MOA-2010-BLG-328Lb: A sub-Neptune orbiting very late M dwarf?
We analyze the planetary microlensing event MOA-2010-BLG-328. The best fit yields host and planetary massesof Mh = 0.11 ± 0.01M and Mp = 9.2 ± 2.2M?, corresponding to a very late M dwarf and sub-Neptune-massplanet, respectively. The system lies at DL = 0.81 ± 0.10 kpc with projected separation r? =...
| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
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| Format: | Journal Article |
| Published: |
IOP Publishing Ltd.
2013
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| Subjects: | |
| Online Access: | http://iopscience.iop.org/0004-637X/779/2/91/pdf/0004-637X_779_2_91.pdf http://hdl.handle.net/20.500.11937/16718 |