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

doi:10.1017/S1743921324001741

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: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

8 Downloads (Orbit)

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
Title of host publication	Proceedings of the International Astronomical Union
Editors	Z. Benkhaldoun, Y. Moulane, A. Szentgyorgyi
Volume	20
Publisher	Cambridge University Press
Publication date	2026
Edition	S393
Pages	150-155
DOIs	https://doi.org/10.1017/S1743921324001741
Publication status	Published - 2026
Event	IAUS 393: Planetary Science and Exoplanets in the Era of James Webb Space Telescope - Cape Town, South Africa Duration: 6 Aug 2024 → 15 Aug 2024

Conference

Conference	IAUS 393
Country/Territory	South Africa
City	Cape Town
Period	06/08/2024 → 15/08/2024

Series	Proceedings of the International Astronomical Union
ISSN	1743-9213

Keywords

Exoplanet characterisation
Exoplanets
Radial velocities
Transits

Access to Document

10.1017/S1743921324001741Licence: CC BY

FulltextFinal published version, 281 KBLicence: CC BY

OpenUrl availability

Full text

Cite this

Rice, K., Mortier, A., Malavolta, L., Pepe, F., Cameron, A., Ghedina, A., Latham, D., Udry, S., Affer, L., Aigrain, S., Bonomo, A. S., Bourrier, V., Buchhave, L. A., Cegla, H., Cortes-Zuleta, P., Cosentino, R., Cretignier, M., Damasso, M., Dumusque, X., ... Wilson, T. (2026). Detecting and characterising exoplanets with HARPS-N. In Z. Benkhaldoun, Y. Moulane, & A. Szentgyorgyi (Eds.), Proceedings of the International Astronomical Union (S393 ed., Vol. 20, pp. 150-155). Cambridge University Press. https://doi.org/10.1017/S1743921324001741

@inproceedings{f67a43eafbfb4c458538ecd4df928aa2,

title = "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.",

keywords = "Exoplanet characterisation, Exoplanets, Radial velocities, Transits",

author = "K. Rice and A. Mortier and L. Malavolta and F. Pepe and A. Cameron and A. Ghedina and D. Latham and S. Udry and L. Affer and S. Aigrain and Bonomo, \{A. S.\} and V. Bourrier and Buchhave, \{L. A.\} and H. Cegla and P. Cortes-Zuleta and R. Cosentino and M. Cretignier and M. Damasso and X. Dumusque and D. Ehrenreich and John, \{A. A.\} and B. Klein and A. Leleu and M. Lopez-Morales and C. Lovis and J. Maldonado and \{Mart{\'i}nez Fiorenzano\}, A. and G. Micela and E. Molinari and B. Nicholson and N. O'Sullivan and M. Pinamonti and G. Piotto and D. Sasselov and Silva, \{A. M.\} and A. Sozzetti and M. Stalport and A. Vanderburg and S. Vissapragada and C. Watson and T. Wilson",

note = "Publisher Copyright: {\textcopyright} The Author(s), 2026. Published by Cambridge University Press on behalf of International Astronomical Union.; IAUS 393 : Planetary Science and Exoplanets in the Era of James Webb Space Telescope ; Conference date: 06-08-2024 Through 15-08-2024",

