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Jones, N. Espinoza, N. M. Law, O. Turner, P. Sarkis, P. Tenenbaum, R. Brahm, S. Seager, S. Udry, S. Wang, T. Henning, T. Henry, V. Suc","submitted_at":"2018-11-13T20:11:41Z","abstract_excerpt":"We report on the confirmation of a transiting giant planet around the relatively hot (Teff = 6801 $\\pm$ 56 K) star HD2685, whose transit signal was detected in Sector 1 data of the TESS mission. We confirmed the planetary nature of the transit signal by using Doppler velocimetric measurements with CHIRON, CORALIE and FEROS, as well as photometric data with CHAT and LCOGT. From the photometry and radial velocities joint analysis, we derived the following parameters for HD2685 $b$: $P$=4.12692$\\pm$0.00004 days, M$_P$=1.18 $\\pm$ 0.09 $M_J$ and $R_P$=1.44 $\\pm$ 0.01 $R_J$. 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Jordan, A. Shporer, A. Tokovinin, A. Vanderburg, A. W. Mann, B. Cruz, C. Ziegler, D. Bayliss, D. Osip, D. Segransan, D. W. Latham, E. Sedaghati, F. Bouchy, F. Pepe, G. Bakos, G. Furesz, G. Laughlin, H. Relles, J. C. Smith, J. Dittmann, J. Doty, J. Hodari-Sadiki, J. L. Christiansen, J. M. Jenkins, J. N. Winn, K. A. Collins, K. Haworth, L. A. Paredes, L. D. Nielsen, M. Davies, M. I. Jones, N. Espinoza, N. M. Law, O. Turner, P. Sarkis, P. Tenenbaum, R. Brahm, S. Seager, S. Udry, S. Wang, T. Henning, T. Henry, V. Suc","submitted_at":"2018-11-13T20:11:41Z","abstract_excerpt":"We report on the confirmation of a transiting giant planet around the relatively hot (Teff = 6801 $\\pm$ 56 K) star HD2685, whose transit signal was detected in Sector 1 data of the TESS mission. We confirmed the planetary nature of the transit signal by using Doppler velocimetric measurements with CHIRON, CORALIE and FEROS, as well as photometric data with CHAT and LCOGT. 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