tokens: We are infinitely grateful to the staff members at the Nordic Optical Telescope for their valuable and unique support during the observations. We thank the editor and the anonymous referee for their careful review and very positive feedback. Davide Gandolfi thanks Gabriele Cologna for the interesting conversations on the properties of the planetary system. Hannu Parviainen has received support from the Rocky Planets Around Cool Stars (RoPACS) project during this research, a Marie Curie Initial Training Network funded by the European Commission’s Seventh Framework Programme. He has also received funding from the Väisälä Foundation through the Finnish Academy of Science and Letters and from the Leverhulme Research Project grant RPG-2012-661. Financial supports from the Spanish Ministry of Economy and Competitiveness (MINECO) are acknowledged by Hans J. Deeg for the grant AYA2012-39346-C02-02, by Sergio Hoyer for the 2011 Severo Ochoa program SEV-2011-0187, and Roi Alonso for the Ramón y Cajal program RYC-2010-06519. This paper includes data collected by the Kepler mission. Funding for the Kepler mission is provided by the NASA Science Mission Directorate. The Kepler data presented in this paper were obtained from the Mikulski Archive for Space Telescopes (MAST). STScI is operated by the Association of Universities for Research in Astronomy, Inc., under NASA contract NAS5-26555. Support for MAST for non-HST data is provided by the NASA Office of Space Science via grant NNX13AC07G and by other grants and contracts. This research has made an intensive use of the Simbad database and the VizieR catalogue access tool, CDS, Strasbourg, France. The original description of the VizieR service was published in AAS, 143, 23.
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