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| Verfasst von: | Hirao, Yuki [VerfasserIn]  |
| Hundertmark, Markus [VerfasserIn] | |
| Natusch, Tim [VerfasserIn] | |
| Maoz, Dan [VerfasserIn] | |
| McCormick, Jennie [VerfasserIn] | |
| Street, Rachel A. [VerfasserIn] | |
| Tan, Thiam-Guan [VerfasserIn] | |
| Tsapras, Yiannis [VerfasserIn] | |
| Jørgensen, U. G. [VerfasserIn] | |
| Dominik, M. [VerfasserIn] | |
| Bozza, V. [VerfasserIn] | |
| Skottfelt, J. [VerfasserIn] | |
| Snodgrass, C. [VerfasserIn] | |
| Ciceri, S. [VerfasserIn] | |
| Jaimes, R. Figuera [VerfasserIn] | |
| Evans, D. F. [VerfasserIn] | |
| Peixinho, N. [VerfasserIn] | |
| Hinse, T. C. [VerfasserIn] | |
| Burgdorf, M. J. [VerfasserIn] | |
| Southworth, J. [VerfasserIn] | |
| Rahvar, S. [VerfasserIn] | |
| Sajadian, S. [VerfasserIn] | |
| Rabus, M. [VerfasserIn] | |
| Essen, C. von [VerfasserIn] | |
| Fujii, Y. I. [VerfasserIn] | |
| Campbell-White, J. [VerfasserIn] | |
| Lowry, S. [VerfasserIn] | |
| Helling, C. [VerfasserIn] | |
| Mancini, L. [VerfasserIn] | |
| Haikala, L. [VerfasserIn] | |
| Kandori, Ryo [VerfasserIn] | |
| Titel: | OGLE-2017-BLG-0406 |
| Titelzusatz: | spitzer microlens parallax reveals Saturn-mass planet orbiting M-dwarf host in the inner galactic disk |
| Verf.angabe: | 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 |
| E-Jahr: | 2020 |
| Jahr: | 2020 July 23 |
| Umfang: | 20 S. |
| Fussnoten: | Gesehen am 14.12.2020 |
| Titel Quelle: | Enthalten in: The astronomical journal |
| Ort Quelle: | London : Institute of Physics Publ., 1998 |
| Jahr Quelle: | 2020 |
| Band/Heft Quelle: | 160(2020,2) Artikel-Nummer 74, 20 Seiten |
| ISSN Quelle: | 1538-3881 |
| Abstract: | We report the discovery and analysis of the planetary microlensing event OGLE-2017-BLG-0406, which was observed both from the ground and by the Spitzer satellite in a solar orbit. At high magnification, the anomaly in the light curve was densely observed by ground-based-survey and follow-up groups, and it was found to be explained by a planetary lens with a planet/host mass ratio of from the light-curve modeling. The ground-only and Spitzer-“only” data each provide very strong one-dimensional (1D) constraints on the 2D microlens parallax vector . When combined, these yield a precise measurement of and of the masses of the host and planet M planet = 0.41 ± 0.05 M Jup. The system lies at a distance D L = 5.2 ± 0.5 kpc from the Sun toward the Galactic bulge, and the host is more likely to be a disk population star according to the kinematics of the lens. The projected separation of the planet from the host is (i.e., just over twice the snow line). The Galactic-disk kinematics are established in part from a precise measurement of the source proper motion based on OGLE-IV data. By contrast, the Gaia proper-motion measurement of the source suffers from a catastrophic 10σ error. |
| DOI: | doi:10.3847/1538-3881/ab9ac3 |
| URL: | Bitte beachten Sie: Dies ist ein Bibliographieeintrag. Ein Volltextzugriff für Mitglieder der Universität besteht hier nur, falls für die entsprechende Zeitschrift/den entsprechenden Sammelband ein Abonnement besteht oder es sich um einen OpenAccess-Titel handelt. Volltext ; Verlag: https://doi.org/10.3847/1538-3881/ab9ac3 |
| Volltext: https://iopscience.iop.org/article/10.3847/1538-3881/ab9ac3 | |
| DOI: https://doi.org/10.3847/1538-3881/ab9ac3 | |
| Datenträger: | Online-Ressource |
| Sprache: | eng |
| K10plus-PPN: | 1742699243 |
| Verknüpfungen: | → Zeitschrift |
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