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New Limits to the Small Scale Fluctuations in the Cosmic Background Radiation

Published online by Cambridge University Press:  04 August 2017

K. I. Kellermann ,
E. B. Fomalont  and
J. V. Wall
K. I. Kellermann
Affiliation:
National Radio Astronomy Observatory*
E. B. Fomalont
Affiliation:
National Radio Astronomy Observatory*
J. V. Wall
Affiliation:
Royal Greenwich Observatory

Extract

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The VLA has been used at 4.9 GHz to observe a small region of sky in order to extend the radio source count to low flux density (Fomalont et al., these proceedings) and to look for small scale fluctuations in the 2.7 K cosmic microwave background radiation.

Type
Research Article
Information
Symposium - International Astronomical Union , Volume 104: Early Evolution of the Universe and Its Present Structure , 1983 , pp. 125 - 126
Copyright
Copyright © Reidel 1983