Host Galaxy Identification

Host Galaxy Identification is the astrophysical process of associating a detected multimessenger signal, such as gravitational waves or neutrinos, with its specific galactic source environment through positional, redshift, and contextual observational data.

625

Publications

42.2K

Citations

4.4K

Authors

879

Institutions

Publications per year

2017–2026

209

Authors

4.4K

  1. SR
    S. R. Kulkarni

    California Institute of Technology, United States

    20 publications · 2.3K citations

    18

    h-index

  2. JS
    J. S. Bloom

    University of California, Berkeley, United States

    17 publications · 2.3K citations

    17

    h-index

  3. RF
    R. Falomo

    Osservatorio Astronomico di Padova, Italy

    22 publications · 1.1K citations

    16

    h-index

  4. MM
    M. Mignoli

    Osservatorio astronomico di Bologna, Italy

    15 publications · 1.2K citations

    15

    h-index

  5. MB
    M. Brusa

    University of Bologna, Italy

    15 publications · 1.4K citations

    15

    h-index

1–5 of 4.4K

Venues

  1. The Astrophysical Journal

    ApJ · 181 publications · 15.4K citations

    69

    h-index

  2. Monthly Notices of the Royal Astronomical Society

    120 publications · 5.3K citations

    42

    h-index

  3. Astronomy and Astrophysics

    87 publications · 4.5K citations

    40

    h-index

  4. The Astrophysical Journal Letters

    42 publications · 4.1K citations

    30

    h-index

  5. The Astronomical Journal

    AJ · 34 publications · 2.9K citations

    23

    h-index

1–5