Fig. 8
Derived properties of the daily flux variation. The panels are: a) 2.5–25 keV bolometric flux due to the disk black-body component, termed black-body (BB) flux, b) 2.5–25 keV flux due to the power-law component, termed power-law (PL) flux, c) 2.5–25 keV total flux, and d) the ratio of the total to PL fluxes. The error bars of the model fitted fluxes are at 1σ level.
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