An analysis based on the Bayes theorem is applied to study the Primary Cosmic Ray spectrum with the ARGO-YBJ detector. The method is discussed in the framework of the superposition model, in order to assess the detector capability to measure the spectral index of the all-nucleon spectrum

Bussino, S.A.M., De Marinis, E., Mari, S.M. (2003). The Primary Cosmic Ray All Nucleon Spectrum As Seen By ARGO-YBJ. In 28th International Cosmic Ray Conference (pp.255-258). TOKYO : Universal Academy Press, Inc..

The Primary Cosmic Ray All Nucleon Spectrum As Seen By ARGO-YBJ

BUSSINO, Severino Angelo Maria;MARI, Stefano Maria
2003-01-01

Abstract

An analysis based on the Bayes theorem is applied to study the Primary Cosmic Ray spectrum with the ARGO-YBJ detector. The method is discussed in the framework of the superposition model, in order to assess the detector capability to measure the spectral index of the all-nucleon spectrum
2003
4-946443-80-8
Bussino, S.A.M., De Marinis, E., Mari, S.M. (2003). The Primary Cosmic Ray All Nucleon Spectrum As Seen By ARGO-YBJ. In 28th International Cosmic Ray Conference (pp.255-258). TOKYO : Universal Academy Press, Inc..
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11590/184089
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