(Q59215372)

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Pinning down the mass of Kepler-10c: the importance of sampling and model comparison

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Pinning down the mass of Kepler-10c: the importance of sampling and model comparison (English)

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S. Aigrain

3

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Lars A. Buchhave

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2

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L. A. Buchhave

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V. Rajpaul

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1

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publication date

22 July 2017

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published in

Monthly Notices of the Royal Astronomical Society: Letters

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volume

471

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issue

1

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page(s)

L125-L130

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cites work

KEPLER 'S FIRST ROCKY PLANET: KEPLER-10b

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https://api.crossref.org/works/10.1093%2FMNRASL%2FSLX116

retrieved

21 January 2018

Radial velocity planets de-aliased: a new, short period for super-earth 55 Cnc e

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https://api.crossref.org/works/10.1093%2FMNRASL%2FSLX116

retrieved

21 January 2018

The Kepler-10 planetary system revisited by HARPS-N: a hot rocky world and a solid neptune-mass planet

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Crossref

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https://api.crossref.org/works/10.1093%2FMNRASL%2FSLX116

retrieved

21 January 2018

KEPLER-10 c: A 2.2 EARTH RADIUS TRANSITING PLANET IN A MULTIPLE SYSTEM

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https://api.crossref.org/works/10.1093%2FMNRASL%2FSLX116

retrieved

21 January 2018

False positive probabilities for all Kepler objects of interest: 1284 newly validated planets and 428 likely false positives

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reference URL

https://api.crossref.org/works/10.1093%2FMNRASL%2FSLX116

retrieved

21 January 2018

A Gaussian process framework for modelling stellar activity signals in radial velocity data

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stated in

Crossref

reference URL

https://api.crossref.org/works/10.1093%2FMNRASL%2FSLX116

retrieved

21 January 2018

Ghost in the time series: no planet for Alpha Cen B

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reference URL

https://api.crossref.org/works/10.1093%2FMNRASL%2FSLX116

retrieved

21 January 2018

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DOI

10.1093/MNRASL/SLX116

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(Q59215372)

Pinning down the mass of Kepler-10c: the importance of sampling and model comparison

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