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Updated: May 30, 2026

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Time Multiplexing Super Resolving Technique for Imaging from a Moving Platform
Published on: February 12, 2014
Phase-shifting technique for improving the imaging capacity of sparse-aperture optical interferometers
1UMR 6525 H. Fizeau, Université de Nice-Sophia Antipolis, Centre National de la Recherche Scientifique, Observatoire de la Côte d’Azur, Avenue Nicolas Copernic, 06130 Grasse, France. francois.henault@obs‐azur.fr
Applied Optics
|July 21, 2011
Summary
A new multiaperture interferometer design enables high-angular resolution astronomical imaging using phase-shifting and Fourier inversion. This technique offers radiometric efficiency and simplified optical designs for capturing detailed snapshots of celestial objects.
Area of Science:
- Astronomy and Astrophysics
- Optical Engineering
Background:
- Current astronomical imaging techniques face limitations in achieving extreme angular resolution.
- Interferometry offers high resolution but can be complex to implement and calibrate.
Purpose of the Study:
- To present a novel multiaperture interferometer design for rapid, high-resolution astrophysical imaging.
- To highlight the advantages of this phase-shifting interferometer for astronomical observations.
Main Methods:
- Utilizes a phase-shifting technique combined with Fourier inversion for image reconstruction.
- Employs a multiaperture configuration suitable for coupling numerous telescopes.
- Numerical simulations were performed to validate the design's feasibility.
Main Results:
- The proposed interferometer demonstrates radiometric efficiency and a wide field of view comparable to Fizeau interferometers.
- A preliminary calibration procedure is outlined for characterizing instrumental errors.
- The design allows for significant simplification of optical and mechanical components, especially for large telescope arrays.
Conclusions:
- The multiaperture interferometer is a promising technology for achieving extreme angular resolution in astronomical snapshots.
- The design facilitates the integration of hundreds of telescopes onto a single detector, leveraging conventional and emerging optical technologies.

