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Radio Astronomy

descriptionPublicationkeyboard_double_arrow_right External research report , Report 15 Apr 1969 United States English Publisher:Research Laboratory of Electronics (RLE) at the Massachusetts Institute of Technology (MIT)
Authors: Papadopoulos, George D.; Schwartz, P. R.; Whitney, A. R.; Waters, J. W.; Wilson, W. J.; Zapata, C. A.; Price, R. M.; +10 Authors

handle: 1721.1/55857

Radio Astronomy

Abstract

Contains reports on seven research projects. ; M. I. T. Sloan Fund for Basic Research ; National Science Foundation (Grant GP-8415) ; Joint Services Electronics Programs (U. S. Army, U. S. Navy, and U. S. Air Force) under Contract DA 28-043-AMC-02536(E) ; National Aeronautics and Space Administration (Grant NGL 22-009-016)

Country
United States
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Keywords

20-Channel Digital Synchronous Detector, Observations of Radio Emission from Galactic H₂0, Pulsar Studies, Pulsar Facility, Radio Astronomy, KU-band Interferometer, Observations of OH Emission Associated with Infrared Stars, Very Long Baseline Interferometry

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Powered by OpenAIRE graph
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selected citations
These citations are derived from selected sources.
This is an alternative to the "Influence" indicator, which also reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Citations provided by BIP!
popularity
This indicator reflects the "current" impact/attention (the "hype") of an article in the research community at large, based on the underlying citation network.
BIP!Popularity provided by BIP!
influence
This indicator reflects the overall/total impact of an article in the research community at large, based on the underlying citation network (diachronically).
BIP!Influence provided by BIP!
impulse
This indicator reflects the initial momentum of an article directly after its publication, based on the underlying citation network.
BIP!Impulse provided by BIP!
0
Average
Average
Average
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