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Fig. 2
Absorbed spectra of 1E 1740.7−2942, which are modeled with diskbb + compTT, for the three XMM + INTEGRAL observations shown in this study. In only the 2012 spectrum, a feature at 7.11 keV (modeled as a Gauss in XSPEC), interpreted as being a Fe-edge (see text for details) is also included.
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