Detecting and characterising exoplanets with HARPS-N

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.

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Publication Details

Journal
Proceedings of the International Astronomical Union
Published
2024-12-01
DOI
https://doi.org/10.1017/s1743921324001741
Primary Topic
Stellar, planetary, and galactic studies
Type
article
Field-Weighted Citation Impact
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article

Detecting and characterising exoplanets with HARPS-N

M. Pinamonti, Baptiste Klein, A. Ghedina, Susanne Aigrain et al.
Proceedings of the International Astronomical Union
Stellar, planetary, and galactic studies
article

Detecting and characterising exoplanets with HARPS-N

M. Pinamonti, Baptiste Klein, A. Ghedina, Susanne Aigrain, Andrew Vanderburg, Belinda Nicholson, M. Cretignier, E. Molinari, P. Cortés-Zuleta, H. M. Cegla, Adrien Leleu, T. G. Wilson, G. Micela, A. Cameron, L. Affer, A. Mortier, C. Watson, A. Sozzetti, L. Malavolta, A. M. Silva, G. Piotto, M. Stalport, S. Vissapragada, L. A. Buchhave, J. Maldonado, R. Cosentino, M. Lopez-Morales, K. Rice, A. Martínez Fiorenzano, M. Damasso, F. Pepe, X. Dumusque, C. Lovis, D. Ehrenreich, V. Bourrier, A. A. John, S. Udry, D. Sasselov, D. Latham, N. O’Sullivan, A. S. Bonomo
article en

Abstract

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.

Proceedings of the International Astronomical UnionVol. 20(S393)
University of Geneva (CH), Queen's University Belfast (GB), University of Padua (IT), University of Liège (BE), University of St Andrews (GB), University of Southern Queensland (AU), University of Warwick (GB), University of Oxford (GB), Centro de Astrofísica da Universidade do Porto (PT), Moscow Institute of Thermal Technology (RU), University of Birmingham (GB), National Institute for Astrophysics (IT), Technical University of Denmark (DK), University of Edinburgh (GB)
Openalex Percentile: Top 40%
Stellar, planetary, and galactic studies
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