- Abstract:
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Initial RV characterisation of the enigmatic planet Kepler-10c suggested a mass of $\sim17$ M$_\oplus$, which was remarkably high for a planet with radius $2.32$ R$_\oplus$; further observations and subsequent analysis hinted at a (possibly much) lower mass, but masses derived using RVs from two different spectrographs (HARPS-N and HIRES) were incompatible at a $3\sigma$-level. We demonstrate here how such mass discrepancies may readily arise from sub-optimal sampling and/or neglecting to mod...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Version:
- Publisher's version
- Files:
-
-
(pdf, 435.1KB)
-
- Publisher copy:
- 10.1093/mnrasl/slx116
-
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- Publisher:
- Oxford University Press Publisher's website
- Journal:
- Monthly Notices of the Royal Astronomical Society: Letters Journal website
- Volume:
- 471
- Issue:
- 1
- Pages:
- L125-L130
- Publication date:
- 2017-07-22
- Acceptance date:
- 2017-07-19
- DOI:
- EISSN:
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1745-3933
- ISSN:
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1745-3925
- Pubs id:
-
pubs:709938
- URN:
-
uri:67f661ed-b1c6-4f36-86de-e2cf521f7616
- UUID:
-
uuid:67f661ed-b1c6-4f36-86de-e2cf521f7616
- Local pid:
- pubs:709938
- Paper number:
- 1
- Copyright holder:
- Rajpaul et al.
- Copyright date:
- 2017
- Notes:
-
Copyright © 2017 The Authors.
Published by Oxford University Press on behalf of the Royal Astronomical Society.
Journal article
Pinning down the mass of Kepler-10c: the importance of sampling and model comparison
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