OGLE-2016-BLG-1093Lb: A Sub-Jupiter-mass Spitzer Planet Located in the Galactic Bulge

Author:

Shin In-GuORCID,Yee Jennifer C.ORCID,Hwang Kyu-HaORCID,Gould Andrew,Udalski AndrzejORCID,Bond Ian A.,Albrow Michael D.ORCID,Chung Sun-JuORCID,Han CheonghoORCID,Kil Jung Youn,Woo Kim Hyoun,Ryu Yoon-HyunORCID,Shvartzvald YossiORCID,Zang WeichengORCID,Cha Sang-Mok,Kim Dong-Jin,Kim Seung-LeeORCID,Lee Chung-UkORCID,Lee Dong-Joo,Lee Yongseok,Park Byeong-GonORCID,Pogge Richard W.ORCID,Mróz PrzemekORCID,Szymański Michał K.ORCID,Skowron JanORCID,Poleski Radek,Soszyński IgorORCID,Pietrukowicz PawełORCID,Kozłowski SzymonORCID,Ulaczyk KrzysztofORCID,Beichman Charles A.,Bryden GeofferyORCID,Calchi Novati Sebastiano,Carey Sean,Gaudi B. ScottORCID,Henderson Calen B.ORCID,Zhu WeiORCID,Abe Fumio,Barry Richard K.ORCID,Bennett David P.ORCID,Bhattacharya Aparna,Fujii Hirosane,Fukui AkihikoORCID,Hirao YukiORCID,Itow YoshitakaORCID,Kirikawa Rintaro,Koshimoto NaokiORCID,Kondo IonaORCID,Matsubara Yutaka,Matsumoto Sho,Miyazaki ShotaORCID,Muraki YasushiORCID,Olmschenk GregORCID,Okamura Arisa,Ranc ClémentORCID,Rattenbury Nicholas J.ORCID,Satoh YukiORCID,Silva Stela Ishitani,Sumi TakahiroORCID,Suzuki Daisuke,Toda Taiga,Tristram Paul J.,Vandorou AikateriniORCID,Yama Hibiki

Abstract

Abstract OGLE-2016-BLG-1093 is a planetary microlensing event that is part of the statistical Spitzer microlens parallax sample. The precise measurement of the microlens parallax effect for this event, combined with the measurement of finite-source effects, leads to a direct measurement of the lens masses and system distance, M host =0.38–0.57 M and m p = 0.59–0.87 M Jup, and the system is located at the Galactic bulge (D L ∼ 8.1 kpc). Because this was a high-magnification event, we are also able to empirically show that the “cheap-space parallax” concept produces well-constrained (and consistent) results for ∣π E∣. This demonstrates that this concept can be extended to many two-body lenses. Finally, we briefly explore systematics in the Spitzer light curve in this event and show that their potential impact is strongly mitigated by the color constraint.

Publisher

American Astronomical Society

Subject

Space and Planetary Science,Astronomy and Astrophysics

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