Energy Reconstruction in Analysis of Cherenkov Telescopes Images in TAIGA Experiment Using Deep Learning Methods
Imaging Atmospheric Cherenkov Telescopes (IACT) of TAIGA astrophysical complex allow to observe high energy gamma radiation helping to study many astrophysical objects and processes. TAIGA-IACT enables us to select gamma quanta from the total cosmic radiation flux and recover their primary parameter...
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description | Imaging Atmospheric Cherenkov Telescopes (IACT) of TAIGA astrophysical complex allow to observe high energy gamma radiation helping to study many astrophysical objects and processes. TAIGA-IACT enables us to select gamma quanta from the total cosmic radiation flux and recover their primary parameters, such as energy and direction of arrival. The traditional method of processing the resulting images is an image parameterization - so-called the Hillas parameters method. At the present time Machine Learning methods, in particular Deep Learning methods have become actively used for IACT image processing. This paper presents the analysis of simulated Monte Carlo images by several Deep Learning methods for a single telescope (mono-mode) and multiple IACT telescopes (stereo-mode). The estimation of the quality of energy reconstruction was carried out and their energy spectra were analyzed using several types of neural networks. Using the developed methods the obtained results were also compared with the results obtained by traditional methods based on the Hillas parameters. |
doi_str_mv | 10.48550/arxiv.2211.08971 |
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Using the developed methods the obtained results were also compared with the results obtained by traditional methods based on the Hillas parameters.</description><subject>Computer Science - Learning</subject><subject>Cosmic rays</subject><subject>Deep learning</subject><subject>Direction of arrival</subject><subject>Energy spectra</subject><subject>Gamma ray telescopes</subject><subject>Image processing</subject><subject>Image reconstruction</subject><subject>Machine learning</subject><subject>Neural networks</subject><subject>Parameterization</subject><subject>Parameters</subject><subject>Physics - High Energy Astrophysical Phenomena</subject><subject>Physics - Instrumentation and Methods for Astrophysics</subject><subject>Radiation</subject><subject>Taiga & tundra</subject><subject>Telescopes</subject><issn>2331-8422</issn><fulltext>true</fulltext><rsrctype>article</rsrctype><creationdate>2022</creationdate><recordtype>article</recordtype><sourceid>ABUWG</sourceid><sourceid>AFKRA</sourceid><sourceid>AZQEC</sourceid><sourceid>BENPR</sourceid><sourceid>CCPQU</sourceid><sourceid>DWQXO</sourceid><sourceid>GOX</sourceid><recordid>eNotkNFqwjAUhsNgMHE-wK4W2HVdcmKa9rI45wTHYHTXJW1PtE6TLqmib2_VXf0czsfPOR8hT5yNJ4mU7FX7Y3MYA3A-Zkmq-B0ZgBA8SiYAD2QUwoYxBrECKcWAtDOLfnWi31g5Gzq_r7rGWdpYmlm9PYUmUGfodI0e7a870By3GCrXYqCLnV710aN5tphndHZs0Tc7tB39CY1d0TfEli5Re3uZPrFbuzo8knujtwFH_zkk-fssn35Ey6_5YpotIy1BRmBirEtWotSGlYZxTIQGVHWaJiadsFgqWXJlSi2UMQq5MXW_U2kqagmqFEPyfKu96ija_jDtT8VFS3HV0hMvN6L17m-PoSs2bu_7p0MBSihQwEGKM2rIZqs</recordid><startdate>20221116</startdate><enddate>20221116</enddate><creator>Gres, E O</creator><creator>Kryukov, A P</creator><general>Cornell University Library, arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PIMPY</scope><scope>PQEST</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope><scope>AKY</scope><scope>GOX</scope></search><sort><creationdate>20221116</creationdate><title>Energy Reconstruction in Analysis of Cherenkov Telescopes Images in TAIGA Experiment Using Deep Learning Methods</title><author>Gres, E O ; 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TAIGA-IACT enables us to select gamma quanta from the total cosmic radiation flux and recover their primary parameters, such as energy and direction of arrival. The traditional method of processing the resulting images is an image parameterization - so-called the Hillas parameters method. At the present time Machine Learning methods, in particular Deep Learning methods have become actively used for IACT image processing. This paper presents the analysis of simulated Monte Carlo images by several Deep Learning methods for a single telescope (mono-mode) and multiple IACT telescopes (stereo-mode). The estimation of the quality of energy reconstruction was carried out and their energy spectra were analyzed using several types of neural networks. 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subjects | Computer Science - Learning Cosmic rays Deep learning Direction of arrival Energy spectra Gamma ray telescopes Image processing Image reconstruction Machine learning Neural networks Parameterization Parameters Physics - High Energy Astrophysical Phenomena Physics - Instrumentation and Methods for Astrophysics Radiation Taiga & tundra Telescopes |
title | Energy Reconstruction in Analysis of Cherenkov Telescopes Images in TAIGA Experiment Using Deep Learning Methods |
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