Point-source Detection

Point-Source Detection is a methodology in ground-based gamma-ray astronomy that identifies localized astrophysical sources of gamma radiation by distinguishing statistically significant emissions from background noise within angular resolution limits of the observatory.

372

Publications

32K

Citations

5K

Authors

813

Institutions

Publications per year

2017–2026

72

Authors

5K

  1. TM
    T. Montaruli

    University of Wisconsin–Madison, United States

    9 publications · 673 citations

    10

    h-index

  2. SF
    S. Fegan

    Centre National de la Recherche Scientifique, France

    10 publications · 1.3K citations

    10

    h-index

  3. UK
    U. Katz

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    9 publications · 583 citations

    10

    h-index

  4. JJ
    J. J. Beatty

    The Ohio State University, United States

    9 publications · 396 citations

    10

    h-index

  5. GA
    G. Anton

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    8 publications · 523 citations

    9

    h-index

1–5 of 5K

Venues

  1. The Astrophysical Journal

    ApJ · 78 publications · 4.3K citations

    37

    h-index

  2. Astronomy and Astrophysics

    28 publications · 1.7K citations

    23

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    31 publications · 1.3K citations

    21

    h-index

  4. The Astrophysical Journal Supplement Series

    15 publications · 2.2K citations

    14

    h-index

  5. The Astrophysical Journal Letters

    11 publications · 500 citations

    12

    h-index

1–5