Cmb Angular Correlation Function

The CMB Angular Correlation Function is a statistical metric in cosmology that quantifies the degree of spatial correlation in temperature fluctuations of the Cosmic Microwave Background as a function of angular separation on the celestial sphere.

657

Publications

50.3K

Citations

3.1K

Authors

675

Institutions

Publications per year

2017–2026

121

Variants

Cosmic Microwave Background Angular Correlation Function

Authors

3.1K

  1. KM
    K. M. Górski

    University of Warsaw, Poland

    27 publications · 9.2K citations

    24

    h-index

  2. GD
    G. de Zotti

    Osservatorio Astronomico di Padova, Italy

    22 publications · 6.6K citations

    21

    h-index

  3. RB
    R. B. Barreiro

    Universidad de Cantabria, Spain

    20 publications · 9.4K citations

    20

    h-index

  4. AL
    A. Lasenby

    University of Cambridge, United Kingdom

    20 publications · 8.8K citations

    20

    h-index

  5. JC
    J.-F. Cardoso

    Centre National de la Recherche Scientifique, France

    20 publications · 9K citations

    20

    h-index

1–5 of 3.1K

Venues

  1. The Astrophysical Journal

    ApJ · 99 publications · 7K citations

    44

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    119 publications · 6.4K citations

    44

    h-index

  3. 33

    h-index

  4. Astronomy and Astrophysics

    42 publications · 11K citations

    30

    h-index

  5. Journal of Cosmology and Astroparticle Physics

    JCAP · 57 publications · 3.2K citations

    26

    h-index

1–5