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Fig. 3


Typical spectrum for an observation during the flaring phase of the giant outburst (obsid: 80067-11-03-05, Lx = 2.8 × 1037 erg s-1): in the upper panel, PCA and HEXTE data points and corresponding best fit are reported; below: residuals for the best fit a), the fit excluding the absorption feature at  ~11 keV b), and the one excluding the CRSF c), respectively.

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