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Stable deep nulling in polychromatic unpolarized light with multiaxial beam combination
Christophe Buisset1, Xavier Rejeaunier, Yves Rabbia
1Département Gemini, Observatoire de la Côte d'Azur, UMR CNRS 6203, Avenue Copernic, 06130 Grasse, France. christophe.buisset@obs-azur.fr
Applied Optics
|November 13, 2007
Summary
The multiaperture imaging interferometer (MAII) breadboard demonstrated deep and stable nulling for the European Space Agency's (ESA) Darwin mission. Multiaxial beam combination achieved excellent nulling ratios, meeting Darwin requirements.
Area of Science:
- * Astronomy and astrophysics
- * Optical interferometry
- * Space-based observatories
Background:
- * The European Space Agency (ESA) Darwin mission aims for space-based nulling. Thales Alenia Space developed the multiaperture imaging interferometer (MAII) breadboard for ESA to demonstrate deep and stable nulling.
- * Investigations extended to multiaxial beam combination, offering simplicity, compactness, and high coupling efficiency for three-beam combinations.
Purpose of the Study:
- * To demonstrate deep and stable nulling using the MAII breadboard.
- * To investigate subsystems of the ESA Darwin interferometer.
- * To evaluate the multiaxial beam combination scheme for space-based nulling.
Main Methods:
- * Upgraded the near-infrared (λ ≈ 1.55 μm) MAII breadboard to a multiaxial beam combination configuration.
- * Investigated polarization and stability issues within the multiaxial setup.
- * Conducted experiments with unpolarized light and a relative spectral bandwidth of 5%.
Main Results:
- * Achieved mean nulling ratios (N) of 1.7 x 10⁻⁵.
- * Demonstrated stability of nulling over 1 hour with a standard deviation (σ(N)) of 5.7 x 10⁻⁷.
- * Validated performance in unpolarized light with a 5% relative spectral bandwidth.
Conclusions:
- * The multiaxial beam combination is a promising technique for space-based nulling.
- * The MAII breadboard's performance meets the stringent requirements of the ESA Darwin mission.
- * This approach offers a viable path for future high-contrast imaging missions.

