Journal
ASTRONOMY & ASTROPHYSICS
Volume 641, Issue -, Pages -Publisher
EDP SCIENCES S A
DOI: 10.1051/0004-6361/202038173
Keywords
gravitational lensing: micro; planets and satellites: detection; brown dwarfs
Categories
Funding
- National Research Foundation of Korea [2017R1A4A1015178, 2019R1A2C2085965]
- JPL grant [1500811]
- National Research Foundation of Korea [2017R1A4A1015178, 2019R1A2C2085965] Funding Source: Korea Institute of Science & Technology Information (KISTI), National Science & Technology Information Service (NTIS)
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Aims. We announce the discovery of a microlensing planetary system, in which a sub-Saturn planet is orbiting an ultracool dwarf host. Methods. We detected the planetary system by analyzing the short-timescale (t(E) similar to 4.4 days) lensing event KMT-2018-BLG-0748. The central part of the light curve exhibits asymmetry due to negative deviations in the rising side and positive deviations in the falling side. Results. We find that the deviations are explained by a binary-lens model with a mass ratio between the lens components of q similar to 2 x 10(-3). The short event timescale, together with the small angular Einstein radius, theta(E) similar to 0.11 mas, indicate that the mass of the planet host is very small. The Bayesian analysis conducted under the assumption that the planet frequency is independent of the host mass indicates that the mass of the planet is M-p = 0.18(-0.10)(+0.29) M-J, and the mass of the host, M-h = 0.087(-0.047)(+0.138) M-circle dot, is near the starbrown dwarf boundary, but the estimated host mass is sensitive to this assumption about the planet hosting probability. High-resolution follow-up observations would lead to revealing the nature of the planet host.
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