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Fig. 6.
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BXA fit of the phabs*zphabs*pow model to the Chandra X-ray data of CDF-S XT1 (left) and XT2 (right), where the darker (lighter) blue-filled bands enclose 68% (98%) of the posterior. The Galactic hydrogen column density and redshift are fixed parameters during the fitting process (see Table 3).
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