Fig. 4
Averaged XMM-Newton Epic-pn spectra of AX J1910.7+0917 extracted from the observations 0084100401 (top) and 0084100501 (bottom). In both cases we also show the best-fit model (an absorbed power-law) and the residuals from these fits. In the observation 0084100501 the residuals clearly showed an iron line at ~6.4 keV.
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