Paper
29 June 2006 An infrared integral field spectrograph specialized for speckle suppression and the direct detection of extrasolar planets
Author Affiliations +
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.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Jean-François Lavigne, René Doyon, Simon Thibault, and David Lafrenière "An infrared integral field spectrograph specialized for speckle suppression and the direct detection of extrasolar planets", Proc. SPIE 6269, Ground-based and Airborne Instrumentation for Astronomy, 62693X (29 June 2006); https://doi.org/10.1117/12.671578
Lens.org Logo
CITATIONS
Cited by 4 scholarly publications.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Point spread functions

Iterated function systems

Speckle

Sensors

Signal attenuation

Contamination

Planets

Back to Top