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Fig. 14


Fit to the spectrum of the CXB measured by INTEGRAL IBIS/ISGRI (squares, Türler et al. 2010). The model used is a combination of our best-fit models for the average spectra of the different classes of objects (AB and LOB), normalizing their ratio using the N   H distribution of Treister et al. (2009). We also show the data obtained by INTEGRAL JEM-X (stars, Türler et al. 2010) and Swift BAT (triangles, Ajello et al. 2008b) above 10 keV.

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