Halo Decomposition

Halo Decomposition is a computational framework in astrophysics that decomposes the rotation curve of a galaxy into distinct dynamical components—such as stellar, gaseous, and dark matter halo contributions—to isolate and characterize the gravitational influence of the dark matter halo.

41

Publications

2.8K

Citations

145

Authors

96

Institutions

Publications per year

2017–2026

8

Authors

145

  1. JJ
    Julianne J. Dalcanton

    University of Washington, United States

    4 publications · 347 citations

    4

    h-index

  2. GB
    G. Bertin

    University of Milan, Italy

    3 publications · 167 citations

    3

    h-index

  3. US
    Uroš Seljak

    Lawrence Berkeley National Laboratory, United States

    3 publications · 149 citations

    3

    h-index

  4. TO
    Teppei Okumura

    The University of Tokyo, Japan

    3 publications · 121 citations

    3

    h-index

  5. EM
    Enrico M. Di Teodoro

    Australian National University, Australia

    2 publications · 109 citations

    2

    h-index

1–5 of 145

Venues

  1. 13

    h-index

  2. The Astrophysical Journal

    ApJ · 7 publications · 671 citations

    7

    h-index

  3. Journal of Cosmology and Astroparticle Physics

    JCAP · 3 publications · 87 citations

    3

    h-index

  4. Astronomy and Astrophysics

    3 publications · 96 citations

    3

    h-index

  5. 2

    h-index

1–5