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arxiv: 2507.21767 · v1 · pith:Q5CKAI6Cnew · submitted 2025-07-29 · 🌌 astro-ph.IM · astro-ph.EP

NIRPS joining HARPS at ESO 3.6 m. On-sky performance and science objectives

Francois Bouchy , Rene Doyon , Francesco Pepe , Claudio Melo , Etienne Artigau , Lison Malo , Francois Wildi , Frederique Baron
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Xavier Delfosse Jose Renan De Medeiros Rafael Rebolo Nuno C. Santos Gregg Wade Romain Allart Khaled Al Moulla Nicolas Blind Charles Cadieux Bruno L. Canto Martins Neil J. Cook Xavier Dumusque Yolanda Frensch Frederic Genest Jonay I. Gonzalez Hernandez Nolan Grieves Gaspare Lo Curto Christophe Lovis Lucile Mignon Louise D. Nielsen Anne-Sophie Poulin-Girard Jose Luis Rasilla Vladimir Reshetov Danuta Sosnowska Michael Sordet Jonathan Saint-Antoine Alejandro Suarez Mascareno Simon Thibault Philippe Vallee Thomas Vandal Manuel Abreu Jose L. A. Aguiar Guillaume Allain Tomy Arial Hugues Auger Susana C. C. Barros Luc Bazinet Bjorn Benneke Xavier Bonfils Anne Boucher Vincent Bourrier Sebastien Bovay Christopher Broeg Denis Brousseau Vincent Bruniquel Marta Bryan Alexandre Cabral Andres Carmona Yann Carteret Zalpha Challita Bruno Chazelas Ryan Cloutier Joao Coelho Marion Cointepas Uriel Conod Nicolas B. Cowan Eduardo Cristo Joao Gomes da Silva Laurie Dauplaise Antoine Darveau-Bernier Roseane de Lima Gomes Daniel Brito de Freitas Elisa Delgado-Mena Jean-Baptiste Delisle David Ehrenreich Joao Faria Pedro Figueira Dasaev O. Fontinele Thierry Forveille Jonathan Gagne Ludovic Genolet Felix Gracia Temich Olivier Hernandez Melissa J. Hobson Jens Hoeijmakers Norbert Hubin Farbod Jahandar Ray Jayawardhana Hans-Ulrich Kauf Dan Kerley Johann Kolb Vigneshwaran Krishnamurthy David Lafreniere Pierrot Lamontagne Pierre Larue Henry Leath Alexandrine L Heureux Izan de Castro Leao Olivia Lim Allan M. Martins Jaymie Matthews Jean-Sebastien Mayer Yuri S. Messias Stan Metchev Leslie Moranta Christoph Mordasini Dany Mounzer Nicola Nari Ares Osborn Mathieu Ouellet Jon Otegi Lena Parc Luca Pasquini Vera M. Passegger Stefan Pelletier Celine Peroux Caroline Piaulet-Ghorayeb Mykhaylo Plotnykov Emanuela Pompei Jason Rowe Mirsad Sarajlic Alex Segovia Julia Seidel Damien Segransan Robin Schnell Ana Rita Costa Silva Avidaan Srivastava Valentina Vaulato Atanas K. Stefanov Marcio A. Teixeira Stephane Udry Joost P. Wardenier Bachar Wehbe Drew Weisserman Vincent Yariv Gerard Zins
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classification 🌌 astro-ph.IM astro-ph.EP
keywords nirpshighspectralcharacterisationfibreinstrumenton-skyprecision
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The Near-InfraRed Planet Searcher (NIRPS) is a high-resolution, high-stability near-infrared (NIR) spectrograph equipped with an AO system. Installed on the ESO 3.6-m telescope, it was developed to enable radial velocity (RV) measurements of low-mass exoplanets around M dwarfs and to characterise exoplanet atmospheres in the NIR. This paper provides a comprehensive design overview and characterisation of the NIRPS instrument, reporting on its on-sky performance, and presenting its GTO programme. The instrument started its operations on 1 Apr 2023 after intensive on-sky testing phases. The spectral range continuously covers the Y, J, and H bands from 972.4 to 1919.6 nm. The thermal control system maintains 1 mK stability over several months. The NIRPS AO-assisted fibre link improves coupling efficiency and offers a unique high-angular resolution capability with a fibre acceptance of only 0.4 arcsec. A high spectral resolving power of 90 000 and 75 000 is provided in HA and HE modes, respectively. The overall throughput from the top of the atmosphere to the detector peaks at 13 percent. The RV precision, measured on the bright star Proxima with a known exoplanetary system, is 77 cm/s. NIRPS and HARPS can be used simultaneously, offering unprecedented spectral coverage for spectroscopic characterisation and stellar activity mitigation. Modal noise can be aptly mitigated by the implementation of fibre stretchers and AO scanning mode. Initial results confirm that NIRPS opens new possibilities for RV measurements, stellar characterisation, and exoplanet atmosphere studies with high precision and high spectral fidelity. NIRPS demonstrated stable RV precision at the level of 1 m/s over several weeks. The instrument high throughput offers a notable improvement over previous spectrographs, enhancing our ability to detect small exoplanets.

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