Zero-point Calibration

Zero-Point Calibration is a methodological procedure in observational astronomy that establishes the absolute reference point for photometric magnitude systems, enabling the conversion of observed apparent magnitudes into absolute magnitudes by anchoring empirical measurements to a standardized flux scale.

46

Publications

6.2K

Citations

228

Authors

127

Institutions

Publications per year

2017–2026

16

Authors

228

  1. RB
    R. Brent Tully

    University of Hawaii System, United States

    4 publications · 1.2K citations

    4

    h-index

  2. DB
    Dillon Brout

    Center for Astrophysics Harvard & Smithsonian, United States

    3 publications · 2.3K citations

    3

    h-index

  3. LM
    Lucas M. Macri

    Texas A&M University, United States

    2 publications · 2.3K citations

    2

    h-index

  4. AV
    A. V. Filippenko

    University of California, Berkeley, United States

    2 publications · 2.3K citations

    2

    h-index

  5. JM
    John MacKenty

    Space Telescope Science Institute, United States

    2 publications · 2.3K citations

    2

    h-index

1–5 of 228

Venues

  1. 13

    h-index

  2. The Astrophysical Journal

    ApJ · 10 publications · 1K citations

    10

    h-index

  3. The Astronomical Journal

    AJ · 4 publications · 643 citations

    4

    h-index

  4. arXiv (Cornell University)

    Repository · 3 publications · 258 citations

    3

    h-index

  5. Publications of the Astronomical Society of the Pacific

    PASP · 2 publications · 82 citations

    2

    h-index

1–5