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Issue EAS Publications Series
Volume 22, 2006
Astronomy with High Contrast Imaging III: Instrumental Techniques, Modeling and Data Processing
Page(s) 213 - 221
DOI 10.1051/eas:2006134
Published online 13 October 2006

Astronomy with High Contrast Imaging III: Instrumental Techniques, Modeling and Data Processing
M. Carbillet, A. Ferrari and C. Aime (eds)
EAS Publications Series, 22 (2006) 213-221

DOI: 10.1051/eas:2006134

Earth-like planet detection with Extremely Large Telescopes

C. Cavarroc1, A. Boccaletti1, P. Baudoz1, T. Fusco2 and D. Rouan1

1  Observatoire de Paris-Meudon, France
2  ONERA, France


(Published online 13 October 2006)

Abstract
Direct detection of Earth-like planets is one of the major objectives for the next generation of ground based telescopes (Extremely Large Telescopes, ELT). ELT instruments will be conditionned by such scientific programs. Here, we consider here a system made with an adaptive optics device, a coronagraph and a simultaneous calibration system. We refined this simple model by including static aberrations upstream the coronagraph and differential aberrations downstream. Using numerical simulations, we evaluate how these static aberrations limit the detectability of telluric planets.



© EAS, EDP Sciences 2006


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