Field correction for very large telescopes

Details Field correction for very large telescopes Field correction for very large telescopes

Apr 1995

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1995mnras.273l..45w&link_type=abstract

Monthly Notices of the Royal Astronomical Society, Volume 273, Issue 3, pp. L45-L46.

Astronomy and Astrophysics

Astronomy

Instrumentation: Miscellaneous, Telescopes

Scientific paper

Very large telescopes at present being built or planned commonly have a mirror configuration involving quite highly aberrated field imagery at the Cassegrain focus, the only focus accessible. These aberrations cause problems for instrumentation, both with and without the use of adaptive optics. The possibility of designing correctors to give wide field imagery is discussed.

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