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Fig. C.1.

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SED of A0620-00 simulated with our toy model, using the physical parameters of Cantrell et al. (2010). The accretion disc contribution to the SED (blue) consists of a multicolour blackbody (dashed magenta) plus an inner hot-spot with Th = 10000 K (dashed cyan). The flux of the Hα line (green Gaussian) has been scaled so that EW = 58 Å. For comparison, we overlay SED photometric points from Froning et al. (2011).

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