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R. Ricker, H. Parviainen, I. Ribas, J. A. Caballero, J. C. Morales, J. de Leon, J. D. Twicken, J. L. Bean, J. M. Jenkins, J. N. Winn, J. Sanz-Forcada, J. St\\\"urmer, K. A. Collins, K. I. Collins, K. Molaverdikhani, M. Azzaro, M. Cort\\'es-Contreras, M. Fausnaugh, M. K\\\"urster, M. Lafarga, M. Oshagh, M. Stangret, M. Zechmeister, N. Casasayas-Barris, N. Espinoza, N. Narita, P. Bluhm, P. J. Amado, P. Tenenbaum, R. Luque, R. P. Schwarz, R. Vanderspek, S. Dreizler, S. N. Quinn, S. Seager, S. Stock, S. V. Jeffers, T. Barclay, T. G. Tan, Th. Henning, T. Trifonov, V. J. S. B\\'ejar, V. M. Passegger","submitted_at":"2021-03-08T18:12:41Z","abstract_excerpt":"Spectroscopy of transiting exoplanets can be used to investigate their atmospheric properties and habitability. Combining radial velocity (RV) and transit data provides additional information on exoplanet physical properties. 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