A&A 503, 601–612 (2009) Astronomy DOI: 10.1051/0004-6361/200811466 & c ESO 2009 Astrophysics Characterization of the HD 17156 planetary system, M. Barbieri1, R. Alonso1,S.Desidera2, A. Sozzetti3, A. F. Martinez Fiorenzano4,J.M.Almenara5, M. Cecconi4, R. U. Claudi2, D. Charbonneau7 ,M.Endl8, V. Granata2,9, R. Gratton2,G.Laughlin10, B. Loeillet1,6, and Exoplanet Amateur Consortium 1 Laboratoire d’Astrophysique de Marseille, 38 rue Joliot-Curie, 13388 Marseille Cedex 13, France e-mail:
[email protected] 2 INAF Osservatorio Astronomico di Padova, Vicolo dell’ Osservatorio 5, 35122 Padova, Italy 3 INAF Osservatorio Astronomico di Torino, 10025 Pino Torinese, Italy 4 Fundación Galileo Galilei – INAF, Rambla José Ana Fernández Pérez 7, 38712 Breña Baja (TF), Spain 5 Instituto de Astrofísica de Canarias, C/Vía Láctea s/n, 38200 La Laguna, Spain 6 IAP, 98bis Bd Arago, 75014 Paris, France 7 Harvard-Smithsonian Center for Astrophysics, 60 Garden Street, Cambridge, MA 02138, USA 8 McDonald Observatory, The University of Texas at Austin, Austin, TX 78712, USA 9 CISAS, Università di Padova, Italy 10 University of California Observatories, University of California at Santa Cruz Santa Cruz, CA 95064, USA Received 2 December 2008 / Accepted 12 March 2009 ABSTRACT Aims. We present data to improve the known parameters of the HD 17156 system (peculiar due to the eccentricity and long orbital period of its transiting planet) and constrain the presence of stellar companions. Methods. Photometric data were acquired for 4 transits, and high precision radial velocity measurements were simultaneously acquired with the SARG spectrograph at TNG for one transit.