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Fig. 2


JEM-X1 (black), JEM-X2 (red), and ISGRI (green) spectra of IGR J17329-2731 extracted by using all combined data across revolutions 1850–1878 (excluding SCW 35 in revolution 1850). The best fit model is obtained with an absorbed power law (see text for details). The residuals from the fit are shown in the bottom panel.

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