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Characterization of the Kepler-101 planetary system with HARPS-N⋆

AS Bonomo,A Sozzetti,C Lovis,L Malavolta,K Rice,LA Buchhave,D Sasselov,AC Cameron,DW Latham,E Molinari,F Pepe,S Udry,L Affer,D Charbonneau,R Cosentino,CD Dressing,X Dumusque,P Figueira,AFM Fiorenzano,S Gettel,A Harutyunyan,RD Haywood,K Horne,M Lopez-Morales,M Mayor,G Micela,F Motalebi,V Nascimbeni,DF Phillips,G Piotto,D Pollacco,D Queloz,D Ségransan,A Szentgyorgyi,C Watson

arXiv preprint arXiv:1409.4592（2014）

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摘要
We report on the characterization of the Kepler-101 planetary system, thanks to a combined DE-MCMC analysis of Kepler data and forty radial velocities obtained with the HARPS-N spectrograph. This system was previously validated by Rowe et al.(2014) and is composed of a hot super-Neptune, Kepler-101b, and an Earth-sized planet, Kepler-101c. These two planets orbit the slightly evolved and metal-rich G-type star in 3.49 and 6.03 days, respectively. With mass Mp= 51.1+ 5.1
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