Testing Gamma/Hadron Separation for Ultra-High-Energy Cherenkov Astronomy

Dark100 is a planned array of six telescopes, using the Panoramic Search for Extraterrestrial Intelligence (PANOSETI) telescope system. It will operate as an imaging atmospheric Cherenkov telescope array, with a telescope design and array layout optimized for accessing gamma rays with tens of TeV to PeV energies. The science goals of Dark100 include the search for ultra-heavy dark matter, observations of Galactic Pevatrons, and the search for ultra-fast optical transients. Rejection of background cosmic rays is key to the sensitivity of the array. We present a first study of gamma/hadron separation based on simulated gamma rays and protons, focusing on the impact of the hadronic background models used in CORSIKA.

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Publication Details

Published
2025-09-24
DOI
https://doi.org/10.22323/1.501.0519
Primary Topic
Particle Detector Development and Performance
Type
article
Field-Weighted Citation Impact
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article

Testing Gamma/Hadron Separation for Ultra-High-Energy Cherenkov Astronomy

Yuriy Popovych, Dan Werthimer, Nicolas Rault-Wang, Andrew W. Howard et al.
Particle Detector Development and Performance
article

Testing Gamma/Hadron Separation for Ultra-High-Energy Cherenkov Astronomy

Yuriy Popovych, Dan Werthimer, Nicolas Rault-Wang, Andrew W. Howard, S. Wright, N. Korzoun, E. Pueschel, Benjamin Godfrey, Paul Horowitz, Alyssa E. Johnson, Felix Riehn, Sruthiranjani Ravikularaman, D. Elsäesser, Aaron Brown, J. Holder, Jérôme Maîre, Wei Liu
article en

Abstract

Dark100 is a planned array of six telescopes, using the Panoramic Search for Extraterrestrial Intelligence (PANOSETI) telescope system. It will operate as an imaging atmospheric Cherenkov telescope array, with a telescope design and array layout optimized for accessing gamma rays with tens of TeV to PeV energies. The science goals of Dark100 include the search for ultra-heavy dark matter, observations of Galactic Pevatrons, and the search for ultra-fast optical transients. Rejection of background cosmic rays is key to the sensitivity of the array. We present a first study of gamma/hadron separation based on simulated gamma rays and protons, focusing on the impact of the hadronic background models used in CORSIKA.

National Science Foundation, California Institute of Technology, Harvard University, Planetary Society, Secretário de Ciência, Tecnologia e Ensino Superior, Governo do Estado de Parana, University of California, San Diego, University of California Observatories
Openalex Percentile: Top 89%
Particle Detector Development and Performance
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