Table 8
AGN luminosity.
Galaxy name | Type |
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L14−195 keVa |
![]() |
![]() |
|||
(1042 erg s-1) | ||||||||
|
||||||||
NGC 3690 | Sy2 | 3.9b | <10 | 55 | 19 | |||
MCG−03-34-064 | Sy2 | 15 | 20 | 290 | 1.7 | |||
NGC 5135 | Sy2 | 10b | <16 | 180 | 3.9 | |||
IC 4518W | Sy2 | 2.2 | 18 | 26 | 21 | |||
MCG+04-48-002 | ··· | 6.9 | 38 | 120 | 3.0 | |||
NGC 7130 | Sy2 | 10b | <23 | 180 | 5.1 | |||
NGC 7469 | Sy1 | 17 | 39 | 340 | 5.0 | |||
NGC 7679 | Sy1 | 0.4 | 15c | 4.1 | 120 |
Notes. Intrinsic AGN 2–10 keV, 14–195 keV and bolometric luminosities. We used the bolometric corrections of Marconi et al. (2004).
Observed Swift/BAT 14–195 keV luminosity from Tueller et al. (2010). For non-detections we assumed a flux < 3.9 × 10-11 erg cm-2 s-1, which is the 4.8 σ sensitivity achieved for 95% of the sky in this survey.
Estimated from the 6.4 keV Fe Kα emission line luminosity using the relation LFeKα/L2−10 keV = 2 × 10-3 from Levenson et al. (2006).
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