Fig. 3
EPIC-pn (black), EPIC-MOS1 (red), and EPIC-MOS2 (green) spectra of XTE J1743-363 extracted by using the entire exposure time available from the XMM-Newton observation. The best fit is obtained here with an absorbed BMC model. The residuals from this fit are shown in the bottom panel. The middle panel shows the residuals from a fit with a simple power-law model.
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