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Mr\\'oz, P. Pietrukowicz, R.K. Barry, R. Poleski, S. Koz{\\l}owski, To. Saito, T. Sumi, Y. Asakura, Y. Hirao, Y. Itow, Y. Matsubara, Y. Muraki","submitted_at":"2018-03-14T12:33:32Z","abstract_excerpt":"We report on the analysis of a microlensing event OGLE-2014-BLG-1722 that showed two distinct short term anomalies. The best fit model to the observed light curves shows that the two anomalies are explained with two planetary mass ratio companions to the primary lens. Although a binary source model is also able to explain the second anomaly, it is marginally ruled out by 3.1 $\\sigma$. 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