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LINC-NIRVANA: first attempt of an instrument for a 23-m-class telescope

Authors :
Thomas Bertram
Hans-Walter Rix
Jacopo Farinato
Carmelo Arcidiacono
Christian Straubmeier
Robert Weiss
Andreas Eckart
G. Weigelt
W. Xu
Emiliano Diolaiti
Wolfgang Gässler
Roberto Ragazzoni
Roberto Soci
David R. Andersen
Udo Beckmann
Hermann Böhnhardt
Harald Baumeister
Piero Salinari
Elise Vernet-Viard
Tom Herbst
Peter Bizenberger
Sebastiano Ligori
Ralf-Rainer Rohloff
Source :
SPIE Proceedings.
Publication Year :
2004
Publisher :
SPIE, 2004.

Abstract

LINC-NIRVANA is a Fizeau interferometer which will be built for the Large Binocular Telescope (LBT). The LBT exists of two 8.4m mirrors on one mounting with a distance of 22.8m between the outer edges of the two mirrors. The interferometric technique used in LINC-NIRVANA provides direct imaging with the resolution of a 23m telescope in one direction and 8.4m in the other. The instrument uses multi-conjugated adaptive optics (MCAO) to increase the sky coverage and achieve the diffraction limit in J, H, K over a moderate Field of View (2 arcmin in diameter). During the preliminary design phase the team faced several problems similar to those for an instrument at a 23m telescope. We will give an overview of the current design, explain problems related to 20m class telescopes and present solutions.

Details

ISSN :
0277786X
Database :
OpenAIRE
Journal :
SPIE Proceedings
Accession number :
edsair.doi...........eee9a560025d67f6085bde24f61ff18b
Full Text :
https://doi.org/10.1117/12.566389