International audienceNulling interferometry requires, among other things, a symmetric recombination module and an optical path difference control system. The symmetric recombination stage has been particularly studied over the last ten years and several concepts are now well known. One of them is the "Modified Mach Zehnder" (MMZ) interferometer, proposed by Serabyn and Colavita (2001) [1]. In this paper, we describe a new version of the MMZ beam combiner which provides a deep null signal in the science channel and, at the same time, phase-sensitive signals in the so-called co-phasing channel. From the latter, accurate optical path difference measurements can be derived. This beam combiner works in the 0.8 to 3.3 mum spectral range (0.8 to ...
Deep, stable nulling of starlight requires careful control of the amplitudes and phases of the beams...
The Polarization-Based Collimated Beam Combiner efficiently produces pairwise interference between b...
International audienceContext: Direct detection of a planet around a star and its characterisation f...
International audienceNulling interferometry requires, among other things, a symmetric recombination...
International audienceNulling interferometry requires, among other things, a symmetric recombination...
International audienceNulling interferometry requires, among other things, a symmetric recombination...
This paper describes the design of Mach Zehnder Interferometer and reviews its applications in emerg...
Direct detections of Earth-like extrasolar planets are extremely challenging and require to overcome...
We present an interferometer design that provides a null at the star and a direct measurement of bot...
International audienceContext: Recently, an increasing number of scientific publications making use ...
International audienceContext: Recently, an increasing number of scientific publications making use ...
International audienceContext: Direct detection of a planet around a star and its characterisation f...
International audienceContext: Direct detection of a planet around a star and its characterisation f...
A self-switching mechanism in Mach-Zehnder interferometers (MZIs) is described. The input light sign...
Context. To find evidence one day of life on extra solar planets, one will have to directly detect p...
Deep, stable nulling of starlight requires careful control of the amplitudes and phases of the beams...
The Polarization-Based Collimated Beam Combiner efficiently produces pairwise interference between b...
International audienceContext: Direct detection of a planet around a star and its characterisation f...
International audienceNulling interferometry requires, among other things, a symmetric recombination...
International audienceNulling interferometry requires, among other things, a symmetric recombination...
International audienceNulling interferometry requires, among other things, a symmetric recombination...
This paper describes the design of Mach Zehnder Interferometer and reviews its applications in emerg...
Direct detections of Earth-like extrasolar planets are extremely challenging and require to overcome...
We present an interferometer design that provides a null at the star and a direct measurement of bot...
International audienceContext: Recently, an increasing number of scientific publications making use ...
International audienceContext: Recently, an increasing number of scientific publications making use ...
International audienceContext: Direct detection of a planet around a star and its characterisation f...
International audienceContext: Direct detection of a planet around a star and its characterisation f...
A self-switching mechanism in Mach-Zehnder interferometers (MZIs) is described. The input light sign...
Context. To find evidence one day of life on extra solar planets, one will have to directly detect p...
Deep, stable nulling of starlight requires careful control of the amplitudes and phases of the beams...
The Polarization-Based Collimated Beam Combiner efficiently produces pairwise interference between b...
International audienceContext: Direct detection of a planet around a star and its characterisation f...