Absolute Photometry

Absolute Photometry is a photometric method that determines the total flux of celestial sources in physical units by calibrating measurements relative to established standard stars or reference systems, thereby enabling quantitative comparisons across observations and instruments.

161

Publications

11.1K

Citations

988

Authors

333

Institutions

Publications per year

2017–2026

11

Authors

988

  1. MC
    Martin Cohen

    University of California, Berkeley, United States

    3 publications · 103 citations

    3

    h-index

  2. RA
    R. A. Swaters

    University of Maryland, College Park, United States

    3 publications · 577 citations

    3

    h-index

  3. MB
    M. Balcells

    Instituto de Astrofísica de Canarias, Spain

    3 publications · 258 citations

    3

    h-index

  4. RE
    Rudolph E. Schild

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 572 citations

    3

    h-index

  5. JM
    James Muzerolle

    University of Arizona, United States

    3 publications · 940 citations

    3

    h-index

1–5 of 988

Venues

  1. The Astronomical Journal

    AJ · 32 publications · 2.8K citations

    21

    h-index

  2. The Astrophysical Journal

    ApJ · 21 publications · 1.8K citations

    18

    h-index

  3. 14

    h-index

  4. Astronomy and Astrophysics

    12 publications · 1.1K citations

    12

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 12 publications · 1.1K citations

    12

    h-index

1–5