Fizeau beam combination with optical interferometers: some ideas for second-generation VLTI instrumentation

Details Fizeau beam combination with optical interferometers: some ideas for second-generation VLTI instrumentation Fizeau beam combination with optical interferometers: some ideas for second-generation VLTI instrumentation

Jul 2000

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2000spie.4006..116s&link_type=abstract

Proc. SPIE Vol. 4006, p. 116-123, Interferometry in Optical Astronomy, Pierre J. Lena; Andreas Quirrenbach; Eds.

Astronomy and Astrophysics

Astronomy

1

Scientific paper

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.

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