Paper
5 July 2000 Fizeau beam combination with optical interferometers: some ideas for second-generation VLTI instrumentation
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Abstract
All ground based interferometers are using a Michelson beam combination scheme in their current and planned interferometric instruments. This leads to a severe restriction on their interferometric field-of-view. One can overcome this restriction by using Fizeau beam combination instead. We are describing a possible scheme for Fizeau beam combination with two and more telescopes, trying to minimize the technical complexity and at the same time giving better signal-to-noise characteristics than previously favored concepts.
© (2000) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Markus Schoeller "Fizeau beam combination with optical interferometers: some ideas for second-generation VLTI instrumentation", Proc. SPIE 4006, Interferometry in Optical Astronomy, (5 July 2000); https://doi.org/10.1117/12.390191
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Cited by 5 scholarly publications.
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KEYWORDS
Telescopes

Interferometry

Signal to noise ratio

Space telescopes

Interferometers

Sensors

Point spread functions

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