Stellar Photometry

Stellar Photometry is the scientific measurement of the brightness or flux of stars, distinguished by its focus on quantifying stellar light intensity across specific wavelength bands to determine physical properties such as luminosity, temperature, and distance.

6.8K

Publications

470.9K

Citations

16.2K

Authors

1.9K

Institutions

Publications per year

2017–2026

1.1K

Authors

16.2K

  1. DQ
    D. Queloz

    University of Geneva, Switzerland

    75 publications · 6.8K citations

    44

    h-index

  2. SU
    S. Udry

    University of Geneva, Switzerland

    61 publications · 5.8K citations

    42

    h-index

  3. CA
    C. Aerts

    KU Leuven, Belgium

    74 publications · 13.9K citations

    41

    h-index

  4. MG
    M. Gillon

    University of Liège, Belgium

    63 publications · 5.1K citations

    40

    h-index

  5. FB
    F. Bouchy

    University of Geneva, Switzerland

    58 publications · 5.1K citations

    37

    h-index

1–5 of 16.2K

Venues

  1. The Astrophysical Journal

    ApJ · 1.3K publications · 98.3K citations

    144

    h-index

  2. The Astronomical Journal

    AJ · 1.1K publications · 86.5K citations

    127

    h-index

  3. Astronomy and Astrophysics

    932 publications · 67.4K citations

    112

    h-index

  4. Monthly Notices of the Royal Astronomical Society

    1.2K publications · 56.7K citations

    106

    h-index

  5. The Astrophysical Journal Supplement Series

    276 publications · 36.6K citations

    86

    h-index

1–5