Transient Source Detection

Transient Source Detection is a methodological framework in high-energy astrophysics that identifies abrupt, short-lived emissions of gamma-ray radiation from celestial sources by distinguishing statistically significant temporal variations in photon flux from background noise within observational data streams.

1.1K

Publications

64.8K

Citations

9.7K

Authors

1.3K

Institutions

Publications per year

2017–2026

299

Authors

9.7K

  1. FL
    F. Longo

    University of Trieste, Italy

    33 publications · 2.3K citations

    27

    h-index

  2. CK
    C. Kouveliotou

    Marshall Space Flight Center, United States

    37 publications · 3K citations

    22

    h-index

  3. KH
    K. Hurley

    University of California, Berkeley, United States

    43 publications · 2.1K citations

    22

    h-index

  4. DP
    D. Paneque

    University of Trieste, Italy

    23 publications · 1.8K citations

    21

    h-index

  5. SR
    S. R. Kulkarni

    California Institute of Technology, United States

    25 publications · 4.9K citations

    21

    h-index

1–5 of 9.7K

Venues

  1. The Astrophysical Journal

    ApJ · 277 publications · 18.1K citations

    65

    h-index

  2. Astronomy and Astrophysics

    102 publications · 5.8K citations

    45

    h-index

  3. Monthly Notices of the Royal Astronomical Society

    123 publications · 5.3K citations

    39

    h-index

  4. The Astrophysical Journal Letters

    65 publications · 5.6K citations

    38

    h-index

  5. Nature

    22 publications · 1.4K citations

    20

    h-index

1–5