A targeted search for point sources of EeV neutrons

A flux of neutrons from an astrophysical source in the Galaxy can be detected in the Pierre Auger Observatory as an excess of cosmic-ray air showers arriving from the direction of the source. To avoid the statistical penalty for making many trials, classes of objects are tested in combinations as ni...

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Detalles Bibliográficos
Autores principales:	Dova, María Teresa, Gómez Albarracín, Flavia Alejandra, Hansen, Patricia María, Jarne, Cecilia Gisele, Mariazzi, Analisa Gabriela, Moreno, Juan Cruz, Sciutto, Sergio Juan, Wahlberg, Hernán Pablo, The Pierre Auger Collaboration
Formato:	Articulo
Lenguaje:	Inglés
Publicado:	2014
Materias:	Física Astronomía cosmic rays Galaxy: disk methods: data analysis
Acceso en línea:	http://sedici.unlp.edu.ar/handle/10915/79334 https://arxiv.org/abs/1406.4038v1
Aporte de:	SEDICI (UNLP) de Universidad Nacional de La Plata

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