Detecting and characterising exoplanets with HARPS-N

  • 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
*Corresponding author for this work

Research output: Contribution to journalConference articlepeer-review

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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.

Original languageEnglish
Pages (from-to)150-155
Number of pages6
JournalProceedings of the International Astronomical Union
Volume20
Issue numberS393
Early online date31 Dec 2024
DOIs
Publication statusPublished - 9 Jan 2026
Event393rd Symposium of the International Astronomical Union on Planetary Science and Exoplanets in the Era of JWST - Cape Town, South Africa
Duration: 13 Aug 202415 Aug 2024
Conference number: 393
https://iaus393.uca.ma/

Bibliographical note

Publisher Copyright:
© The Author(s), 2026. Published by Cambridge University Press on behalf of International Astronomical Union.

Keywords

  • Exoplanet characterisation
  • Exoplanets
  • Radial velocities
  • Transits

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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