Geomagnetic field effects on background primary electrons for low energy Cherenkov Telescopes
Extensive air showers produced by primary electrons constitute an important component of the background signal for imaging atmospheric Cherenkov Telescopes with low energy thresholds. When the threshold for gamma-ray detection is very low, down to 3-5 GeV as suggested for large telescopes at high al...
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| Autores principales: | Supanitsky, A.D., Rovero, A.C. |
|---|---|
| Formato: | CONF |
| Materias: | |
| Acceso en línea: | http://hdl.handle.net/20.500.12110/paper_NIS23756_v9_n_p50_Supanitsky |
| Aporte de: |
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