Surface Brightness Fluctuations

Surface Brightness Fluctuations is a photometric distance measurement method that relies on the variance in pixel-to-pixel brightness of a galaxy's resolved stellar population to estimate its distance by quantifying the apparent fluctuations in surface brightness caused by the discrete distribution of stars.

369

Publications

40.7K

Citations

1.3K

Authors

543

Institutions

Publications per year

2017–2026

60

Authors

1.3K

  1. JT
    J. Tonry

    University of Hawaii System, United States

    26 publications · 3K citations

    25

    h-index

  2. JP
    John P. Blakeslee

    Johns Hopkins University, United States

    25 publications · 2.9K citations

    23

    h-index

  3. EA
    Edward A. Ajhar

    Kitt Peak National Observatory, United States

    12 publications · 1.2K citations

    12

    h-index

  4. MC
    Michele Cantiello

    Collurania Teramo Observatory, Italy

    12 publications · 604 citations

    12

    h-index

  5. LF
    Laura Ferrarese

    Herzberg Institute of Astrophysics, Canada

    11 publications · 2K citations

    11

    h-index

1–5 of 1.3K

Venues

  1. The Astrophysical Journal

    ApJ · 128 publications · 13.4K citations

    50

    h-index

  2. The Astronomical Journal

    AJ · 40 publications · 5.4K citations

    27

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    42 publications · 12.7K citations

    27

    h-index

  4. Astronomy and Astrophysics

    38 publications · 1.5K citations

    23

    h-index

  5. The Astrophysical Journal Letters

    11 publications · 624 citations

    11

    h-index

1–5