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Data processing in nulling interferometry: case of the Darwin mission

Published online by Cambridge University Press:  13 October 2006

M. Carbillet ,
A. Ferrari ,
C. Aime ,
L. Mugnier ,
E. Thiébaut  and
A. Belu
L. Mugnier
Affiliation:
ONERA, Département d'Optique Théorique et Appliquée, BP. 72, 92322 Châtillon Cedex, France
E. Thiébaut
Affiliation:
CRAL, URA 300, 9 Av. Charles André, 69561 Saint Genis Laval Cedex, France
A. Belu
Affiliation:
Laboratoire Universitaire d'Astrophysique de Nice, Parc Valrose, 06100 Nice, France
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Abstract

This paper first gives an introduction to the broad features of the Darwin mission of ESA and then describes in some detail the data processing that is necessary to detect planets and spectrally characterize them. The proposed data processing method is validated by means of simulated data.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 22: Astronomy with High Contrast Imaging III: Instrumental Techniques, Modeling and Data Processing , 2006 , pp. 69 - 83
Copyright
© EAS, EDP Sciences, 2006

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