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KMT-2018-BLG-0029LB: A VERY LOW MASS-RATIO Spitzer MICROLENS PLANET

Gould, A; Ryu, YH; Novati, SC; Zang, WC; Albrow, MD; Chung, SJ; Han, C; Hwang, KH; Jung, YK; Shin, IG; Shvartzvald, Y; Yee, JC; Cha, SM; Kim, DJ; Kim, HW; Kim, SL; Lee, CU; Lee, DJ; Lee, Y; Park, BG; Pogge, RW; Beichman, C; Bryden, G; Carey, S; Gaud, BS; Henderson, CB; Zhu, W; Fouque, P; Penny, MT; Petric, A; Burdullis, T; Mao, SD

Gould, A (corresponding author), Max Planck Inst Astron, Konigstuhl 17, D-69117 Heidelberg, Germany.; Gould, A (corresponding author), Ohio State Univ, Dept Astron, 140 W 18th Ave, Columbus, OH 43210 USA.

JOURNAL OF THE KOREAN ASTRONOMICAL SOCIETY, 2020; 53 (1): 9

Abstract

At q = 1.81 +/- 0.20 x 10 KMT-2018-BLG-0029Lb has the lowest planet-host mass ratio q of any microlensing planet to date by more than a factor of two.......

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