Fig. 3
Data, residuals, and unfolded spectra in the 0.2–10 keV range extracted from time slice 5 in orbit 0265 in 2001 (see Table A.2). Upper panel: the fit model comprises just the BMC and the Galactic absorption. Lower panel: the fit model is improved by the addition of the PEXRAV and the ZXIPCF components. A Gaussian emission line is also included whose parameters are E = 6.59 ± 0.19 keV, 
keV.
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