Foreground Component Separation

Foreground Component Separation is a computational method in cosmic microwave background observations that isolates the cosmological signal from superimposed astrophysical emissions by distinguishing their spectral, spatial, and statistical properties.

198

Publications

20.4K

Citations

1.3K

Authors

385

Institutions

Publications per year

2017–2026

69

Authors

1.3K

  1. CD
    C. Dickinson

    University of Manchester, United Kingdom

    29 publications · 5.5K citations

    26

    h-index

  2. KM
    K. M. Górski

    University of Warsaw, Poland

    26 publications · 9.4K citations

    24

    h-index

  3. MR
    M. Remazeilles

    University of Manchester, United Kingdom

    25 publications · 9.2K citations

    24

    h-index

  4. AL
    A. Lasenby

    University of Cambridge, United Kingdom

    26 publications · 9.2K citations

    23

    h-index

  5. RB
    R. B. Barreiro

    Universidad de Cantabria, Spain

    24 publications · 9.3K citations

    22

    h-index

1–5 of 1.3K

Venues

  1. Monthly Notices of the Royal Astronomical Society

    61 publications · 3.3K citations

    33

    h-index

  2. Astronomy and Astrophysics

    32 publications · 10.1K citations

    24

    h-index

  3. The Astrophysical Journal

    ApJ · 21 publications · 1.8K citations

    19

    h-index

  4. Journal of Cosmology and Astroparticle Physics

    JCAP · 9 publications · 340 citations

    9

    h-index

  5. arXiv (Cornell University)

    Repository · 5 publications · 151 citations

    5

    h-index

1–5