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    • The First Planetary Microlensing Event with Two Microlensed Source Stars 

      Bennett DP; Udalski A; Han C; Bond IA; Beaulieu JP; Skowron J; Gaudi BS; Koshimoto N; Abe F; Asakura Y; Barry RK; Bhattacharya A; Donachie M; Evans P; Fukui A; Hirao Y; Itow Y; Li MCA; Ling CH; Masuda K; Matsubara Y; Muraki Y; Nagakane M; Ohnishi K; Oyokawa H; Ranc C; Rattenbury NJ; Rosenthal MM; Saito T; Sharan A; Sullivan DJ; Sumi T; Suzuki D; Tristram PJ; Yonehara A; Szymański MK; Poleski R; Soszyński I; Ulaczyk K; Wyrzykowski; Depoy D; Gould A; Pogge RW; Yee JC; Albrow MD; Bachelet E; Batista V; Bowens-Rubin R; Brillant S; Caldwell JAR; Cole A; Coutures C; Dieters S; Prester DD; Donatowicz J; Fouqué P; Horne K; Hundertmark M; Kains N; Kane SR; Marquette JB; Menzies J; Pollard KR; Ranc C; Sahu KC; Wambsganss J; Williams A; Zub M (2018)
      © 2018. The American Astronomical Society. All rights reserved. We present the analysis of the microlensing event MOA-2010-BLG-117, and show that the light curve can only be explained by the gravitational lensing of a ...