no code implementations • 21 Dec 2020 • Yun Hak Kim, Sun-Ju Chung, A. Udalski, Ian A. Bond, Youn Kil Jung, Andrew Gould, Michael D. Albrow, Cheongho Han, Kyu-Ha Hwang, Yoon-Hyun Ryu, In-Gu Shin, Yossi Shvartzvald, Jennifer C. Yee, Weicheng Zang, Sang-Mok Cha, Dong-Jin Kim, Hyoun-Woo Kim, Seung-Lee Kim, Chung-Uk Lee, Dong-Joo Lee, Yongseok Lee, Byeong-Gon Park, Richard W. Pogge, Radek Poleski, Przemek Mroz, Jan Skowron, Michal K. Szymanski, Igor Soszynski, Pawel Pietrukowicz, Syzmon Kozlowski, Krzysztof Ulaczyk, Krzysztof A. Rybicki, Patryk Iwanek, Fumio Abe, Richard Barry, David P. Bennett, Aparna Bhattacharya, Martin Donachie, Hirosane Fujii, Akihiko Fukui, Yoshitaka Itow, Yuki Hirao, Rintaro Kirikawa, Iona Kondo, Naoki Koshimoto, Yutaka Matsubara, Yasushi Muraki, Shota Miyazaki, Clement Ranc, Nicholas J. Rattenbury, Yuki Satoh, Hikaru Shoji, Takahiro Sumi, Daisuke Suzuki, Paul J. Tristram, Yuzuru Tanaka, Tsubasa Yamawaki, Atsunori Yonehara
From this, we find that the lens system has a star with mass $M_{\rm h}=0. 55^{+0. 36}_{-0. 29} \ M_{\odot}$ hosting a giant planet with $M_{\rm p}=5. 53^{+3. 62}_{-2. 87} \ M_{\rm Jup}$, at a distance of $D_{\rm L}=5. 67^{+1. 11}_{-1. 52}\ {\rm kpc}$.
Earth and Planetary Astrophysics Astrophysics of Galaxies
1 code implementation • 17 Sep 2020 • Sean K. Terry, Aparna Bhattacharya, David P. Bennett, Jean-Phillipe Beaulieu, Naoki Koshimoto, Joshua W. Blackman, Ian A. Bond, Andrew A. Cole, Calen B. Henderson, Jessica R. Lu, Jean Baptiste Marquette, Clement Ranc, Aikaterini Vandorou
The $\sim$10 year baseline between the event and the Keck observations allows the planetary host star to be detected at a separation of $66. 5\pm 1. 7\,$mas from the source star, consistent with the light curve model prediction.
Earth and Planetary Astrophysics Astrophysics of Galaxies Instrumentation and Methods for Astrophysics
