Contents 1 Parameters of vertical SD energy bias 1 2 Parameterization of inclined SD energy resolution 1 The Pierre Auger collaboration 2 1 Parameters of vertical SD energy bias In the original article, there were typographical errors in the values of the parameters in eq. (B.5). The correct values are P0 = 0.0566, P1 = -0.0720, P2 = 0.0227. 2 Parameterization of inclined SD energy resolution The original article incorrectly stated that the folding procedure for the inclined spectrum was fully described in ref. [68], which actually only contains a qualitative discussion. The parameterizations we used for the trigger efficiency T , the energy bias b and the energy resolution E/E were: T = 1; b = 1; and (Formula Presented).
Combined fit of spectrum and composition data as measured by the Pierre Auger Observatory (vol 4, 038, 2017)
ANASTASI, JESSICA;Aramo C.;S. Buscemi;CATALDI, ALESSIA;R. M.;DI GIULIO, Augusto;R. Garcia;LAS CASAS, Maria Carmela;Insolia A.;AYSAR M.M., YASIN;PIRRONELLO, SILVIA MARIA GRAZIA;BONILLA VARELA, ADELAIDA;
2018-01-01
Abstract
Contents 1 Parameters of vertical SD energy bias 1 2 Parameterization of inclined SD energy resolution 1 The Pierre Auger collaboration 2 1 Parameters of vertical SD energy bias In the original article, there were typographical errors in the values of the parameters in eq. (B.5). The correct values are P0 = 0.0566, P1 = -0.0720, P2 = 0.0227. 2 Parameterization of inclined SD energy resolution The original article incorrectly stated that the folding procedure for the inclined spectrum was fully described in ref. [68], which actually only contains a qualitative discussion. The parameterizations we used for the trigger efficiency T , the energy bias b and the energy resolution E/E were: T = 1; b = 1; and (Formula Presented).File | Dimensione | Formato | |
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_2018_J._Cosmol._Astropart._Phys._2018_E02-erratum.pdf
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