Application of Machine Learning Ensemble Methods to ASTRI Mini-Array Cherenkov Event Reconstruction
Problem
Imaging Atmospheric Cherenkov Telescope data is overwhelmingly dominated by cosmic-ray background, requiring efficient gamma/hadron separation and energy reconstruction.
Why it matters
Rejecting background is essential to discovering and characterizing very high-energy gamma-ray astrophysical sources.
What the AI did
Supervised machine learning methods, including Random Forest, were assessed and compared for gamma/hadron separation and energy reconstruction on simulated ASTRI Mini-Array data.
Results
not stated in source
Impact
ML methods were evaluated for event reconstruction on simulated ASTRI telescope data.
Record
| Venue | Applied Sciences |
|---|---|
| Published | 2023 |
| Work type | article |
| Authors | Antonio Pagliaro, G. Cusumano, A. La Barbera, Valentina La Parola, Saverio Lombardi |
| Citations | 11 (OpenAlex, at import time) |
| References | 25 |
| Model or method | Random Forest and other supervised ML methods |
| Organization | not stated in source |
| Primary source | https://doi.org/10.3390/app13148172 |
| Open access | gold |
| Keywords | machine learning, Cherenkov telescopes, gamma-ray astronomy, event reconstruction, background rejection |
Importance rating
real but narrower advance
Background rejection is essential for discovering and characterizing VHE gamma-ray sources, a specialized astrophysics subfield; no broad societal scale stated.
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