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SPIRou is a near-infrared (nIR) spectropolarimeter / velocimeter for the Canada-France-Hawaii Telescope (CFHT), that will focus on two forefront science topics, (i) the quest for habitable Earth-like planets around nearby M stars, and (ii)…

SPIRou is a near-infrared spectropolarimeter and high-precision radial-velocity instrument, to be mounted on the 3.6m Canada-France-Hawaii telescope ontop Maunakea and to be offered to the CFHT community from 2018. It focuses on two main…

天体物理仪器与方法 · 物理学 2015-10-07 C. Moutou , I. Boisse , G. Hebrard , E. Hebrard , J. -F. Donati , X. Delfosse , D. Kouach

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…

SPIRou, a near infrared spectropolarimeter, is a project of new instrument to be mounted at the Canada France Hawaii Telescope in 2017. One of the main objectives of SPIRou is to reach a radial velocity accuracy better than 1 m/s in the…

SPIRou is a near-infrared (nIR) spectropolarimeter / velocimeter proposed as a new-generation instrument for CFHT. SPIRou aims in particular at becoming world-leader on two forefront science topics, (i) the quest for habitable Earth-like…

SPIRou is a near-infrared (nIR) spectropolarimeter at the CFHT, covering the YJHK nIR spectral bands ($980-2350\,\mathrm{nm}$). We describe the development and current status of the SPIRou wavelength calibration in order to obtain precise…

天体物理仪器与方法 · 物理学 2021-04-14 M. J. Hobson , F. Bouchy , N. J. Cook , E. Artigau , C. Moutou , I. Boisse , C. Lovis , A. Carmona , X. Delfosse , J. -F. Donati , the SPIRou Team

The field of exoplanet research is moving towards the detection and characterization of habitable planets. These exo-Earths can be easily found around low-mass stars by using either photometric transit or radial-velocity (RV) techniques. In…

天体物理仪器与方法 · 物理学 2017-02-22 Federica Cersullo , François Wildi , Bruno Chazelas , Francesco Pepe

The SPIRou near infrared spectro-polarimeter is destined to begin science operations at the Canada-France-Hawaii Telescope in mid-2018. One of the instrument's primary science goals is to discover the closest exoplanets to the Solar System…

With the maturation of near-infrared high-resolution spectroscopy, especially when used for precision radial velocity, data reduction has faced unprecedented challenges in terms of how one goes from raw data to calibrated, extracted, and…

The search for exoplanets around nearby M dwarfs represents a crucial milestone in the census of planetary systems in the vicinity of our Solar System. Since 2018 our team is carrying a radial-velocity blind search program for planets…

SPIRou is the newest spectropolarimeter and high-precision velocimeter that has recently been installed at the Canada-France-Hawaii Telescope on Maunakea, Hawaii. It operates in the near-infrared and simultaneously covers the 0.98-2.35…

SPICA is a mid to far infra-red space mission to explore the processes that form galaxies, stars and planets. SPICA/SAFARI is the far infrared spectrometer that provides near-background limited observations between 34 and 230 micrometers.…

天体物理仪器与方法 · 物理学 2021-01-13 Russell F. Shipman , Bart Vandenbussche , Edgar Castillo-Dominguez , Alvaro Labiano , Willem Jellema , Angiola Orlando

Present and future high-precision radial-velocity spectrometers dedicated to the discovery of low-mass planets orbiting low-mass dwarfs need to focus on the best selected stars to make an efficient use of telescope time. In the framework of…

We present the results of a study aiming at retrieving the fundamental parameters of M dwarfs from spectra secured with SPIRou, the near-infrared high-resolution spectropolarimeter installed at the Canada-France-Hawaii Telescope (CFHT), in…

SPIRou is a near-infrared spectropolarimeter and a high-precision velocimeter. The SPIRou Legacy Survey collected data from February 2019 to June 2022, half of the time devoted to a blind search for exoplanets around nearby cool stars. The…

