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Table 8

AGN luminosity.

Galaxy name Type 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).

(a)

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.

(b)

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).

(c)

The L14−195   keV of NGC 7679 is likely to be contaminated by the nearby Seyfert 2 NGC 7682.

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