We noticed two typos in Appendix C.2.1 in the published article, in the analytical parameterization of the local interstellar spectrum of He nuclei, Equation (C2), and in an expression for T(x), Equation (C32). The correct expressions are provided below: FHc(R) = {a - bR + c√sin(r) +[dRG(fR)2- gR]sin(R) - (h + iR)G(fr), R ≤ 2.5 GV, R-2.0[l + M/R + n/R2+ o/p + qR + r tanh (s/t + uR) - vz3/R], R ≥ 2.5 GV, Here FHe(R) is the differential intensity in units (m2s sr GV)-1, R is the particle rigidity in GV, G(x) is a function defined in Equation (C30), and the values of the fitting parameters a to z are given in Table C1. The function T(x) is defined as: T (x) = (3.764 x2)xG(x)3.764xThis work is supported by ASI (Agenzia Spaziale Italiana) through contract ASI-INFN No. 2019-19-HH.0 and by ESA (European Space Agency) through contract 4000116146/16/NL/HK. I.V.M. and T.A.P. acknowledge support from NASA grant No. NNX17AB48G.
Boschini, M., Della Torre, S., Gervasi, M., Grandi, D., Johannesson, G., La Vacca, G., et al. (2021). Erratum: Inference of the Local Interstellar Spectra of Cosmic-Ray Nuclei Z ≤ 28 with the GALPROP-HELMOD Framework (ApJS (2020) 250 (27) DOI: 10.3847/1538-4365/aba901) [Altro] [10.3847/1538-4365/ac2518].
Erratum: Inference of the Local Interstellar Spectra of Cosmic-Ray Nuclei Z ≤ 28 with the GALPROP-HELMOD Framework (ApJS (2020) 250 (27) DOI: 10.3847/1538-4365/aba901)
Gervasi M.;Grandi D.;La Vacca G.;Pensotti S.;Rozza D.;Tacconi M.
2021
Abstract
We noticed two typos in Appendix C.2.1 in the published article, in the analytical parameterization of the local interstellar spectrum of He nuclei, Equation (C2), and in an expression for T(x), Equation (C32). The correct expressions are provided below: FHc(R) = {a - bR + c√sin(r) +[dRG(fR)2- gR]sin(R) - (h + iR)G(fr), R ≤ 2.5 GV, R-2.0[l + M/R + n/R2+ o/p + qR + r tanh (s/t + uR) - vz3/R], R ≥ 2.5 GV, Here FHe(R) is the differential intensity in units (m2s sr GV)-1, R is the particle rigidity in GV, G(x) is a function defined in Equation (C30), and the values of the fitting parameters a to z are given in Table C1. The function T(x) is defined as: T (x) = (3.764 x2)xG(x)3.764xThis work is supported by ASI (Agenzia Spaziale Italiana) through contract ASI-INFN No. 2019-19-HH.0 and by ESA (European Space Agency) through contract 4000116146/16/NL/HK. I.V.M. and T.A.P. acknowledge support from NASA grant No. NNX17AB48G.
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