New Giant Planet beyond the Snow Line for an Extended MOA Exoplanet Microlens Sample

Characterizing a planet detected by microlensing is hard if the planetary signal is weak or the lens-source relative trajectory is far from caustics. However, statistical analyses of planet demography must include those planets to accurately determine occurrence rates. As part of a systematic modeli...

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Veröffentlicht in:	arXiv.org 2021-07
Hauptverfasser:	Ranc, Clément, Bennett, David P, Barry, Richard K, Koshimoto, Naoki, Skowron, Jan, Hirao, Yuki, Bond, Ian A, Sumi, Takahiro, Bathe-Peters, Lars, Abe, Fumio, Bhattacharya, Aparna, Donachie, Martin, Fujii, Hirosane, Fukui, Akihiko, Stela Ishitani Silva, Itow, Yoshitaka, Kirikawa, Rintaro, Kondo, Iona, Man Cheung Alex Li, Matsubara, Yutaka, Muraki, Yasushi, Miyazaki, Shota, Olmschenk, Greg, Rattenbury, Nicholas J, Satoh, Yuki, Shoji, Hikaru, Suzuki, Daisuke, Tanaka, Yuzuru, Tristram, Paul J, Yamawaki, Tsubasa, Yonehara, Atsunori
Format:	Artikel
Sprache:	eng
Schlagworte:	Bayesian analysis Demography Extrasolar planets Galactic bulge Light curve Microlenses Milky Way Physical properties Physics - Astrophysics of Galaxies Physics - Earth and Planetary Astrophysics Statistical analysis
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