Produção Nacional
SPIRou: the near-infrared spectropolarimeter/high-precision velocimeter for the Canada-France-Hawaii telescope
2014; SPIE; Linguagem: Inglês
10.1117/12.2055663
ISSN1996-756X
AutoresÉtienne Artigau, Driss Kouach, J.‐F. Donati, René Doyon, X. Delfosse, Sébastien Baratchart, Marielle Lacombe, C. Moutou, Patrick Rabou, L. Parès, Yoan Micheau, Simon Thibault, В. А. Решетов, Bruno Dubois, O. Hernandez, Philippe Vallée, Shiang‐Yu Wang, F. Dolon, F. Pepe, F. Bouchy, Nicolas Striebig, François Hénault, David Loop, Leslie Saddlemyer, Gregory Barrick, Tom Vermeulen, M. Dupieux, Guillaume Hébrard, I. Boisse, Eder Martioli, S. H. P. Alencar, J.-D. Do Nascimento, P. Figueira,
Tópico(s)Astronomy and Astrophysical Research
ResumoSPIRou is a near-IR \'echelle spectropolarimeter and high-precision velocimeter under construction as a next-generation instrument for the Canada-France-Hawaii-Telescope. It is designed to cover a very wide simultaneous near-IR spectral range (0.98-2.35 {\mu}m) at a resolving power of 73.5K, providing unpolarized and polarized spectra of low-mass stars at a radial velocity (RV) precision of 1m/s. The main science goals of SPIRou are the detection of habitable super-Earths around low-mass stars and the study of how critically magnetic fields impact star / planet formation. Following a successful final design review in Spring 2014, SPIRou is now under construction and is scheduled to see first light in late 2017. We present an overview of key aspects of SPIRou's optical and mechanical design.
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