Fig. 11
Variations in veling factor (VF, upper panel) and V magnitude (lower panel) over the 3rd observing period in August 2005 (photometric data from SMARTS and ASAS). The shaded area indicates the time interval over which X-ray observations were obtained (2nd point in Fig. 10). The large drop in veiling occurred from the second to the third night of ground-based observations.
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