Fig. 9

X-ray and UV light curves folded with the orbital period and ephemerides determined from the spectroscopy. The two orbital periods were observed by Swift. The X-ray flux peaks briefly at around orbital phase 0.2, while there seems to be a deep minimum at the phase between phases 0.5 and 0.7. The UV light curve in two filters (UVW1 blue squares and UVM2 red triangles) presented in the upper panel shows a behavior similar to that in the X-ray, except that the maximum peak is shifted relative to X-rays by 0.2 orbital phases and reaches maximum at 0.4.
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