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Fig. 2


X-ray spectra: Combined Suzaku/XMM-Newton spectrum of PMN J1603–4904 (blue), Chandra/ACIS spectrum of PMN J1603–4904 (black), and Chandra/ACIS spectrum of the source east of PMN J1603–4904 (pink). A best-fit absorbed power law is shown for the two Chandra spectra. The fit models shown are the best fit power-law models for the Chandra spectrum and the APEC model for the combined Suzaku/XMM data. Residuals are given for the a) best fit power-law spectrum, b) the combined APEC fit, and c) the Suzaku/XMM APEC fit.

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