Characterization of small planets with Kepler and HARPS-N

A. S. Bonomo, A. Sozzetti, C. Lovis, L. Malavolta, K. Rice, X. Dumusque, A. C. Cameron, D. W. Latham, E. Molinari, F. Pepe, S. Udry

Research output: Contribution to conferenceAbstract

Abstract

The high-accuracy and high-precision HARPS-N spectrograph has been installed at the italian Telescopio Nazionale Galileo in La Palma approximately two years and a half ago. Eighty nights per year of Guaranteed Time of Observation are mostly dedicated to the radial-velocity (RV) follow up of Kepler small-size planetary candidates to establish their nature and to determine accurately their masses. We report on recent results of this ongoing RV campaign, including the recent characterization of the planetary system Kepler-101.
Original languageEnglish
Pages6011
Publication statusPublished - 1 Sep 2015

Fingerprint Dive into the research topics of 'Characterization of small planets with Kepler and HARPS-N'. Together they form a unique fingerprint.

Cite this