Photometric Reduction

Photometric Reduction is a data reduction method in observational astronomy that calibrates raw detector measurements to derive precise apparent brightness values of celestial sources by correcting for instrumental, atmospheric, and geometric effects.

76

Publications

5K

Citations

428

Authors

220

Institutions

Publications per year

2017–2026

15

Authors

428

  1. PB
    P. B. Stetson

    Herzberg Institute of Astrophysics, Canada

    3 publications · 501 citations

    3

    h-index

  2. MN
    M. Nonino

    Trieste Astronomical Observatory, Italy

    3 publications · 501 citations

    3

    h-index

  3. SK
    Sergii Khlamov

    Kharkiv National University of Radio Electronics, Ukraine

    2 publications · 60 citations

    2

    h-index

  4. JF
    Joseph F. Hennawi

    Max Planck Institute for Astronomy, Germany

    2 publications · 548 citations

    2

    h-index

  5. ED
    E. Deul

    Leiden University, Netherlands

    2 publications · 469 citations

    2

    h-index

1–5 of 428

Venues

  1. Publications of the Astronomical Society of the Pacific

    PASP · 9 publications · 1K citations

    9

    h-index

  2. 6

    h-index

  3. The Astrophysical Journal

    ApJ · 7 publications · 402 citations

    6

    h-index

  4. The Astronomical Journal

    AJ · 5 publications · 204 citations

    5

    h-index

  5. Astronomy and Astrophysics

    5 publications · 438 citations

    5

    h-index

1–5