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SPIRou: nIR velocimetry & spectropolarimetry at the CFHT

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arxiv 2008.08949 v1 pith:2ZXGRHOM submitted 2020-08-20 astro-ph.IM astro-ph.EPastro-ph.SR

SPIRou: nIR velocimetry & spectropolarimetry at the CFHT

classification astro-ph.IM astro-ph.EPastro-ph.SR
keywords spiroucfhtsciencedwarfsatmospheresgoalsinstrumentlike
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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This paper presents an overview of SPIRou, the new-generation near-infrared spectropolarimeter / precision velocimeter recently installed on the 3.6-m Canada-France-Hawaii Telescope (CFHT). Starting from the two main science goals, namely the quest for planetary systems around nearby M dwarfs and the study of magnetized star / planet formation, we outline the instrument concept that was designed to efficiently address these forefront topics, and detail the in-lab and on-sky instrument performances measured throughout the intensive testing phase that SPIRou was submitted to before passing the final acceptance review in early 2019 and initiating science observations. With a central position among the newly started programmes, the SPIRou Legacy Survey (SLS) Large Programme was allocated 300 CFHT nights until at least mid 2022. We also briefly describe a few of the first results obtained in the various science topics that SPIRou started investigating, focusing in particular on planetary systems of nearby M dwarfs, transiting exoplanets and their atmospheres, magnetic fields of young stars, but also on alternate science goals like the atmospheres of M dwarfs and the Earth's atmosphere. We finally conclude on the essential role that SPIRou and the CFHT can play in coordination with forthcoming major facilities like the JWST, the ELTs, PLATO and ARIEL over the decade.

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Cited by 2 Pith papers

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  1. Uniform Metallicity Measurements of M Dwarf Planet Hosts Support Metallicity-Dependent Sub-Neptune Formation

    astro-ph.EP 2026-07 conditional novelty 6.0

    Homogeneous SpeX metallicities of M-dwarf planet hosts show sub-Neptune hosts are more metal-rich than super-Earth hosts, supporting ice-line formation plus migration.

  2. Unstable magnetospheric accretion on the T Tauri star TW Hya

    astro-ph.SR 2026-07 accept novelty 4.5

    TW Hya’s large-scale field is a ~0.83 kG tilted dipole that varies yearly; accretion is unstable (rmag/rcor ≈ 0.33–0.40) and no close-in planet is detected above ~0.3–1 Mjup.