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Muraki","submitted_at":"2017-05-10T20:00:26Z","abstract_excerpt":"We present the MOA Collaboration light curve data for planetary microlensing event OGLE-2015-BLG-0954, which was previously announced in a paper by the KMTNet and OGLE Collaborations. The MOA data cover the caustic exit, which was not covered by the KMTNet or OGLE data, and they provide a more reliable measurement of the finite source effect. The MOA data also provide a new source color measurement that reveals a lens-source relative proper motion of $\\mu_{\\rm rel} = 11.8\\pm 0.8\\,$mas/yr, which compares to the value of $\\mu_{\\rm rel} = 18.4\\pm 1.7\\,$mas/yr reported in the KMTNet-OGLE paper. 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