期刊
MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
卷 454, 期 1, 页码 946-951出版社
OXFORD UNIV PRESS
DOI: 10.1093/mnras/stv2045
关键词
gravitational lensing: micro; planets and satellites: detection; stars: individual: MOA-2010-BLG-353
资金
- Japan Society for the Promotion of Science (JSPS) [JSPS23103002, JSPS24253004, JSPS26247023, JSPS25103508, JSPS23340064]
- Royal Society of New Zealand Marsden Grant [MAU1104]
- NeSI's collaborator institutions
- Ministry of Business, Innovation & Employment's Research Infrastructure programme
- Direct For Mathematical & Physical Scien
- Division Of Astronomical Sciences [GRANTS:13664515, 1211875] Funding Source: National Science Foundation
- Grants-in-Aid for Scientific Research [15H00781, 15J01676, 23340064, 26247023] Funding Source: KAKEN
We report the discovery of a possible planet in microlensing event MOA-2010-BLG-353. This event was only recognized as having a planetary signal after the microlensing event had finished, and following a systematic analysis of all archival data for binary lens microlensing events collected to date. Data for event MOA-2010-BLG-353 were only recorded by the high-cadence observations of the OGLE and MOA survey groups. If we make the assumptions that the probability of the lens star hosting a planet of the measured mass ratio is independent of the lens star mass or distance, and that the source star is in the Galactic bulge, a probability density analysis indicates the planetary system comprises a 0.9(-0.53)(+1.6) M-Saturn mass planet orbiting a 0.18(-0.11)(+0.32) M-circle dot red dwarf star, 6.43(-1.15)(+1.09) kpc away. The projected separation of the planet from the host star is 1.72(-0.48)(+0.56) au. Under the additional assumption that the source is on the far side of the Galactic bulge, the probability density analysis favours a lens system comprising a slightly lighter planet.
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