Year: 2024
Type: article
Abstract: 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.
Authors: K. Rice, A. Mortier, L. Malavolta, F. Pepe, A. Cameron, A. Ghedina, D. Latham, S. Udry, L. Affer, S. Aigrain, A. S. Bonomo, V. Bourrier, L. A. Buchhave, H. Cegla, P. Cortes-Zuleta, R. Cosentino, M. Cretignier, M. Damasso, X. Dumusque, D. Ehrenreich, A. A. John, B. Klein, A. Leleu, M. Lopez-Morales, C. Lovis, J. Maldonado, A. Martínez Fiorenzano, G. Micela, E. Molinari, B. Nicholson, N. O’Sullivan, M. Pinamonti, G. Piotto, D. Sasselov, A. M. Silva, A. Sozzetti, M. Stalport, A. Vanderburg, S. Vissapragada, C. Watson, T. Wilson
Institutions: University of Edinburgh, University of Birmingham, University of Padua, National Institute for Astrophysics, University of Geneva, University of St Andrews, Smithsonian Institution, Center for Astrophysics Harvard & Smithsonian, University of Oxford, Technical University of Denmark, University of Warwick, University of Southern Queensland, Centro de Astrofísica da Universidade do Porto, University of Liège, Massachusetts Institute of Technology, Queen's University Belfast
Language: English
Subfield: Astronomy and Astrophysics
Field: Physics and Astronomy
Domain: Physical Sciences
Open Access status: hybrid
Estimated APC paid: $3,450
OpenAlex ID: W7119470530
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