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 Citationer (Scopus)
OriginalsprogEngelsk
Artikelnummer3
TidsskriftAstronomical Journal
Vol/bind154
Udgave nummer1
ISSN0004-6256
DOI
StatusUdgivet - jul. 2017

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