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Fig. 5.
STELLA/WiFSIP photometry of 3XMM J183333.1+225136 obtained in July 2014 (top plot) and June 2015 (bottom plot). The relative flux is the flux of the optical counterpart divided by PSO J183332.533+225135.43, to correct for sky variations. The photometric uncertainties are of the order of the data scatter outside the eclipse.
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