Fig. 3.
GX13+1 XMM-Newton EPIC pn spectra. Left panel: spectrum of Obs. 1 in the 2.5–10 keV energy range, the data (in black), and the total model TBABS*(BBODYRAD+COMPTT+WINDLINE(6.6 KEV))*LGABS*LGABS*LGABS (solid red line). Right panel: spectrum of Obs. 2 in the 2.5–10 keV energy range, the data (in black), and the best-fit model TBABS*(BBODYRAD+COMPTT+WINDLINE(6.6 KEV))*LGABS (solid red line). The lower panels, in the left and right figures, show the residuals of the data vs. model.
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