Fig. 5.
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Spectral models computed with the uxclumpy code described in (Buchner et al. 2019) rescaled to the observed 10–30 keV flux from the stacking analysis. We refer to the text for details on the model assumptions and geometry. The column density increases from 5 × 1023 cm−2 (red curve) to 2 × 1024 cm−2 (blue curve) and 1025 cm−2 (cyan curve). The UHB detection and the upper limits in the SB and MB are also reported.
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