TL;DR
This study applies machine learning algorithms to classify uncertain gamma-ray sources in the 4FGL catalog, achieving over 91% accuracy in distinguishing blazar types using minimal parameters.
Contribution
It demonstrates the effectiveness of supervised machine learning models in classifying Fermi blazars and identifies optimal parameter combinations for high accuracy.
Findings
Random forests, SVMs, and ANNs achieve over 91% accuracy.
Optimal models use 8 to 12 parameters for best performance.
Predicted 724 BL Lac and 332 FSRQ candidates with high confidence.
Abstract
The recently published fourth Fermi Large Area Telescope source catalog (4FGL) reports 5065 gamma-ray sources in terms of direct observational gamma-ray properties. Among the sources, the largest population is the Active Galactic Nuclei (AGN), which consists of 3137 blazars, 42 radio galaxies, and 28 other AGNs. The blazar sample comprises 694 flat-spectrum radio quasars (FSRQs), 1131 BL Lac-type objects (BL Lacs), and 1312 blazar candidates of an unknown type (BCUs). The classification of blazars is difficult using optical spectroscopy given the limited knowledge with respect to their intrinsic properties, and the limited availability of astronomical observations. To overcome these challenges, machine learning algorithms are being investigated as alternative approaches. Using the 4FGL catalog, a sample of 3137 Fermi blazars with 23 parameters is systematically selected. Three…
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