Journal article
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.
- Publication status:
- Published
- Peer review status:
- Peer reviewed
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(Preview, Version of record, pdf, 250.8KB, Terms of use)
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- Publisher copy:
- 10.1017/s1743921324001741
Authors
- Publisher:
- Cambridge University Press
- Journal:
- Proceedings of the International Astronomical Union More from this journal
- Volume:
- 20
- Issue:
- S393
- Pages:
- 150-155
- Publication date:
- 2026-01-09
- DOI:
- EISSN:
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1743-9221
- ISSN:
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1743-9213
- Language:
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English
- Keywords:
- Pubs id:
-
2361227
- Local pid:
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pubs:2361227
- Source identifiers:
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3646756
- Deposit date:
-
2026-01-09
- ARK identifier:
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Terms of use
- Copyright date:
- 2026
- Licence:
- CC Attribution (CC BY)
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