High-precision high-fidelity spectrographs are the most powerful instruments for exoplanets detection and characterization. The sub-m/s radial-velocity precision, required to detect Earth-mass exoplanets, necessitates tackling all the sources of instrumental and stellar instabilities.
We present the new high-precision high-fidelity spectrographs ESPRESSO, NIRPS, ANDES and RISTRETTO designed, developed, and operated with support of PlanetS.
François Bouchy, Francesco Pepe, Xavier Dumusque, Tobias Schmidt, Christophe Lovis, Stéphane Udry
Comments: Chapter accepted for publication in the NCCR PlanetS Legacy Book: Benz, W. et al. (Eds), The National Center for Competence in Research, PlanetS: A Swiss-wide network expanding planetary sciences. Springer (2026)
Subjects: Instrumentation and Methods for Astrophysics (astro-ph.IM); Earth and Planetary Astrophysics (astro-ph.EP)
Cite as: arXiv:2604.09020 [astro-ph.IM] (or arXiv:2604.09020v1 [astro-ph.IM] for this version)
https://doi.org/10.48550/arXiv.2604.09020
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Submission history
From: Francois Bouchy
[v1] Fri, 10 Apr 2026 06:34:01 UTC (5,012 KB)
https://arxiv.org/abs/2604.09020
Astrobiology, Astronomy,
