Fig. 1

Contours of the corona optical depth τ
(in red), the amplification factor A
(in blue) andthe minimal fraction (in %) of disk intrinsic emission
(in green) in the corona spectral parameter Γ-kT
plane. A slab geometry (i.e., g = 1
in Eq. (21)) is assumed here. Smaller values of g
(i.e., a patchy corona) would move the green contours down. The magenta rectangle corresponds to the
Γ
and temperature kTe
ranges obtained by P13 for the soft excess in the spectral analysis of the Mkn 509 campaign.
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