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This article has an erratum: [https://doi.org/10.1051/0004-6361/201321430e]


Fig. 3

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Phased light curves for the two new variable stars, plotted in differential flux units and using the periods from Table 1. Black and red dots represent the data from the first and second nights of observation, respectively. The typical uncertainty in the period is about 0.01 d for both variables.

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