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The Gregorian Upgrade at Arecibo and its Impact on Some Aspects of Extragalactic Research

  • Riccardo Giovanelli
Conference paper
Part of the Astrophysics and Space Science Library book series (ASSL, volume 141)

Abstract

The performance of the 305m telescope at Arecibo is flawed with a number of limitations that are related with the current optical design. These shortcomings are correctible with the replacement of line feeds with a Gregorian subreflector system and the construction of a ground shield around the edge of the main reflector. The upgrade will substantially increase the sensitivity of the telescope and allow optimal implementation of advances in electronic technology. Its potential impact on selected topics of extragalactic spectroscopy is discussed in some detail.

Keywords

Zenith Angle Line Feed Main Reflector Illumination Pattern Ground Radiation 
These keywords were added by machine and not by the authors. This process is experimental and the keywords may be updated as the learning algorithm improves.

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References

  1. Butcher, H. and Oemler Jr., A. 1981, Ap. J. 285,426ADSCrossRefGoogle Scholar
  2. Nilson, P. 1973, Uppsala General Catalog of Galaxies, Uppsala Ann. Obs. 6 (UGC)Google Scholar
  3. Zwicky, F., Herzog, E., Karpowicz, M., Kowal, C.T. and Wild, P. 1961–68, Catalogue of Galaxies and of Clusters of Galaxies ,6 volumes, Pasadena: Cal. Inst. of Tech. Press (CGCG)Google Scholar

Copyright information

© Kluwer Academic Publishers 1988

Authors and Affiliations

  • Riccardo Giovanelli
    • 1
    • 2
  1. 1.Arecibo ObservatoryNAICUSA
  2. 2.Arecibo ObservatoryArecibo P.R.USA

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