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Measurements of the effective zenith noise temperature of the 20-foot horn-reflector antenna (Crawford, Hogg, and Hunt 1961) at the Crawford Hill Laboratory, Holmdel, New Jersey, at 4080 Mc/s have yielded a value of about 3.5 K higher than expected. This excess temperature is, within the limits of our observations, isotropic, unpolarized, and free from seasonal variations (July, 1964 - April, 1965). A possible explanation for the observed excess noise temperature is the one given by Dicke, Peebles, Roll, and Wilkinson (1965) in a companion letter in this issue.
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Penzias et al. (Thu,) studied this question.
www.synapsesocial.com/papers/69d68c5f3db2fe4b91db8265 — DOI: https://doi.org/10.1086/148307
A. A. Penzias
R. W. Wilson
The Astrophysical Journal
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