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Wide-Field-Imaging 3-Mirror-Systems by High Light Gathering Power and a Wide-Field Optical System for the ‘Large Imaging Telescope’ (Lite)

Published online by Cambridge University Press:  26 July 2016

U. Laux
U. Laux*
Affiliation:
Thüringer Landessternwarte Tautenburg, Karl-Schwarzschild-Observatorium, D-07778 Tautenburg, Germany

Extract

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The desire of astronomers for wide field telescope systems which surpass the RCC (1:8 max. 1.5 degree) in light gathering power and field of view are relative concrete today. For this type of telescope, detectors planned ARE CCDs in multichip arrangement.

Type
Part Two: Digital Detectors in Wide-Field Imaging
Information
Symposium - International Astronomical Union , Volume 161: Astronomy from Wide-Field Imaging , 1994 , pp. 101 - 107
Copyright
Copyright © Kluwer 1994 

References

Laux, U., Astrooptik, Sterne und Weltraum Taschenbuch Nr. 11.Google Scholar
Wilson, R., 1992. Optical Design Considerations for modern Telescopes. Google Scholar
Wilson, R. and Laux, U. A European Large Wide-field Telescope Beratung in Tautenburg 26.9.92, Vortrag ESO Meeting 11.12.92.Google Scholar
Patenschrift Google Scholar