Single-mode optical fibers are playing an increasing role in astronomical interferometry, e.g., in high-accuracy visibility measurements and in nulling interferometry. However, such observing modes typically involve only small numbers of fibers. On the other hand, some recently proposed observing techniques call for arrays of single mode fibers coupled to arrays of sub-apertures within a large telescope pupil. The concepts include pupil-masked visibility measurements (non-redundant masking), pupil-sheared nulling interferometry, and coronagraphic imaging using a fiber-linked phased-array of small optical telescopes. The latter arrangement may also be relevant to optical communications. Here we provide an overview of a number of recent novel...
Adaptive Optics is now making it possible to efficiently use large telescopes in ground-based interf...
Aims: In this paper we present the first on-sky results with the fibered aperture masking instrument...
Classical single-mode fiber interferometers, using one fiber per aperture, have very limited imaging...
Single-mode optical fibers are playing an increasing role in astronomical interferometry, e.g., in h...
A rotating nulling coronagraph has been built for use on ground-based telescopes. The system is base...
he small angular distance (<100 mas) and the huge flux ratio (107) between an Earth-like exoplanet i...
International audienceFIRST, the Fibered Imager foR a Single Telescope instrument, is an ultra-high ...
Using single-mode fibers (SMFs) in the image plane of coronagraphs allows access to a new wavefront ...
High-dispersion coronagraphy (HDC) optimally combines high contrast imaging techniques such as adapt...
Despite recent advances in high-contrast imaging techniques, high resolution spectroscopy for charac...
Vortex Fiber Nulling (VFN) is an interferometric method for suppressing starlight to detect and spec...
Long baseline interferometry is now a mature technique in the optical domain. Current interferometer...
Aims. In this paper we present the first on-sky results with the fibered aperture masking instrument...
The small angular distance (<100 mas) and the huge flux ratio (10^7) between an Earth-like exoplanet...
Vortex fiber nulling is a method for spectroscopically characterizing exoplanets at small angular se...
Adaptive Optics is now making it possible to efficiently use large telescopes in ground-based interf...
Aims: In this paper we present the first on-sky results with the fibered aperture masking instrument...
Classical single-mode fiber interferometers, using one fiber per aperture, have very limited imaging...
Single-mode optical fibers are playing an increasing role in astronomical interferometry, e.g., in h...
A rotating nulling coronagraph has been built for use on ground-based telescopes. The system is base...
he small angular distance (<100 mas) and the huge flux ratio (107) between an Earth-like exoplanet i...
International audienceFIRST, the Fibered Imager foR a Single Telescope instrument, is an ultra-high ...
Using single-mode fibers (SMFs) in the image plane of coronagraphs allows access to a new wavefront ...
High-dispersion coronagraphy (HDC) optimally combines high contrast imaging techniques such as adapt...
Despite recent advances in high-contrast imaging techniques, high resolution spectroscopy for charac...
Vortex Fiber Nulling (VFN) is an interferometric method for suppressing starlight to detect and spec...
Long baseline interferometry is now a mature technique in the optical domain. Current interferometer...
Aims. In this paper we present the first on-sky results with the fibered aperture masking instrument...
The small angular distance (<100 mas) and the huge flux ratio (10^7) between an Earth-like exoplanet...
Vortex fiber nulling is a method for spectroscopically characterizing exoplanets at small angular se...
Adaptive Optics is now making it possible to efficiently use large telescopes in ground-based interf...
Aims: In this paper we present the first on-sky results with the fibered aperture masking instrument...
Classical single-mode fiber interferometers, using one fiber per aperture, have very limited imaging...