Ageron, M.; Aguilar, J.; Al Samarai, I.; Albert, A.; Andre, M.; Anghinolfi, M.; Anton, G.... (2012). The ANTARES telescope neutrino alert system. Astroparticle Physics. 35(8):530-536. https://doi.org/10.1016/j.astropartphys.2011.11.011
Por favor, use este identificador para citar o enlazar este ítem: http://hdl.handle.net/10251/36273
Título:
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The ANTARES telescope neutrino alert system
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Autor:
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Ageron, M
Aguilar, JA
Al Samarai, I
Albert, A
Andre, M
Anghinolfi, M
Anton, G
Anvar, S
Ardid Ramírez, Miguel
Bou Cabo, Manuel
Camarena Femenia, Francisco
Ferri García, Marcelino
Larosa, Giuseppina
Martínez Mora, Juan Antonio
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Entidad UPV:
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Universitat Politècnica de València. Departamento de Física Aplicada - Departament de Física Aplicada
Universitat Politècnica de València. Instituto de Investigación para la Gestión Integral de Zonas Costeras - Institut d'Investigació per a la Gestió Integral de Zones Costaneres
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Fecha difusión:
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Resumen:
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The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance ...[+]
The ANTARES telescope has the capability to detect neutrinos produced in astrophysical transient sources. Potential sources include gamma-ray bursts, core collapse supernovae, and flaring active galactic nuclei. To enhance the sensitivity of ANTARES to such sources, a new detection method based on coincident observations of neutrinos and optical signals has been developed. A fast online muon track reconstruction is used to trigger a network of small automatic optical telescopes. Such alerts are generated for special events, such as two or more neutrinos, coincident in time and direction, or single neutrinos of very high energy.
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Palabras clave:
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ANTARES
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Neutrino astronomy
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Optical follow-up
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Transient sources
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Alert systems
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Core collapse supernovae
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Detection methods
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Flaring active
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Gamma ray bursts
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Muon tracks
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Optical signals
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Potential sources
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Very high energies
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Gamma rays
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Optical telescopes
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Stars
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Neutrons
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Derechos de uso:
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Reserva de todos los derechos
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Fuente:
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Astroparticle Physics. (issn:
0927-6505
)
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DOI:
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10.1016/j.astropartphys.2011.11.011
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Editorial:
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Elsevier
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Versión del editor:
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http://dx.doi.org/10.1016/j.astropartphys.2011.11.011
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Código del Proyecto:
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info:eu-repo/grantAgreement/MICINN//CSD2009-00064/ES/Método de Multimensajeros para la Detección de la Materia Oscura/
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Agradecimientos:
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This work has been financially supported by the GdR PCHE in France. We want to thank M. Kowalski for discussions on the neutrino triggers and the organization of the optical follow-up.
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Tipo:
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Artículo
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