year = "2026",

doi = "10.1017/S1743921324001741",

language = "English",

volume = "20",

series = "Proceedings of the International Astronomical Union",

publisher = "Cambridge University Press",

pages = "150--155",

editor = "Benkhaldoun, \{Z. \} and Y. Moulane and Szentgyorgyi, \{A. \}",

booktitle = "Proceedings of the International Astronomical Union",

address = "United Kingdom",

edition = "S393",

}

Rice, K, Mortier, A, Malavolta, L, Pepe, F, Cameron, A, Ghedina, A, Latham, D, Udry, S, Affer, L, Aigrain, S, Bonomo, AS, Bourrier, V, Buchhave, LA, Cegla, H, Cortes-Zuleta, P, Cosentino, R, Cretignier, M, Damasso, M, Dumusque, X, Ehrenreich, D, John, AA, Klein, B, Leleu, A, Lopez-Morales, M, Lovis, C, Maldonado, J, Martínez Fiorenzano, A, Micela, G, Molinari, E, Nicholson, B, O'Sullivan, N, Pinamonti, M, Piotto, G, Sasselov, D, Silva, AM, Sozzetti, A, Stalport, M, Vanderburg, A, Vissapragada, S, Watson, C & Wilson, T 2026, Detecting and characterising exoplanets with HARPS-N. in Z Benkhaldoun, Y Moulane & A Szentgyorgyi (eds), Proceedings of the International Astronomical Union. S393 edn, vol. 20, Cambridge University Press, Proceedings of the International Astronomical Union, pp. 150-155, IAUS 393, Cape Town, South Africa, 06/08/2024. https://doi.org/10.1017/S1743921324001741

Detecting and characterising exoplanets with HARPS-N. / Rice, K.; Mortier, A.; Malavolta, L. et al.
Proceedings of the International Astronomical Union. ed. / Z. Benkhaldoun; Y. Moulane; A. Szentgyorgyi. Vol. 20 S393. ed. Cambridge University Press, 2026. p. 150-155 (Proceedings of the International Astronomical Union).

Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

TY - GEN

T1 - Detecting and characterising exoplanets with HARPS-N

AU - Rice, K.

AU - Mortier, A.

AU - Malavolta, L.

AU - Pepe, F.

AU - Cameron, A.

AU - Ghedina, A.

AU - Latham, D.

AU - Udry, S.

AU - Affer, L.

AU - Aigrain, S.

AU - Bonomo, A. S.

AU - Bourrier, V.

AU - Buchhave, L. A.

AU - Cegla, H.

AU - Cortes-Zuleta, P.

AU - Cosentino, R.

AU - Cretignier, M.

AU - Damasso, M.

AU - Dumusque, X.

AU - Ehrenreich, D.

AU - John, A. A.

AU - Klein, B.

AU - Leleu, A.

AU - Lopez-Morales, M.

AU - Lovis, C.

AU - Maldonado, J.

AU - Martínez Fiorenzano, A.

AU - Micela, G.

AU - Molinari, E.

AU - Nicholson, B.

AU - O'Sullivan, N.

AU - Pinamonti, M.

AU - Piotto, G.

AU - Sasselov, D.

AU - Silva, A. M.

AU - Sozzetti, A.

AU - Stalport, M.

AU - Vanderburg, A.

AU - Vissapragada, S.

AU - Watson, C.

AU - Wilson, T.

PY - 2026

Y1 - 2026

N2 - 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.

AB - 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.

KW - Exoplanet characterisation

KW - Exoplanets

KW - Radial velocities

KW - Transits

U2 - 10.1017/S1743921324001741

DO - 10.1017/S1743921324001741

M3 - Article in proceedings

AN - SCOPUS:105027765874

VL - 20

T3 - Proceedings of the International Astronomical Union

SP - 150

EP - 155

BT - Proceedings of the International Astronomical Union

A2 - Benkhaldoun, Z.

A2 - Moulane, Y.

A2 - Szentgyorgyi, A.

PB - Cambridge University Press

T2 - IAUS 393

Y2 - 6 August 2024 through 15 August 2024

ER -

Rice K, Mortier A, Malavolta L, Pepe F, Cameron A, Ghedina A et al. Detecting and characterising exoplanets with HARPS-N. In Benkhaldoun Z, Moulane Y, Szentgyorgyi A, editors, Proceedings of the International Astronomical Union. S393 ed. Vol. 20. Cambridge University Press. 2026. p. 150-155. (Proceedings of the International Astronomical Union). doi: 10.1017/S1743921324001741

Detecting and characterising exoplanets with HARPS-N

Abstract

Conference

Keywords

Access to Document

OpenUrl availability

Fingerprint

Cite this