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We thank all the staff at the observatories involved in this study for their support. This work was based on observations at the following observatories: ESO, Chile (PIDs 271.C-5023 and 073.C-0137, Ondrejov Observatory, Czech Republic (grant A3003204, Centro Astronómico Hispano Atemán (Calar Alto, Spain, Liverpool Telescope, La Palma (Canary Islands, Spain, Isaac Newton Group, La Patma; and Faulkes Telescope North (Maui, Hawaii, We also thank the referees for their helpful reviews. Supported by the Leverhulme Trust (S.C.L, the UK Particle Physics and Astronomy Research Council (A.F, the Grant Agency of the Czech Republic (P.P. and D.V, NASA grant NNG04GN31G (P.A.T. and J.-L.M, and Slovak Grant Agency for Science VEGA grant 1/3074/06 A.G, This work made use of the NASA/JPL HORIZONS ephemeris-generating program
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We thank all the staff at the observatories involved in this study for their support. This work was based on observations at the following observatories: ESO, Chile (PIDs 271.C-5023 and 073.C-0137); Ondrejov Observatory, Czech Republic (grant A3003204); Centro Astronómico Hispano Atemán (Calar Alto, Spain); Liverpool Telescope, La Palma (Canary Islands, Spain); Isaac Newton Group, La Patma; and Faulkes Telescope North (Maui, Hawaii). We also thank the referees for their helpful reviews. Supported by the Leverhulme Trust (S.C.L.), the UK Particle Physics and Astronomy Research Council (A.F.), the Grant Agency of the Czech Republic (P.P. and D.V.), NASA grant NNG04GN31G (P.A.T. and J.-L.M.), and Slovak Grant Agency for Science VEGA grant 1/3074/06 (A.G.). This work made use of the NASA/JPL HORIZONS ephemeris-generating program.
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