Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy
- Autores
- Guelfand, Marion; Decoene, Valentin; Martineau Huynh, Olivier; Prunet, Simon; Tueros, Matias Jorge; Macias, Oscar; Benoit Lévy, Aurélien
- Año de publicación
- 2025
- Idioma
- inglés
- Tipo de recurso
- artículo
- Estado
- versión publicada
- Descripción
- Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above ∼ 10^17 eV. The next-generation of radio experiments aims to extend this technique to the ob-servation of UHE earth-skimming neutrinos, which requires the detection ofvery inclined extensive air showers (EAS). In this article we present a newreconstruction method for the arrival direction and the energy of EAS. Itcombines a point-source-like description of the radio wavefront with a phe-nomenological model: the Angular Distribution Function (ADF). The ADFdescribes the angular distribution of the radio signal amplitude in the 50-200 MHz frequency range, with a particular focus on the Cherenkov angle,a crucial feature of the radio amplitude pattern. The method is applica-ble to showers with zenith angles larger than 60°, and in principle up toneutrino-induced showers with up-going trajectories. It is tested here on asimulated data set of EAS induced by cosmic rays. A resolution better than 4 arc-minutes (0.07°) is achieved on arrival direction, as well as an intrin-sic resolution of 5% on the electromagnetic energy, and around 15% on theprimary energy.
Fil: Guelfand, Marion. Campus Pierre Et Marie Curie ; Sorbonne University;
Fil: Decoene, Valentin. Universite de Nantes; Francia
Fil: Martineau Huynh, Olivier. Campus Pierre Et Marie Curie ; Sorbonne University;
Fil: Prunet, Simon. Observatoire de la Cote D'Azur; Francia
Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina
Fil: Macias, Oscar. San Francisco State University; Estados Unidos
Fil: Benoit Lévy, Aurélien. Universite Paris-saclay (universite Paris-saclay); - Materia
-
Ultra-High-Energy Astroparticles
Extensive Air Showers,
Radio-Detection
Reconstruction - Nivel de accesibilidad
- acceso abierto
- Condiciones de uso
- https://creativecommons.org/licenses/by-nc-nd/2.5/ar/
- Repositorio
.jpg)
- Institución
- Consejo Nacional de Investigaciones Científicas y Técnicas
- OAI Identificador
- oai:ri.conicet.gov.ar:11336/281284
Ver los metadatos del registro completo
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Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energyGuelfand, MarionDecoene, ValentinMartineau Huynh, OlivierPrunet, SimonTueros, Matias JorgeMacias, OscarBenoit Lévy, AurélienUltra-High-Energy AstroparticlesExtensive Air Showers,Radio-DetectionReconstructionhttps://purl.org/becyt/ford/1.3https://purl.org/becyt/ford/1Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above ∼ 10^17 eV. The next-generation of radio experiments aims to extend this technique to the ob-servation of UHE earth-skimming neutrinos, which requires the detection ofvery inclined extensive air showers (EAS). In this article we present a newreconstruction method for the arrival direction and the energy of EAS. Itcombines a point-source-like description of the radio wavefront with a phe-nomenological model: the Angular Distribution Function (ADF). The ADFdescribes the angular distribution of the radio signal amplitude in the 50-200 MHz frequency range, with a particular focus on the Cherenkov angle,a crucial feature of the radio amplitude pattern. The method is applica-ble to showers with zenith angles larger than 60°, and in principle up toneutrino-induced showers with up-going trajectories. It is tested here on asimulated data set of EAS induced by cosmic rays. A resolution better than 4 arc-minutes (0.07°) is achieved on arrival direction, as well as an intrin-sic resolution of 5% on the electromagnetic energy, and around 15% on theprimary energy.Fil: Guelfand, Marion. Campus Pierre Et Marie Curie ; Sorbonne University;Fil: Decoene, Valentin. Universite de Nantes; FranciaFil: Martineau Huynh, Olivier. Campus Pierre Et Marie Curie ; Sorbonne University;Fil: Prunet, Simon. Observatoire de la Cote D'Azur; FranciaFil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; ArgentinaFil: Macias, Oscar. San Francisco State University; Estados UnidosFil: Benoit Lévy, Aurélien. Universite Paris-saclay (universite Paris-saclay);Elsevier Science2025-09info:eu-repo/semantics/articleinfo:eu-repo/semantics/publishedVersionhttp://purl.org/coar/resource_type/c_6501info:ar-repo/semantics/articuloapplication/pdfapplication/pdfapplication/pdfhttp://hdl.handle.net/11336/281284Guelfand, Marion; Decoene, Valentin; Martineau Huynh, Olivier; Prunet, Simon; Tueros, Matias Jorge; et al.; Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy; Elsevier Science; Astroparticle Physics; 171; 9-2025; 1-150927-6505CONICET DigitalCONICETenginfo:eu-repo/semantics/altIdentifier/url/https://linkinghub.elsevier.com/retrieve/pii/S092765052500043Xinfo:eu-repo/semantics/altIdentifier/doi/10.1016/j.astropartphys.2025.103120info:eu-repo/semantics/openAccesshttps://creativecommons.org/licenses/by-nc-nd/2.5/ar/reponame:CONICET Digital (CONICET)instname:Consejo Nacional de Investigaciones Científicas y Técnicas2026-02-26T10:23:47Zoai:ri.conicet.gov.ar:11336/281284instacron:CONICETInstitucionalhttp://ri.conicet.gov.ar/Organismo científico-tecnológicoNo correspondehttp://ri.conicet.gov.ar/oai/requestdasensio@conicet.gov.ar; lcarlino@conicet.gov.arArgentinaNo correspondeNo correspondeNo correspondeopendoar:34982026-02-26 10:23:47.683CONICET Digital (CONICET) - Consejo Nacional de Investigaciones Científicas y Técnicasfalse |
