Optimizing the Wasserstein GAN for TeV Gamma Ray Detection with VERITAS
Deivid Ribeiro, Yuping Zheng, Ramana Sankar, Kameswara Mantha (for, the VERITAS Collaboration)

TL;DR
This paper introduces an unsupervised Wasserstein GAN framework trained on VERITAS gamma-ray data to improve background rejection and gamma-ray detection in high-energy astrophysics.
Contribution
It proposes a novel WGAN-based method to analyze gamma-ray images, enhancing understanding and classification of real versus simulated events.
Findings
WGAN successfully models the latent space of gamma-ray images.
Preliminary results show improved background rejection capabilities.
Exploration of conditional parameters enhances model performance.
Abstract
The observation of very-high-energy (VHE, E>100 GeV) gamma rays is mediated by the imaging atmospheric Cherenkov technique (IACTs). At these energies, gamma rays interact with the atmosphere to create a cascade of electromagnetic air showers that are visible to the IACT cameras on the ground with distinct morphological and temporal features. However, hadrons with significantly higher incidence rates are also imaged with similar features, and must be distinguished with handpicked parameters extracted from the images. The advent of sophisticated deep learning models has enabled an alternative image analysis technique that has been shown to improve the detection of gamma rays, by improving background rejection. In this study, we propose an unsupervised Wasserstein Generative Adversarial Network (WGAN) framework trained on normalized, uncleaned stereoscopic shower images of real events from…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena
