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Koz{\\l}owski, T. Matsuo, To. Saito, T. Sumi, Y. Asakura, Y. Hirao, Y. Itow, Y. Matsubara, Y. Muraki","submitted_at":"2016-04-19T08:00:16Z","abstract_excerpt":"We report the discovery of a planet by the microlensing method, OGLE-2012-BLG-0724Lb. Although the duration of the planetary signal for this event was one of the shortest seen for a planetary event, the anomaly was well covered thanks to high cadence observations taken by the survey groups OGLE and MOA. By analyzing the light curve, this planetary system is found to have a mass ratio $q=(1.58\\pm0.15)\\times10^{-3}$. 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Bhattacharya, A. Fukui, A. Sharan, A. Udalski, A. Yonehara, C.H. Ling, D.J. Sullivan, D.P. Bennett, D. Suzuki, F. Abe, H. Oyokawa, H. Shibai, I.A. Bond, I. Soszy\\'nski, J. Skowron, K. Masuda, K. Ohnishi, K. Ulaczyk, \\L. Wyzykowski, M.C.A. Li, M. Freeman, M.K. Szyma\\'nski, M. Nagakane, N. Koshimoto, N. Rattenbury, P.J. Tristram, P. Mr\\'oz, P. Pietrukowicz, R. Poleski, S. Koz{\\l}owski, T. Matsuo, To. Saito, T. Sumi, Y. Asakura, Y. Hirao, Y. Itow, Y. Matsubara, Y. Muraki","submitted_at":"2016-04-19T08:00:16Z","abstract_excerpt":"We report the discovery of a planet by the microlensing method, OGLE-2012-BLG-0724Lb. Although the duration of the planetary signal for this event was one of the shortest seen for a planetary event, the anomaly was well covered thanks to high cadence observations taken by the survey groups OGLE and MOA. By analyzing the light curve, this planetary system is found to have a mass ratio $q=(1.58\\pm0.15)\\times10^{-3}$. 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