| dc.title.none.fl_str_mv |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy |
| title |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy |
| spellingShingle |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy Guelfand, Marion Ultra-High-Energy Astroparticles Extensive Air Showers, Radio-Detection Reconstruction |
| title_short |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy |
| title_full |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy |
| title_fullStr |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy |
| title_full_unstemmed |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy |
| title_sort |
Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy |
| dc.creator.none.fl_str_mv |
Guelfand, Marion Decoene, Valentin Martineau Huynh, Olivier Prunet, Simon Tueros, Matias Jorge Macias, Oscar Benoit Lévy, Aurélien |
| author |
Guelfand, Marion |
| author_facet |
Guelfand, Marion Decoene, Valentin Martineau Huynh, Olivier Prunet, Simon Tueros, Matias Jorge Macias, Oscar Benoit Lévy, Aurélien |
| author_role |
author |
| author2 |
Decoene, Valentin Martineau Huynh, Olivier Prunet, Simon Tueros, Matias Jorge Macias, Oscar Benoit Lévy, Aurélien |
| author2_role |
author author author author author author |
| dc.subject.none.fl_str_mv |
Ultra-High-Energy Astroparticles Extensive Air Showers, Radio-Detection Reconstruction |
| topic |
Ultra-High-Energy Astroparticles Extensive Air Showers, Radio-Detection Reconstruction |
| purl_subject.fl_str_mv |
https://purl.org/becyt/ford/1.3 https://purl.org/becyt/ford/1 |
| dc.description.none.fl_txt_mv |
Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above ∼ 10^17 eV. The next-generation of radio experiments aims to extend this technique to the ob-servation of UHE earth-skimming neutrinos, which requires the detection ofvery inclined extensive air showers (EAS). In this article we present a newreconstruction method for the arrival direction and the energy of EAS. Itcombines a point-source-like description of the radio wavefront with a phe-nomenological model: the Angular Distribution Function (ADF). The ADFdescribes the angular distribution of the radio signal amplitude in the 50-200 MHz frequency range, with a particular focus on the Cherenkov angle,a crucial feature of the radio amplitude pattern. The method is applica-ble to showers with zenith angles larger than 60°, and in principle up toneutrino-induced showers with up-going trajectories. It is tested here on asimulated data set of EAS induced by cosmic rays. A resolution better than 4 arc-minutes (0.07°) is achieved on arrival direction, as well as an intrin-sic resolution of 5% on the electromagnetic energy, and around 15% on theprimary energy. Fil: Guelfand, Marion. Campus Pierre Et Marie Curie ; Sorbonne University; Fil: Decoene, Valentin. Universite de Nantes; Francia Fil: Martineau Huynh, Olivier. Campus Pierre Et Marie Curie ; Sorbonne University; Fil: Prunet, Simon. Observatoire de la Cote D'Azur; Francia Fil: Tueros, Matias Jorge. Consejo Nacional de Investigaciones Científicas y Técnicas. Centro Científico Tecnológico Conicet - La Plata. Instituto de Física La Plata. Universidad Nacional de La Plata. Facultad de Ciencias Exactas. Instituto de Física La Plata; Argentina Fil: Macias, Oscar. San Francisco State University; Estados Unidos Fil: Benoit Lévy, Aurélien. Universite Paris-saclay (universite Paris-saclay); |
| description |
Radio detection is now an established technique for the study of ultra-high-energy (UHE) cosmic rays with energies above ∼ 10^17 eV. The next-generation of radio experiments aims to extend this technique to the ob-servation of UHE earth-skimming neutrinos, which requires the detection ofvery inclined extensive air showers (EAS). In this article we present a newreconstruction method for the arrival direction and the energy of EAS. Itcombines a point-source-like description of the radio wavefront with a phe-nomenological model: the Angular Distribution Function (ADF). The ADFdescribes the angular distribution of the radio signal amplitude in the 50-200 MHz frequency range, with a particular focus on the Cherenkov angle,a crucial feature of the radio amplitude pattern. The method is applica-ble to showers with zenith angles larger than 60°, and in principle up toneutrino-induced showers with up-going trajectories. It is tested here on asimulated data set of EAS induced by cosmic rays. A resolution better than 4 arc-minutes (0.07°) is achieved on arrival direction, as well as an intrin-sic resolution of 5% on the electromagnetic energy, and around 15% on theprimary energy. |
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2025 |
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2025-09 |
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http://hdl.handle.net/11336/281284 Guelfand, Marion; Decoene, Valentin; Martineau Huynh, Olivier; Prunet, Simon; Tueros, Matias Jorge; et al.; Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy; Elsevier Science; Astroparticle Physics; 171; 9-2025; 1-15 0927-6505 CONICET Digital CONICET |
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Guelfand, Marion; Decoene, Valentin; Martineau Huynh, Olivier; Prunet, Simon; Tueros, Matias Jorge; et al.; Reconstruction of inclined extensive air showers using radio signals: From arrival times and amplitudes to direction and energy; Elsevier Science; Astroparticle Physics; 171; 9-2025; 1-15 0927-6505 CONICET Digital CONICET |
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eng |
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