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A Measurement of Excess Antenna Temperature at 4080 Mc/s.

Penzias, A. A., Wilson, R. W.·1965·The Astrophysical Journal

Abstract

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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Metadata

Authors
Penzias, A. A., & Wilson, R. W.
Venue
The Astrophysical Journal
Published
1965-07
Volume
142
Pages
419
ISSN
  • 0004-637X (ISSN-L)
  • 1538-4357
OpenAlex
W1997756830
Cited by
2,604
References
0
FWCI
46.62
Type
journal article
Language
en
Open access
closed

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CoChat. (2026). Citation check: A Measurement of Excess Antenna Temperature at 4080 Mc/s. https://app.cochat.ai/papers/10.1086/148307
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Penzias, A. A., & Wilson, R. W. (1965). A Measurement of Excess Antenna Temperature at 4080 Mc/s. The Astrophysical Journal. https://doi.org/10.1086/148307

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