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Galactic background surveys and the galactic halo

Published online by Cambridge University Press:  14 August 2015

J. E. Baldwin
J. E. Baldwin*
Affiliation:
Mullard Radio Astronomy Observatory, Cavendish Laboratory Cambridge, England

Extract

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Two surveys of the galactic background radiation at low frequencies have recently been made at Cambridge. At 38 Mc/s, a survey of the sky between declinations −20° and +70° has been made by Blythe [1] using a new type of pencil-beam aerial system. This instrument, consisting of an array 1200 feet long in an east-west direction together with a small movable aerial, used the principle of aperture synthesis to provide a beam 2°.2 × 2°.3 at the zenith increasing to 2°.2 × 7°.4 at an angle of 70 degrees from the zenith.

Type
Part IV: The Large-Scale Structure of Galaxies
Information
Symposium - International Astronomical Union , Volume 9: Paris Symposium on Radio Astronomy , 1959 , pp. 460 - 464
Copyright
Copyright © Stanford University Press 1959 

References

1. Blythe, J. H. M.N.R.A.S. 117, 652, 1957.Google Scholar
2. Shain, C. A. Aust. J. Phys. 10, 195, 1957.CrossRefGoogle Scholar
3. Baldwin, J. E. M.N.R.A.S. 115, 684, 1955.Google Scholar
4. Reber, G., and Ellis, G. R. J. Geophys. Res. 61, 1, 1956.Google Scholar
5. Baldwin, J. E. The Observatory , 78, 166, 1958.Google Scholar