Fig. 21
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Top: simultaneous spectral fit of an absorbed power law to the spectra of SXP 726 using observations 700001–5 (marked in black, red, green, blue, and cyan, respectively). Bottom: spectrum of SXP 726 from observation 710000. All spectra are obtained by combining data from TM1–4 and 6. The histograms trace the best-fit model, and the residuals are plotted in the narrow panels.
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