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Fig. 1

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Background-subtracted X-ray and UV light curves of V405 Peg obtained with XMM-Newton on Dec. 29, 2009. The data were binned using a bin size of 100 s. They are shown in original time sequence with time transformed to binary phase using the ephemeris of Thorstensen et al. (2009). Phase zero refers to the inferior conjunction of the secondary star.

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