Photometric Zero Points

Photometric Zero Points is a calibration constant in stellar photometry that defines the magnitude of a source producing one detected photon per unit time at a specified wavelength or passband, thereby establishing the reference flux level for photometric measurements in ultraviolet photometry and related observational systems.

44

Publications

7.6K

Citations

312

Authors

147

Institutions

Publications per year

2017–2026

8

Authors

312

  1. DJ
    David J. Schlegel

    Lawrence Berkeley National Laboratory, United States

    2 publications · 443 citations

    2

    h-index

  2. BJ
    Benjamin J. Taylor

    Brigham Young University, United States

    2 publications · 32 citations

    2

    h-index

  3. MD
    M. D. Joner

    Brigham Young University, United States

    2 publications · 32 citations

    2

    h-index

  4. MD
    M. Dennefeld

    Institut d'Astrophysique de Paris, France

    2 publications · 98 citations

    2

    h-index

  5. SC
    S. Cassisi

    Collurania Teramo Observatory, Italy

    2 publications · 365 citations

    2

    h-index

1–5 of 312

Venues

  1. The Astronomical Journal

    AJ · 9 publications · 3.6K citations

    9

    h-index

  2. Publications of the Astronomical Society of the Pacific

    PASP · 7 publications · 385 citations

    7

    h-index

  3. 6

    h-index

  4. The Astrophysical Journal

    ApJ · 4 publications · 326 citations

    4

    h-index

  5. The Astrophysical Journal Supplement Series

    4 publications · 1.3K citations

    4

    h-index

1–5