Aperture Photometry

Aperture photometry is a technique in stellar photometry that measures the flux of a celestial source by summing the detected photons within a defined circular or annular aperture centered on the object, while subtracting a local background estimate derived from an adjacent region.

222

Publications

12.3K

Citations

1.6K

Authors

505

Institutions

Publications per year

2017–2026

51

Authors

1.6K

  1. XZ
    Xu Zhou

    National Astronomical Observatories, China

    6 publications · 182 citations

    5

    h-index

  2. HW
    Hong Wu

    Chinese Academy of Sciences, China

    5 publications · 152 citations

    5

    h-index

  3. JM
    Jun Ma

    Chinese Academy of Sciences, China

    5 publications · 164 citations

    5

    h-index

  4. XY
    Xiangyan Yuan

    Nanjing Institute of Astronomical Optics & Technology, China

    5 publications · 168 citations

    4

    h-index

  5. ZZ
    Zhenxi Zhu

    UNSW Sydney, Australia

    5 publications · 168 citations

    4

    h-index

1–5 of 1.6K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    40 publications · 2.3K citations

    25

    h-index

  2. The Astronomical Journal

    AJ · 30 publications · 1.3K citations

    21

    h-index

  3. The Astrophysical Journal

    ApJ · 30 publications · 1.4K citations

    20

    h-index

  4. Astronomy and Astrophysics

    29 publications · 1.5K citations

    20

    h-index

  5. The Astrophysical Journal Supplement Series

    20 publications · 1.2K citations

    18

    h-index

1–5