Paper
28 June 2006 Post processing of differential images for direct extrasolar planet detection from the ground
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Abstract
The direct imaging from the ground of extrasolar planets has become today a major astronomical and biological focus. This kind of imaging requires simultaneously the use of a dedicated high performance Adaptive Optics [AO] system and a differential imaging camera in order to cancel out the flux coming from the star. In addition, the use of sophisticated post-processing techniques is mandatory to achieve the ultimate detection performance required. In the framework of the SPHERE project, we present here the development of a new technique, based on Maximum A Posteriori [MAP] approach, able to estimate parameters of a faint companion in the vicinity of a bright star, using the multi-wavelength images, the AO closed-loop data as well as some knowledge on non-common path and differential aberrations. Simulation results show a 10-5 detectivity at 5σ for angular separation around 15λ/D with only two images.
© (2006) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
J.-F. Sauvage, L. Mugnier, T. Fusco, and G. Rousset "Post processing of differential images for direct extrasolar planet detection from the ground", Proc. SPIE 6272, Advances in Adaptive Optics II, 62722B (28 June 2006); https://doi.org/10.1117/12.671470
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Cited by 8 scholarly publications.
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KEYWORDS
Stars

Point spread functions

Adaptive optics

Optical transfer functions

Turbulence

Imaging systems

Image processing

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