MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Light-curve Analysis and Keck AO Imaging

N. Koshimoto, Y. Shvartzvald, D. P. Bennett, M. T. Penny, M. Hundertmark, I. A. Bond, W. C. Zang, Calen B. Henderson, D. Suzuki, N. J. Rattenbury, T. Sumi, Fumiko Abe, Y. Asakura, A. Bhattacharya, A.M. Donachie, Tom P. Evans, M. C. A. Li, C. H. Ling, K. Masuda, Yoichi MatsubaraT. Matsuo, Y. Muraki, M. Nagakane, K. Ohnishi, C. Ranc, To. Saito, A. Sharan, H. Shibai, D. J. Sullivan, P.J. Tristram, T. Yamada, T. Yamada, A. Yonehara, C. R. Gelino, C. A. Beichman, J.-P Beaulieu, J.-B Marquette, V. Batista, M. Friedmann, N. Hallakoun, S. Kaspi, Dan Maoz, G. Bryden, S. Calchi Novati, Steve B. Howell, T. S. Wang, Shenlan Mao, P. Fouque, H. Korhonen, U. G. Jorgensen, R. Street, E. Kerins, E. Bachelet, V. Bozza, D. M. Bramich

21 Citations (Scopus)
Original languageEnglish
Article number3
JournalAstronomical Journal
Volume154
Issue number1
ISSN0004-6256
DOIs
Publication statusPublished - Jul 2017

Keywords

  • gravitational lensing: micro
  • planetary systems

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