Abstract
In the context of atmospheric shower arrays designed for γ-ray astronomy and in the context of the ALTO project, we present: a study of the impact of heavier nuclei in the cosmic-ray background on the estimated γ-ray detection performance on the basis of dedicated Monte Carlo simulations, a method to calculate the sensitivity to a point-like source, and finally the required observation times to reach a firm detection on a list of known point-like sources.
| Original language | British English |
|---|---|
| Pages (from-to) | 1-13 |
| Number of pages | 13 |
| Journal | Journal of High Energy Astrophysics |
| Volume | 39 |
| DOIs | |
| State | Published - Aug 2023 |
Keywords
- ALTO project
- Analysis and statistical methods
- Extensive air showers
- Particle detector arrays
- Very high-energy γ-rays
- γ-ray experiments
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