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The Bonn 408 MHz Survey

Published online by Cambridge University Press:  14 August 2015

C. G. T. Haslam ,
W. E. Wilson ,
D. A. Graham  and
G. C. Hunt
C. G. T. Haslam
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.
W. E. Wilson
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.
D. A. Graham
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.
G. C. Hunt
Affiliation:
Max-Planck-Institut für Radioastronomie, Bonn, F.R.G.

Abstract

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The 100 m telescope was used to complete the northern sky survey started at Jodrell Bank. The survey aimed at reaching the confusion limit of the telescope. Zero levels are consistent within ± 3 K, and scale errors are less than 10%. The survey will be published in the form of maps; a machine readable version is also available.

Type
Part 6: Large-Scale Galactic Structure
Information
Symposium - International Astronomical Union , Volume 60: Galactic Radio Astronomy , 1974 , pp. 649 - 650
Copyright
Copyright © Reidel 1974 

References

Haslam, C. G. T., Quigley, M. J. S., and Salter, C. J.: 1970, Monthly Notices Roy. Astron. Soc. 147, 405.CrossRefGoogle Scholar
Pauliny-Toth, I. I. K. and Shakeshaft, J. R.: 1962, Monthly Notices Roy. Astron. Soc. 124, 61.CrossRefGoogle Scholar