Investigating the VHE Gamma-ray Sources Using Deep Neural Networks

Vodeb V, Bhattacharyya S, Principe G, Zaharijaš G, Austri R, Stoppa F, Caron S, Malyshev D (2024)


Publication Type: Conference contribution

Publication year: 2024

Journal

Publisher: Sissa Medialab Srl

Book Volume: 444

Conference Proceedings Title: Proceedings of Science

Event location: Nagoya, JPN

Abstract

The upcoming Cherenkov Telescope Array (CTA) will dramatically improve the point-source sensitivity compared to the current Imaging Atmospheric Cherenkov Telescopes (IACTs). One of the key science projects of CTA will be a survey of the whole Galactic plane (GPS) using both southern and northern observatories, specifically focusing on the inner galactic region. We extend a deep learning-based image segmentation software pipeline (autosource-id) developed on Fermi-LAT data to detect and classify extended sources for the simulated CTA GPS. Using updated instrument response functions for CTA (Prod5), we test this pipeline on simulated gamma-ray sources lying in the inner galactic region (specifically 0 < l < 20, |b| < 3) for energies ranging from 30 GeV to 100 TeV. Dividing the source extensions ranging from 0.03 to 1 in three different classes, we find that using a simple and light convolutional neural network it is possible to achieve a 97% global accuracy in separating the extended sources from the point-like sources. The neural net architecture including other data pre-processing codes is available online.

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How to cite

APA:

Vodeb, V., Bhattacharyya, S., Principe, G., Zaharijaš, G., Austri, R., Stoppa, F.,... Malyshev, D. (2024). Investigating the VHE Gamma-ray Sources Using Deep Neural Networks. In Proceedings of Science. Nagoya, JPN: Sissa Medialab Srl.

MLA:

Vodeb, V., et al. "Investigating the VHE Gamma-ray Sources Using Deep Neural Networks." Proceedings of the 38th International Cosmic Ray Conference, ICRC 2023, Nagoya, JPN Sissa Medialab Srl, 2024.

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