Fig. 4.
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Correlations between the best-fit parameters i.e. the height, the photon index, and the energy transferred to the corona) and the X-ray (2–10 keV) and UV observed fluxes. The red lines show the best-fit straight line or power-law model, and the black squares show the binned data. The numbers in each plot show the significance at which each slope is different from zero.
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