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OGLE-2017-BLG-0406: Spitzer Microlens Parallax Reveals Saturn-mass Planet Orbiting M-dwarf Host in the Inner Galactic Disk

  • Authors: Yuki Hirao, David P. Bennett, Yoon-Hyun Ryu, Naoki Koshimoto, Andrzej Udalski, Jennifer C. Yee, Takahiro Sumi, Ian A. Bond, Yossi Shvartzvald, Fumio Abe, Richard K. Barry, Aparna Bhattacharya, Martin Donachie, Akihiko Fukui, Yoshitaka Itow, Iona Kondo, Man Cheung Alex Li, Yutaka Matsubara, Taro Matsuo, Shota Miyazaki, Yasushi Muraki, Masayuki Nagakane, Clément Ranc, Nicholas J. Rattenbury, Haruno Suematsu, Hiroshi Shibai, Daisuke Suzuki, Paul J. Tristram, Atsunori Yonehara, J. Skowron, R. Poleski, P. Mróz, M. K. Szymański, I. Soszyński, S. Kozłowski, P. Pietrukowicz, K. Ulaczyk, K. Rybicki, P. Iwanek, Michael D. Albrow, Sun-Ju Chung, Andrew Gould, Cheongho Han, Kyu-Ha Hwang, Youn Kil Jung, In-Gu Shin, 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, Charles A. Beichman, Geoffery Bryden, Sebastiano Calchi Novati, Sean Carey, B. Scott Gaudi, Calen B. Henderson, Wei Zhu, Etienne Bachelet, Greg Bolt, Grant Christie, Markus Hundertmark, Tim Natusch, Dan Maoz, Jennie McCormick, Rachel A. Street, Thiam-Guan Tan, Yiannis Tsapras, U. G. Jørgensen, M. Dominik, V. Bozza, J. Skottfelt, C. Snodgrass, S. Ciceri, R. Figuera Jaimes, D. F. Evans, N. Peixinho, T. C. Hinse, M. J. Burgdorf, J. Southworth, S. Rahvar, S. Sajadian, M. Rabus, C. von Essen, Y. I. Fujii, J. Campbell-White, S. Lowry, C. Helling, L. Mancini, L. Haikala, and Ryo Kandori

2020 The Astronomical Journal 160 74.

  • Provider: AAS Journals

Caption: Figure 2.

OGLE-2017-BLG-0406 parallax contours for the W+ solution. Left: the ground-only (elliptical) contours are derived from the covariance matrix from the MCMC, while the Spitzer-“only” (arc-like) contours are derived from the analytical expression in Equation (7). The colors (black, red, yellow, green, cyan, blue, magenta) represent ﹩{\rm{\Delta }}{\chi }^{2}\lt (1,4,9,16,25,36,49)﹩. Note that the 1σ contours for the ground-only and Spitzer-“only” measurements overlap. Right: Colored contours are the ﹩{\rm{\Delta }}{\chi }^{2}﹩ values for the sum of the two ﹩{\chi }^{2}﹩ distributions that are shown to the left. Despite the fact the each set of contours on the left provides essentially 1D information, the combination is well constrained in both dimensions. The white ellipses represent the 1σ, 2σ, and 3σ contours from the combined numerical fit to all of the data. The semi-analytic approach (colored contours) provides a very good, although not perfect, representation of the full numerical result. This shows that the semi-analytic approach enables one to accurately trace the information flow.

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