Gamma-ray Blazar Classification using Machine Learning with Advanced Weight Initialization and Self-Supervised Learning Techniques
Gopal Bhatta, Sarvesh Gharat, Abhimanyu Borthakur, Aman Kumar

TL;DR
This paper presents a machine learning approach employing advanced initialization and self-supervised techniques to classify gamma-ray blazars into BL Lac and FSRQ types, improving simplicity and deployment efficiency.
Contribution
It introduces a novel machine learning classification method with minimal features and parameters, utilizing advanced initialization and self-supervised learning for gamma-ray source classification.
Findings
Classified 820 sources as BL Lacs
Classified 295 sources as FSRQs
Achieved high accuracy with simple model
Abstract
Machine learning has emerged as a powerful tool in the field of gamma-ray astrophysics. The algorithms can distinguish between different source types, such as blazars and pulsars, and help uncover new insights into the high-energy universe. The Large Area Telescope (LAT) on-board the Fermi Gamma-ray telescope has significantly advanced our understanding of the Universe. The instrument has detected a large number of gamma-ray emitting sources, among which a significant number of objects have been identified as active galactic nuclei (AGN). The sample is primarily composed of blazars; however, more than one-third of these sources are either of an unknown class or lack a definite association with a low-energy counterpart. In this work, we employ multiple machine learning algorithms to classify the sources based on their other physical properties. In particular, we utilized smart…
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Taxonomy
TopicsAstrophysics and Cosmic Phenomena · Computational Physics and Python Applications · Particle physics theoretical and experimental studies
