Angular Power Spectrum Analysis

Angular Power Spectrum Analysis is a statistical method used in cosmology to decompose the spatial fluctuations of the Cosmic Infrared Background into its angular frequency components, thereby quantifying the distribution of power as a function of angular scale on the sky.

760

Publications

68K

Citations

5.9K

Authors

855

Institutions

Publications per year

2017–2026

196

Authors

5.9K

  1. KM
    K. M. Górski

    University of Warsaw, Poland

    33 publications · 10.6K citations

    30

    h-index

  2. PD
    P. de Bernardis

    Sapienza University of Rome, Italy

    30 publications · 11.4K citations

    27

    h-index

  3. BP
    B. P. Crill

    California Institute of Technology, United States

    27 publications · 10.2K citations

    25

    h-index

  4. GP
    G. Polenta

    Centre National de la Recherche Scientifique, France

    28 publications · 10.2K citations

    25

    h-index

  5. EH
    E. Hivon

    California Institute of Technology, United States

    29 publications · 9.7K citations

    25

    h-index

1–5 of 5.9K

Venues

  1. The Astrophysical Journal

    ApJ · 121 publications · 15.7K citations

    63

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    140 publications · 10.8K citations

    51

    h-index

  3. 34

    h-index

  4. Journal of Cosmology and Astroparticle Physics

    JCAP · 72 publications · 2.9K citations

    33

    h-index

  5. Astronomy and Astrophysics

    42 publications · 10.9K citations

    29

    h-index

1–5