Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations
Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle...
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| Autor*in: |
Tzamarias, S. E. [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2021 |
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| Anmerkung: |
© Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. |
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| Übergeordnetes Werk: |
Enthalten in: Instruments and experimental techniques - Pleiades Publishing, 1959, 64(2021), 1 vom: Jan., Seite 127-140 |
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volume:64 ; year:2021 ; number:1 ; month:01 ; pages:127-140 |
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| DOI / URN: |
10.1134/S0020441220060202 |
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| 520 | |a Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. | ||
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| 700 | 1 | |a Tsirigotis, A. G. |4 aut | |
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10.1134/S0020441220060202 doi (DE-627)OLC2123995959 (DE-He213)S0020441220060202-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Tzamarias, S. E. verfasserin aut Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. Avgitas, T. aut Bourlis, G. aut Fanourakis, G. K. aut Gkialas, I. aut Leisos, A. aut Manthos, I. aut Tsirigotis, A. G. aut Enthalten in Instruments and experimental techniques Pleiades Publishing, 1959 64(2021), 1 vom: Jan., Seite 127-140 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:64 year:2021 number:1 month:01 pages:127-140 https://doi.org/10.1134/S0020441220060202 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY AR 64 2021 1 01 127-140 |
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10.1134/S0020441220060202 doi (DE-627)OLC2123995959 (DE-He213)S0020441220060202-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Tzamarias, S. E. verfasserin aut Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. Avgitas, T. aut Bourlis, G. aut Fanourakis, G. K. aut Gkialas, I. aut Leisos, A. aut Manthos, I. aut Tsirigotis, A. G. aut Enthalten in Instruments and experimental techniques Pleiades Publishing, 1959 64(2021), 1 vom: Jan., Seite 127-140 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:64 year:2021 number:1 month:01 pages:127-140 https://doi.org/10.1134/S0020441220060202 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY AR 64 2021 1 01 127-140 |
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10.1134/S0020441220060202 doi (DE-627)OLC2123995959 (DE-He213)S0020441220060202-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Tzamarias, S. E. verfasserin aut Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. Avgitas, T. aut Bourlis, G. aut Fanourakis, G. K. aut Gkialas, I. aut Leisos, A. aut Manthos, I. aut Tsirigotis, A. G. aut Enthalten in Instruments and experimental techniques Pleiades Publishing, 1959 64(2021), 1 vom: Jan., Seite 127-140 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:64 year:2021 number:1 month:01 pages:127-140 https://doi.org/10.1134/S0020441220060202 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY AR 64 2021 1 01 127-140 |
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10.1134/S0020441220060202 doi (DE-627)OLC2123995959 (DE-He213)S0020441220060202-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Tzamarias, S. E. verfasserin aut Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. Avgitas, T. aut Bourlis, G. aut Fanourakis, G. K. aut Gkialas, I. aut Leisos, A. aut Manthos, I. aut Tsirigotis, A. G. aut Enthalten in Instruments and experimental techniques Pleiades Publishing, 1959 64(2021), 1 vom: Jan., Seite 127-140 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:64 year:2021 number:1 month:01 pages:127-140 https://doi.org/10.1134/S0020441220060202 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY AR 64 2021 1 01 127-140 |
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10.1134/S0020441220060202 doi (DE-627)OLC2123995959 (DE-He213)S0020441220060202-p DE-627 ger DE-627 rakwb eng 620 VZ 11 ssgn Tzamarias, S. E. verfasserin aut Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations 2021 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. Avgitas, T. aut Bourlis, G. aut Fanourakis, G. K. aut Gkialas, I. aut Leisos, A. aut Manthos, I. aut Tsirigotis, A. G. aut Enthalten in Instruments and experimental techniques Pleiades Publishing, 1959 64(2021), 1 vom: Jan., Seite 127-140 (DE-627)129603007 (DE-600)241643-8 (DE-576)015096815 0020-4412 nnns volume:64 year:2021 number:1 month:01 pages:127-140 https://doi.org/10.1134/S0020441220060202 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-TEC SSG-OLC-PHY AR 64 2021 1 01 127-140 |
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Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations |
| abstract |
Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. |
| abstractGer |
Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. |
| abstract_unstemmed |
Abstract The Astroneu array consists of three autonomous Extensive Air Shower (EAS) detection stations installed and operated at the Hellenic Open University campus. Each station (Astroneu station) combines two different detection technologies. Three charged particle detectors arranged in a triangle and an RF antenna in the middle. Before installation several calibration procedures were performed both to the individual detectors of the array as well as to each integrated Astroneu station. In this paper we present the development of simulation methods, data analysis techniques and experimental procedures, which have been used to calibrate and optimize the operating parameters of the Astroneu particle detectors, to process the experimental signals and extract timing and amplitude information, to correct for systematic biases and estimate precisely the particle-front arrival time on each individual detector resulting to accurate reconstruction of the detected EAS direction. Furthermore, the performance of the Astroneu telescope in detecting and reconstructing EAS is demonstrated with special inter-calibration runs, where pairs of stations are detecting simultaneously the same air shower, as well as with comparisons against the predictions of a detailed simulation description of the detectors. © Pleiades Publishing, Ltd. 2020. ISSN 0020-4412, Instruments and Experimental Techniques, 2021, Vol. 64, No. 1, pp. 127–140. © Pleiades Publishing, Ltd., 2021. |
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| title_short |
Calibration Procedures for Accurate Timing and Directional Reconstruction of EAS Particle-fronts with Astroneu Stations |
| url |
https://doi.org/10.1134/S0020441220060202 |
| remote_bool |
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| author2 |
Avgitas, T. Bourlis, G. Fanourakis, G. K. Gkialas, I. Leisos, A. Manthos, I. Tsirigotis, A. G. |
| author2Str |
Avgitas, T. Bourlis, G. Fanourakis, G. K. Gkialas, I. Leisos, A. Manthos, I. Tsirigotis, A. G. |
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| doi_str |
10.1134/S0020441220060202 |
| up_date |
2024-07-03T21:14:51.859Z |
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