.32 | 3.2 | 3.94 | 0.09 | S |
| J0902 + 0443 | 1491 | 1781 | 2.02 | 5.0 | 6.17 | 0.09 | S |
| J0937 + 3615 | 1343 | 2192 | 0.59 | 2.1 | 1.68 | 0.06 | S |
| J0945 + 1915 | 1730 | 2818 | 2.52 | 7.6 | 7.80 | 0.08 | A |
| J0948 + 0022 | 1548 | 1639 | 3.73 | 7.5 | 11.8 | 0.12 | S |
| J0953 + 2836 | 2407 | 2749 | 3.14 | 16.6 | 9.84 | 0.05 | S |
| J1031 + 4234 | 3153 | 1822 | 2.08 | 22.9 | 6.37 | 0.02 | S |
| J1037 + 0036 | 985 | 1776 | 1.75 | 2.0 | 5.31 | 0.20 | S |
| J1038 + 4227 | 1615 | 1917 | 2.62 | 6.8 | 8.12 | 0.09 | S |
| J1047 + 4725 | 1474 | 2237 | 5.80 | 8.6 | 18.9 | 0.17 | S |
| J1048 + 2222 | 1742 | 718 | 1.39 | 5.7 | 4.16 | 0.06 | S |
| J1102 + 2239 | 1940 | 2181 | 3.56 | 11.5 | 11.2 | 0.08 | S |
| J1110 + 3653 | 1230 | 2081 | 1.07 | 2.4 | 3.14 | 0.10 | S |
| J1138 + 3653 | 1231 | 1542 | 1.29 | 2.7 | 3.85 | 0.11 | S |
| J1146 + 3236 | 1737 | 1977 | 3.79 | 9.5 | 12.0 | 0.10 | S |
| J1159 + 2838 | 1907 | 2728 | 0.052 | 1.2 | 0.13 | 0.01 | N |
| J1227 + 3214 | 694 | 1567 | 0.51 | 0.52 | 1.42 | 0.21 | S |
| J1238 + 3942 | 940 | 1229 | 1.16 | 1.5 | 3.42 | 0.18 | S |
| J1246 + 0238 | 1667 | 1756 | 1.80 | 5.9 | 5.45 | 0.07 | S |
| J1333 + 4141 | 1589 | 2942 | 1.73 | 5.3 | 5.25 | 0.08 | S |
| J1346 + 3121 | 1074 | 1503 | 0.64 | 1.4 | 1.83 | 0.10 | S |
| J1348 + 2622 | 2192 | 3361 | 4.09 | 5.3 | 13.0 | 0.19 | S (based on Mg iiλ2798) |
| J1358 + 2658 | 1471 | 1805 | 3.20 | 6.3 | 10.1 | 0.12 | S |
| J1421 + 2824 | 1589 | 1724 | 7.18 | 11.2 | 23.7 | 0.16 | S |
| J1505 + 0326 | 1409 | 1337 | 0.41 | 1.9 | 1.12 | 0.05 | S |
| J1548 + 3511 | 1557 | 2217 | 4.37 | 8.3 | 14.0 | 0.13 | S |
| J1612 + 4219 | 777 | 1200 | 0.87 | 0.88 | 2.53 | 0.22 | S |
| J1629 + 4007 | 1246 | 1410 | 2.00 | 3.5 | 6.10 | 0.13 | S |
| J1633 + 4718 | 945 | 931 | 0.36 | 0.79 | 0.98 | 0.10 | S |
| J1634 + 4809 | 1856 | 1763 | 1.95 | 7.7 | 5.94 | 0.06 | S |
| J1644 + 2619 | 1129 | 1486 | 0.51 | 1.4 | 1.42 | 0.08 | S |
| J1709 + 2348 | 2377 | 1256 | 0.95 | 2.4 | 2.79 | 0.09 | S |
| J2007 − 4434 | 1869 | 2844 | 0.0081 | 0.43 | 0.018 | 0.003 | L (Oshlack et al. 2001) |
| J2021 − 2235 | 491 | 460 | − | 3.75 | 2.91 | 0.60 | M |
Notes. Columns: (1) name of the source; (2) line dispersion σline of the broad component of Hβ [km s-1]; (3) FWHM of the broad component of Hβ [km s-1]; (4) Hβ luminosity [1042 erg s-1]; (5) black hole mass [107 M⊙]; (6) disk luminosity [1044 erg s-1]; (7) disk luminosity [Eddington units]; (8) method adopted: A, from Asiago spectra; L, spectra from literature; M, derived from optical magnitudes; N, spectra downloaded from NED; S, from SDSS spectra.
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