Table 1
Absorption-corrected 2.0–10 keV X-ray luminosities, bolometric luminosities, black hole masses and Eddington ratios for two Seyfert subtypes.
| Name | Seyfert |
|
|
|
|
log MBH | Ref | logλX | logλ [OIII] |
| type | (erg s-1) | (erg s-1) | (erg s-1) | (erg s-1) | (M⊙) | ||||
|
|
|||||||||
| MCG+8-11-11 | 1 | 43.79 | 42.43 | 45.25 | 45.09 | 8.06 | 6 | –1.92 | –2.09 |
| MRK 1218 | 1 | 42.69 | 41.61 | 43.87 | 43.76 | .... | .... | .... | .... |
| NGC 2639 | 1 | 41.92 | 40.86 | 42.94 | 43.02 | 8.02 | 3 | –4.20 | –4.12 |
| NGC 4151 | 1 | 42.40 | 41.39 | 43.51 | 43.54 | 7.18 | 2 | –2.79 | –2.75 |
| MRK 766 | 1 | 42.50 | 41.84 | 43.62 | 43.99 | 6.64 | 4 | –2.13 | –1.76 |
| MRK 231 | 1 | 42.53 | 41.96† | 43.66 | 45.51 | 7.24 | 5 | –2.69 | –0.85 |
| ARK 564 | 1 | 43.37 | 41.38† | 44.71 | 44.93 | 6.50 | 4 | –0.91 | –0.69 |
| NGC 7469 | 1 | 43.45 | 42.96 | 44.82 | 45.62 | 6.84 | 7 | –1.14 | –0.34 |
| MRK 926 | 1 | 44.20 | 42.25† | 45.79 | 45.79 | 7.14 | 6 | –0.47 | –0.46 |
| MRK 530 | 1 | 43.70 | 40.98† | 45.14 | 44.53 | 8.08 | 7 | –2.06 | –2.67 |
| MRK 348 | 2 | 43.45 | 42.19 | 44.81 | 44.85 | 7.21 | 7 | –1.51 | –1.47 |
| MRK 1 | 2 | 42.50 | 42.39 | 43.63 | 45.04 | 7.16 | 7 | –2.64 | –1.23 |
| NGC 2273 | 2 | 42.74 | 41.16 | 43.92 | 43.82 | 7.30 | 7 | –2.50 | –2.60 |
| MRK 78 | 2 | 44.09 | 43.29 | 45.64 | 45.94 | 7.87 | 7 | –1.34 | –1.04 |
| NGC 5135 | 2 | 42.68 | 42.42 | 43.85 | 45.08 | 7.35 | 1 | –2.62 | –1.39 |
| MRK 477 | 2 | 44.44 | 43.44 | 46.11 | 46.10 | 7.20 | 1 | –0.21 | –0.22 |
| NGC 5929 | 2 | 42.04 | 40.98 | 43.07 | 43.64 | 7.25 | 7 | –3.29 | –2.72 |
| NGC 7212 | 2 | 43.90 | 42.80 | 45.39 | 45.46 | 7.47 | 1 | –1.19 | –1.12 |
| MRK 533 | 2 | 43.91 | 42.64 | 45.41 | 45.30 | 7.56 | 7 | –1.27 | –1.38 |
| NGC 7682 | 2 | 43.07 | 41.76 | 44.33 | 44.42 | 7.28 | 7 | –2.06 | –1.98 |
Notes. Column (1), source name; Col. (2), Seyfert subtype; Col. (3), absorption-corrected 2.0–10 keV X-ray luminosity; Col. (4), extinction-corrected [OIII] luminosity; Col. (5), bolometric luminosity derived from 2.0–10 keV X-ray luminosity; Col. (6), bolometric luminosity derived from [OIII] line luminosity; Col. (7), black hole masses; Col. (8), references for black hole masses; Col. (9) Eddington ratio where the estimated bolometric luminosity is derived from X-ray luminosity; Col. (10), Eddington ratio where the estimated bolometric luminosity is derived from [OIII] line luminosity.
References. 1: Bian & Gu (2007), 2: Kaspi et al. (2000), 3: McElory (1995), 4: Merloni et al. (2003), 5: Dasyra et al. (2006), 6: Wang & Zhang (2007), 7: Woo & Urry (2002).
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