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We present the results from broad-band X-ray spectral analysis of 3C 206 andPKS 0707-35 with Suzaku and Swift/BAT, two of the most luminous unobscured andobscured radio-loud active galactic nuclei with hard X-ray luminosities of10^{45.5} erg s^{-1} and 10^{44.9} erg s^{-1} (14--195 keV), respectively.Based on the radio core luminosity, we estimate that the X-ray spectrum of 3C206 contains a significant (~ 60% in the 14--195 keV band) contribution fromthe jet, while it is negligible in PKS 0707-35. We can successfully model thespectra with the jet component (for 3C 206), the transmitted emission, and tworeflection components from the torus and the accretion disk. The reflectionstrengths from the torus are found to be R_{torus} (= \Omega/2\pi) = 0.29 +-0.18 and 0.41 +- 0.18 for 3C 206 and PKS 0707-35, respectively, which aresmaller than those in typical Seyfert galaxies. Utilizing the torus model byIkeda et al. (2009), we quantify the relation between the half opening angle ofa torus (\theta_{oa}) and the equivalent width of an iron-K line. The observedequivalent width of 3C 206, < 71 eV, constrain the column density in theequatorial plane to N_{H}^{eq} < 10^{23} cm^{-2}, or the half opening angle to\theta_{oa} > 80^\circ if N_{H}^{eq} = 10^{24} cm^{-2} is assumed. That of PKS0707-35, 72 +- 36 eV, is consistent with N_{H}^{eq} ~ 10^{23} cm^{-2}. Ourresults suggest that the tori in luminous radio-loud AGNs are only poorlydeveloped. The trend is similar to that seen in radio-quiet AGNs, implying thatthe torus structure is not different between AGNs with jets and without jets.

Suzaku View of the Swift/BAT Active Galactic Nuclei. V. Torus Structure of Two Luminous Radio-loud AGNs (3C 206 and PKS 0707-35)