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OGLE-2019-BLG-0362Lb: A Super-Jovian-Mass Planet around A Low-Mass Star
정선주,Jennifer C. Yee,Andrej Udalski,Andrew Gould,Michael D. Albrow,정연길,황규하,CHEONGHOHAN,Yoon-Hyun Ryu,신인구,Yossi Shvartzvald,Weicheng Zang,차상목,Dong Jin Kim,김승리,이충욱,Dong-Joo Lee,이용석,Byeong-Gon Park,Richar 한국천문학회 2022 Journal of The Korean Astronomical Society Vol.55 No.4
We present the analysis of a planetary microlensing event OGLE-2019-BLG-0362 with a short-duration anomaly (~0.4 days) near the peak of the light curve, which is caused by the resonant caustic. The event has a severe degeneracy with $\delcs = 0.9$ between the close and the wide binary lens models both with planet-host mass ratio $q \simeq 0.007$. We measure the angular Einstein radius but not the microlens parallax, and thus we perform a Bayesian analysis to estimate the physical parameters of the lens. We find that the OGLE-2019-BLG-0362L system is a super-Jovian-mass planet $M_{\rm p}=3.26^{+0.83}_{-0.58}~M_{\rm J}$ orbiting an M dwarf $M_{\rm h}=0.42^{+0.34}_{-0.23}~M_{\odot}$ at a distance $D_{\rm L} =5.83^{+1.04}_{-1.55}$ kpc. The projected star-planet separation is $a_{\perp} = 2.18^{+0.58}_{-0.72}~{\rm AU}$, which indicates that the planet lies beyond the snow line of the host star.