Cherenkov Light Detection

Cherenkov Light Detection is a method in gamma-ray astronomy that identifies and measures high-energy gamma rays by detecting the faint, ultrashort flashes of Cherenkov radiation produced when gamma-ray-induced extensive air showers generate relativistic charged particles in Earth's atmosphere.

246

Publications

8K

Citations

4.6K

Authors

642

Institutions

Publications per year

2017–2026

55

Authors

4.6K

  1. WR
    W. Rhode

    TU Dortmund University, Germany

    10 publications · 840 citations

    10

    h-index

  2. EB
    E. Bernardini

    TU Dortmund University, Germany

    8 publications · 687 citations

    8

    h-index

  3. GA
    G. Anton

    Friedrich-Alexander-Universität Erlangen-Nürnberg, Germany

    8 publications · 557 citations

    8

    h-index

  4. AC
    A. Chiavassa

    University of Turin, Italy

    8 publications · 394 citations

    8

    h-index

  5. AK
    A. Kappes

    University of Wisconsin–Madison, United States

    8 publications · 753 citations

    8

    h-index

1–5 of 4.6K

Venues

  1. 25

    h-index

  2. Journal of Instrumentation

    JINST · 18 publications · 751 citations

    13

    h-index

  3. Astroparticle Physics

    10 publications · 448 citations

    10

    h-index

  4. EPJ Web of Conferences

    8 publications · 191 citations

    8

    h-index

  5. The European Physical Journal C

    7 publications · 458 citations

    7

    h-index

1–5