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Optical System for the University of Texas 7.6M Telescope

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Instrumentation for Astronomy with Large Optical Telescopes

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 92))

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Abstract

As presently conceived, the large telescope now being planned at The University of Texas will have a Ritchey-Chrétien configuration, f/13.5, with a 7.6m diameter f/2 primary of ultra-thin construction, on an alt-azimuth mount.

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References

  1. Weekes, Trevor C. (ed.) 1979, “The MMT and The Future of Ground-Based Astronomy”, SAO Special Report 385.

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  2. Kohler, H. 1966, in “The Construction of Large Telescopes,” IAU Symp. 27, ed. D.L. Crawford, p. 9.

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  3. Gascoigne, S.C.B. 1973, Applied Optics 12, p. 1419.

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  4. Wilson, R.N. 1971, in Proc. ES0/CERN Conf. on Large Telescope Design, ed. R.M. West, p. 131.

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  5. Fehrenbach, C. 1968, in Support and Testing of Large Astronomical Mirrors, ed. D.L. Crawford, A.B. Meinel, and M.W. Stockton, Pub. KPNO, p. 66.

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  6. KPNO Quarterly Bulletin, April–June 1974, p. 24.

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© 1982 D. Reidel Publishing Company

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Tull, R.G., Barnes, T.G., Dittmar, D.N., Ray, F.B., Pearson, E. (1982). Optical System for the University of Texas 7.6M Telescope. In: Humphries, C.M. (eds) Instrumentation for Astronomy with Large Optical Telescopes. Astrophysics and Space Science Library, vol 92. Springer, Dordrecht. https://doi.org/10.1007/978-94-009-7787-7_5

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  • DOI: https://doi.org/10.1007/978-94-009-7787-7_5

  • Publisher Name: Springer, Dordrecht

  • Print ISBN: 978-94-009-7789-1

  • Online ISBN: 978-94-009-7787-7

  • eBook Packages: Springer Book Archive

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