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

Authors

397

  1. PA
    Paul Alexander

    University of Cambridge, United Kingdom

    4 publications · 173 citations

    4

    h-index

  2. DJ
    Daniel Jacobs

    Arizona State University, United States

    3 publications · 88 citations

    3

    h-index

  3. DA
    David A. Green

    University of Cambridge, United Kingdom

    3 publications · 143 citations

    3

    h-index

  4. AR
    Aaron R. Parsons

    University of California, Berkeley, United States

    3 publications · 169 citations

    3

    h-index

  5. JA
    James Aguirre

    University of Pennsylvania, United States

    3 publications · 88 citations

    3

    h-index

1–5 of 397

Venues

  1. 10

    h-index

  2. The Astrophysical Journal

    ApJ · 6 publications · 280 citations

    6

    h-index

  3. Astronomy and Astrophysics

    6 publications · 1.3K citations

    6

    h-index

  4. The Astronomical Journal

    AJ · 4 publications · 190 citations

    4

    h-index

  5. Journal of Applied Crystallography

    2 publications · 196 citations

    2

    h-index

1–5