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 language | English |
|---|---|
| Pages (from-to) | 150-155 |
| Number of pages | 6 |
| Journal | Proceedings of the International Astronomical Union |
| Volume | 20 |
| Issue number | S393 |
| Early online date | 31 Dec 2024 |
| DOIs | |
| Publication status | Published - 9 Jan 2026 |
| Event | 393rd Symposium of the International Astronomical Union on Planetary Science and Exoplanets in the Era of JWST - Cape Town, South Africa Duration: 13 Aug 2024 → 15 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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