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Proceedings Paper

An infrared integral field spectrograph specialized for speckle suppression and the direct detection of extrasolar planets
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Paper Abstract

Quasi-static speckles are the main source of noise preventing the direct detection of exoplanets around bright stars. We are investigating the use of an infrared (1.5-2.4 μm) integral field spectrograph (IFS) specialised for speckle suppression and the detection of self-luminous giant planets. This paper presents the optical design and laboratory results obtained with a TIGER-type IFS prototype based on a microlens array. A similar IFS will be used for the Gemini Planet Imager (GPI). Preliminary speckle-suppression performances of the IFS along with simulations are presented.

Paper Details

Date Published: 29 June 2006
PDF: 11 pages
Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 62693X (29 June 2006); doi: 10.1117/12.671578
Show Author Affiliations
Jean-François Lavigne, Univ. de Montréal (Canada)
Institut National d'Optique (Canada)
Herzberg Insitute of Astrophysics (Canada)
René Doyon, Univ. de Montréal (Canada)
Simon Thibault, Univ. Laval (Canada)
Immervision (Canada)
David Lafrenière, Univ. de Montréal (Canada)


Published in SPIE Proceedings Vol. 6269:
Ground-based and Airborne Instrumentation for Astronomy
Ian S. McLean; Masanori Iye, Editor(s)

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