X-ray view of four high-luminosity Swift/BAT AGN: Unveiling obscuration and reflection with Suzaku

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Table 6

Optical properties of the sample.

Source	Obs. date	E(B − V)_gal^a	E(B − V)_int^a	L(Hα)	L(Hβ)	L[OIII]λ5007	L[OIII]/L(Hβ)	L_{[2−10 keV]}^b	^c

3C 452	2006-11-21	0.14	0.84	40.94	40.09	40.89	6.31	43.81	832
3C 105	2006-11-21	0.48	0.92	41.15	40.26	41.5	17.38	44.21	513
J0318.7+6828	2006-11-21	0.72	0	41.17	40.74	41.64	7.94	44.08	275
J0918.5+0425	2004-03-09	0.04	0.26	41.63	41.03	42.1	14.75	44.30	159

Notes.De-reddened emission line properties taken from Winter et al. (2010), based on observations from the 2.1 m Kitt Peak National Observatory (KPNO) telescope except for J0918.5+0425, which is based on archival SDSS data. All luminosities are expressed as logarithms in units of erg s^-1.

^(a)

Milky Way and source-intrinsic extinction.

^(b)

Logarithm of the intrinsic 2–10 keV power law luminosity in erg s^-1.

^(c)

The ratio of the intrinsic 2–10 keV power law luminosity with respect to the corrected L[OIII].

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