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Fig. 9.

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Fraction of reflected over continuum emission from 10 to 40 keV as a function of absorption. The y values of the black points were estimated as the average reflection fraction of the individual MYTorus best-fit results. The blue dashed line denotes the predicted fraction in the case of a clumpy torus, as estimated by RefleX. The small break at NH ≃ 14 × 1022 cm−2 is probably due to computational noise.

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