Characterization of the planetary system Kepler-101 with HARPS-N.
A hot super-Neptune with an Earth-sized low-mass companion

A. S. Bonomo, A. Sozzetti, C. Lovis, L. Malavolta, K. Rice, L. A. Buchhave, D. Sasselov, A. Collier Cameron, D. W. Latham, E. Molinari, F. Pepe, S. Udry, L. Affer, D. Charbonneau, R. Cosentino, C. D. Dressing, X. Dumusque, P. Figueira, A. F. Martinez Fiorenzano, S. Gettel, A. Harutyunyan, R. D. Haywood, K. Horne, M. López-Morales, M. Mayor, G. Micela, F. Motalebi, V. Nascimbeni, D. F. Phillips, G. Piotto, D. Pollacco, D. Queloz, D. Ségransan, A. Szentgyorgyi, C. A. Watson

Keywords
planetary systems – stars: fundamental parameters – t echniques: photometri c – techniques: radial velocities – techniques: spectroscopic

Astronomy and Astrophysics
Volume 572, Page A2_1
December 2014

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