Primary Beam Correction
Primary Beam Correction is a radiometric calibration technique used in radio astronomy that adjusts observed intensities to account for the sensitivity variation of a radio telescope's primary beam across the field of view, thereby enabling accurate flux measurement of off-axis sources.
54
Publications
4.2K
Citations
397
Authors
133
Institutions
Publications per year
2017–2026
11
Parents
54
The GMRT 150 MHz all-sky radio survey
H. T. Intema, P. Jagannathan, K. P. Mooley et al. · Astronomy and Astrophysics · 2016 · 862 citations · Full text
The GMRT 150 MHz All-sky Radio Survey: First Alternative Data Release TGSS ADR1
H. T. Intema, P. Jagannathan, K. P. Mooley et al. · eSpace (Curtin University) · 2016 · 319 citations · Full text
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National Radio Astronomy Observatory
Charlottesville, United States
16 h-index
40 publications
6.2K citations
Netherlands Institute for Radio Astronomy
Dwingeloo, The Netherlands
5 h-index
11 publications
576 citations
University of California, Berkeley
Berkeley, United States
5 h-index
13 publications
747 citations

University of Cape Town
Rondebosch, South Africa
4 h-index
8 publications
1.7K citations

Commonwealth Scientific and Industrial Research Organisation
Canberra, Australia
4 h-index
20 publications
1.2K citations
Australia Telescope National Facility
Sydney, Australia
4 h-index
5 publications
446 citations
University of Pennsylvania
Philadelphia, United States
3 h-index
5 publications
164 citations

University of Toronto
Toronto, Canada
3 h-index
15 publications
788 citations
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10 publications · 750 citations
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ApJ · 6 publications · 280 citations
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6 publications · 1.3K citations
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AJ · 4 publications · 190 citations
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2 publications · 196 citations
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