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Fig. 4


Spectra of the five AGN with the best counting statistics (34 net counts 148). Spectra in panels a) and c) are extracted from Chandra, while spectra in panels b), d) and e) are from XMM-Newton. The a), b) and d) spectra are fit by a power-law model with Galactic and intrinsic absorption; the c) and e) spectra are fit by a simple power-law model plus Galactic absorption. The black, red, and green points and lines in the b) and d) panels correspond to pn, MOS1, and MOS2, respectively. The black and red points and lines in the e) panel correspond to pn and combined MOS1 and MOS2, respectively. For the sake of clarity, we display the spectra using a minimum binning of 20, 15, 3, 3 and 20 counts for each bin for J0100+2802, J1030+0524, J1120+0641, J1148+5251 and J1306+0356, respectively.

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