The Near-InfraRed Planet Searcher or NIRPS is a precision radial velocity spectrograph developed through collaborative efforts among laboratories in Switzerland, Canada, Brazil, France, Portugal and Spain. NIRPS extends to the 0.98-1.8…

天体物理仪器与方法 · 物理学 2024-06-14 Étienne Artigau , François Bouchy , René Doyon , Frédérique Baron , Lison Malo , François Wildi , Franceso Pepe , Neil J. Cook , Simon Thibault , Vladimir Reshetov , Xavier Dumusque , Christophe Lovis , Danuta Sosnowska , Bruno L. Canto Martins , Jose Renan De Medeiros , Xavier Delfosse , Nuno Santos , Rafael Rebolo , Manuel Abreu , Guillaume Allain , Romain Allart , Hugues Auger , Susana Barros , Luc Bazinet , Nicolas Blind , Isabelle Boisse , Xavier Bonfils , Vincent Bourrier , Sébastien Bovay , Christopher Broeg , Denis Brousseau , Vincent Bruniquel , Alexandre Cabral , Charles Cadieux , Andres Carmona , Yann Carteret , Zalpha Challita , Bruno Chazelas , Ryan Cloutier , João Coelho , Marion Cointepas , Uriel Conod , Nicolas Cowan , Eduardo Cristo , João Gomes da Silva , Laurie Dauplaise , Roseane de Lima Gomes , Elisa Delgado-Mena , David Ehrenreich , João Faria , Pedro Figueira , Thierry Forveille , Yolanda Frensch , Jonathan Gagné , Frédéric Genest , Ludovic Genolet , Jonay I. González Hernández , Félix Gracia Témich , Nolan Grieves , Olivier Hernandez , Melissa J. Hobson , Jens Hoeijmakers , Dan Kerley , Vigneshwaran Krishnamurthy , David Lafrenière , Pierrot Lamontagne , Pierre Larue , Henry Leaf , Izan C. Leão , Olivia Lim , Gaspare Lo Curto , Allan M. Martins , Claudio Melo , Yuri S. Messias , Lucile Mignon , Leslie Moranta , Christoph Mordasini , Khaled Al Moulla , Dany Mounzer , Alexandrine L'Heureux , Nicola Nari , Louise Nielsen , Ares Osborn , Léna Parc , Luca Pasquini , Vera M. Passegger , Stefan Pelletier , Céline Peroux , Caroline Piaulet , Mykhaylo Plotnykov , Anne-Sophie Poulin-Girard , José Luis Rasilla , Jonathan Saint-Antoine , Mirsad Sarajlic , Alex Segovia , Julia Seidel , Damien Ségransan , Ana Rita Costa Silva , Avidaan Srivastava , Atanas K. Stefanov , Alejandro Suárez Mascareño , Michael Sordet , Márcio A. Teixeira , Stéphane Udry , Diana Valencia , Philippe Vallée , Thomas Vandal , Valentina Vaulato , Gregg Wade , Joost P. Wardenier , Bachar Wehbé , Drew Weisserman , Ivan Wevers , Gérard Zins

Context: Advancements in the field of exoplanetary research have extended radial velocity (RV) observations from the optical to the near-infrared (nIR) domain. M dwarf stars, characterized by their lower masses and higher prevalence of…

We describe advances on a method designed to derive accurate parameters of M dwarfs. Our analysis consists in comparing high-resolution infrared spectra acquired with the near-infrared spectro-polarimeter SPIRou to synthetic spectra…

太阳与恒星天体物理 · 物理学 2022-09-28 P. I. Cristofari , J. -F. Donati , T. Masseron , P. Fouqué , C. Moutou , A. Carmona , E. Artigau , E. Martioli , G. Hébrard , E. Gaidos , X. Delfosse

M dwarfs are prime targets in the search for exoplanets because of their prevalence and because low-mass planets can be better detected with radial velocity (RV) methods. In particular, the near-infrared (NIR) spectral domain offers an…

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