Photometric Transformations

Photometric Transformations is a methodological framework in stellar photometry that enables the conversion of observed magnitudes and color indices from one photometric system to another by accounting for differences in instrumental response functions, atmospheric extinction, and standardization conventions.

127

Publications

20.8K

Citations

447

Authors

235

Institutions

Publications per year

2017–2026

21

Variants

Photometric Transformation

Authors

447

  1. BJ
    Benjamin J. Taylor

    Brigham Young University, United States

    5 publications · 167 citations

    5

    h-index

  2. MS
    M. S. Bessell

    Australian National University, Australia

    5 publications · 3.4K citations

    5

    h-index

  3. EG
    E. González-Solares

    University of Cambridge, United Kingdom

    3 publications · 222 citations

    3

    h-index

  4. KS
    Kazuhiro Shimasaku

    The University of Tokyo, Japan

    3 publications · 3.3K citations

    3

    h-index

  5. CJ
    C. Jordi

    Universitat de Barcelona, Spain

    3 publications · 564 citations

    3

    h-index

1–5 of 447

Venues

  1. Publications of the Astronomical Society of the Pacific

    PASP · 18 publications · 6.5K citations

    15

    h-index

  2. The Astronomical Journal

    AJ · 15 publications · 2.2K citations

    14

    h-index

  3. 10

    h-index

  4. The Astrophysical Journal

    ApJ · 9 publications · 1.7K citations

    9

    h-index

  5. Astronomy and Astrophysics

    6 publications · 1.3K citations

    6

    h-index

1–5