Koshimoto, N, Shvartzvald, Y, Bennett, DP, Penny, MT, Hundertmark, M, Bond, IA, Zang, WC, Henderson, CB, Suzuki, D, Rattenbury, NJ, Sumi, T, Abe, F, Asakura, Y, Bhattacharya, A, Donachie, AM, Evans, TP, Li, MCA, Ling, CH, Masuda, K, Matsubara, Y, Matsuo, T, Muraki, Y, Nagakane, M, Ohnishi, K, Ranc, C, Saito, T, Sharan, A, Shibai, H, Sullivan, DJ, Tristram, PJ, Yamada, T, Yamada, T, Yonehara, A, Gelino, CR, Beichman, CA, Beaulieu, J-P, Marquette, J-B, Batista, V, Friedmann, M, Hallakoun, N, Kaspi, S, Maoz, D, Bryden, G, Novati, SC, Howell, SB, Wang, TS, Mao, S, Fouque, P, Korhonen, H
, Jorgensen, UG, Street, R, Kerins, E, Bachelet, E, Bozza, V & Bramich, DM 2017, '
MOA-2016-BLG-227Lb: A Massive Planet Characterized by Combining Light-curve Analysis and Keck AO Imaging',
Astronomical Journal, vol. 154, no. 1, 3.
https://doi.org/10.3847/1538-3881/aa72e0