tokens: This work made use of pyke (Still Barclay 2012 ), a software package for the reduction and analysis of Kepler data. This open source software project is developed and distributed by the NASA Kepler Guest Observer Office. Part of this work is based on observations obtained with the HERMES spectrograph, which is supported by the Fund for Scientific Research of Flanders (FWO), Belgium, the Research Council of K.U. Leuven, Belgium, the Fonds National de la Recherche Scientifique (F.R.S.-FNRS), Belgium, the Royal Observatory of Belgium, the Observatoire de Genée, Switzerland, and the TLS, Germany. Calculations have been carried out in Wrocław Centre for Networking and Supercomputing ( http://www.wcss.pl ), grant no. 214. EN acknowledges support from the NCN grant no. 2014/13/B/ST9/00902. SJM acknowledges research support by the Australian Research Council. Funding for the Stellar Astrophysics Centre is provided by the Danish National Research Foundation (grant agreement no.: DNRF106). The research is supported by the ASTERISK project (ASTERoseismic Investigations with SONG and Kepler) funded by the European Research Council (grant agreement no.: 267864). MSC is supported by FCT through research grant UID/FIS/04434/2013 and through the Investigador FCT contract of reference IF/00894/2012 and POPH/FSE (EC) by FEDER funding through the programme COMPETE. Funds for this work were provided also by the EC, under FP7, through the project FP7-SPACE-2012-31284. LAB wishes to thank the National Research Foundation of South Africa for financial support. MB is F.R.S.-FNRS Postdoctoral Researcher, Belgium. AOT acknowledges support from Sonderforschungsbereich SFB 881 ‘The Milky Way System’ (subprojects A4 and A5) of the German Research Foundation (DFG).
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