High-frequency Radio Continuum
High-Frequency Radio Continuum is a type of radio continuum emission characterized by its origination in the high-frequency end of the radio spectrum, typically above a few gigahertz, and distinguished by its predominance of non-thermal processes such as synchrotron radiation and reduced influence from thermal bremsstrahlung and interstellar scintillation effects.
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9.5K
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1K
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358
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2017–2026
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Upper limit of the spectrum of cosmic rays
G.T. Zatsepin, V.A. Kuzmin · 1966 · 641 citations
Natural Sciences, Astronomy, Physics +13
Radio and millimeter continuum surveys and their astrophysical implications
G. de Zotti, M. Massardi, M. Negrello et al. · The Astronomy and Astrophysics Review · 2009 · 292 citations · Full text
Natural Sciences, Astronomy, Physics +14
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358
National Radio Astronomy Observatory
Charlottesville, United States
20 h-index
49 publications
2.1K citations
Max Planck Institute for Radio Astronomy
Bonn, Germany
16 h-index
54 publications
2.3K citations
Istituto di Radioastronomia di Bologna
Bologna, Italy
15 h-index
43 publications
1.7K citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
12 h-index
34 publications
998 citations

University of Manchester
Manchester, United Kingdom
12 h-index
31 publications
1.5K citations
California Institute of Technology
Pasadena, United States
11 h-index
35 publications
2.8K citations

University of Bologna
Bologna, Italy
10 h-index
24 publications
622 citations
Center for Astrophysics Harvard & Smithsonian
Cambridge, United States
9 h-index
16 publications
556 citations
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ApJ · 43 publications · 2K citations
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33 publications · 1.8K citations
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AJ · 26 publications · 976 citations
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23 publications · 861 citations
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14 publications · 581 citations
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