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Bruni, I. Carleo, I. Pagano, J. Maldonado, J. Southworth, K. Biazzo, L. Affer, L. Malavolta, L. Mancini, M. Brogi, M. Damasso, M. Esposito, M. Pedani, M. Rainer, P. Giacobbe, P. Sarkis, R. Claudi, R. Cosentino, R. Gratton, R. Smareglia, S. Benatti, S. Ciceri, S. Desidera, S. Masiero, Th. Henning, V. Nascimbeni","submitted_at":"2018-02-12T01:38:21Z","abstract_excerpt":"We characterised five transiting planetary systems (HAT-P-3, HAT-P-12, HAT-P-22, WASP-39 and WASP-60) and determined their sky-projected planet orbital obliquity through the measurement of the RM effect. We used HARPS-N high-precision radial velocity measurements, gathered during transit events, to measure the RM effect in the target systems and determine the sky-projected angle between the planetary orbital plane and the stellar equator. 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