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arxiv: 2205.12188 · v1 · pith:R647VDHNnew · submitted 2022-05-24 · 🌌 astro-ph.HE · astro-ph.IM· hep-ex· physics.ins-det

Gamma/Hadron Separation with the HAWC Observatory

classification 🌌 astro-ph.HE astro-ph.IMhep-exphysics.ins-det
keywords gammahawchadronseparationgamma-rayobservatoryraysevents
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The High Altitude Water Cherenkov (HAWC) gamma-ray observatory observes atmospheric showers produced by incident gamma rays and cosmic rays with energy from 300 GeV to more than 100 TeV. A crucial phase in analyzing gamma-ray sources using ground-based gamma-ray detectors like HAWC is to identify the showers produced by gamma rays or hadrons. The HAWC observatory records roughly 25,000 events per second, with hadrons representing the vast majority ($>99.9\%$) of these events. The standard gamma/hadron separation technique in HAWC uses a simple rectangular cut involving only two parameters. This work describes the implementation of more sophisticated gamma/hadron separation techniques, via machine learning methods (boosted decision trees and neural networks), and summarizes the resulting improvements in gamma/hadron separation obtained in HAWC.

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