, + z) m avec m = 0, 3 ou-3 et selon les équations 6.17 et 6.18, avec et sans la correction de la surdensité locale de galaxies. Pour chaque modèle, les figures suivantes sont présentées : le balayage des couples (R cut , ?) (en haut, à gauche), le spectre injecté aux sources des rayons cosmiques primaires, Cette annexe regroupe l'ensemble des figures relatives à l'ajustement combiné des données de spectre et de composition, développé dans le chapitre 6 et testant différents modèles d'évolution des sources en

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