Exoplanet characterisation; Exoplanets; Radial velocities; Transits; Astronomy and Astrophysics; Space and Planetary Science
Abstract :
[en] Exoplanet follow-up with JWST requires precise masses and radii. HARPS-N is a high-resolution spectrograph on the Telescopio Nazionale Galileo (TNG), predominantly used to detect and characterize exoplanets using the radial velocity (RV) method. The HARPS-N Collaboration has been characterising exoplanets with HARPS-N for over a decade. In this short paper we highlight the contributions that the HARPS-N Collaboration has made to the characterisation of small exoplanets.
Research Center/Unit :
STAR - Space sciences, Technologies and Astrophysics Research - ULiège Astrobiology - ULiège
Disciplines :
Space science, astronomy & astrophysics
Author, co-author :
Rice, K. ; University of Edinburgh, United Kingdom
Mortier, A.; University of Birmingham, United Kingdom
Malavolta, L.; Università Degli Studi di Padova, Italy ; INAF, Italy
Pepe, F.; University of Geneva, Switzerland
Cameron, A.; University of St Andrews, United Kingdom
Ghedina, A.; INAF, Italy
Latham, D.; Center for Astrophysics, Harvard & Smithsonian, United States
Udry, S.; INAF, Italy
Affer, L.; INAF, Italy
Aigrain, S.; University of Oxford, United Kingdom
Bonomo, A.S.; INAF, Italy
Bourrier, V.; University of Geneva, Switzerland
Buchhave, L.A.; Technical University of Denmark, Denmark
Cegla, H.; University of Warwick, United Kingdom
Cortes-Zuleta, P.; University of St Andrews, United Kingdom
Cosentino, R.; INAF, Italy
Cretignier, M.; University of Oxford, United Kingdom
Damasso, M.; INAF, Italy
Dumusque, X.; University of Geneva, Switzerland
Ehrenreich, D.; University of Geneva, Switzerland
John, A.A.; University of St Andrews, United Kingdom
Klein, B.; University of Oxford, United Kingdom
Leleu, A.; University of Geneva, Switzerland
Lopez-Morales, M.; Center for Astrophysics, Harvard & Smithsonian, United States
Lovis, C.; University of Geneva, Switzerland
Maldonado, J.; INAF, Italy
Martínez Fiorenzano, A.; INAF, Italy
Micela, G.; INAF, Italy
Molinari, E.; INAF, Italy
Nicholson, B.; University of Southern Queensland, Australia
O'Sullivan, N.; University of Oxford, United Kingdom
Pinamonti, M.; INAF, Italy
Piotto, G.; Università Degli Studi di Padova, Italy ; INAF, Italy
Sasselov, D.; Center for Astrophysics, Harvard & Smithsonian, United States
Silva, A.M.; IA-Porto/CAUP
Sozzetti, A.; INAF, Italy
Stalport, Manu ; Université de Liège - ULiège > Unités de recherche interfacultaires > Space sciences, Technologies and Astrophysics Research (STAR)
Vanderburg, A.; MIT, United States
Vissapragada, S.; Center for Astrophysics, Harvard & Smithsonian, United States
Watson, C.; Queen's University Belfast, United Kingdom
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