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. Le-programme-d-'inversion, Nous avons procédéprocédéà des phases de test sur des simulations d'arcs (ou anneaux d'Einstein) Quelques aspects de ce travail sont présentés dans la section suivante. Après cetté etape de validation du code, nous l'avons appliquéappliquéà une image HST de l'arc atypique dans Abel 1201

. Afin-de-valider-le-code, nous avons simulé plusieurs arcs multiples issus d'une sourcésourcé etendue unique Je présente ici le cas d'un modèle de lentille isotherme elliptique EIRC (cf annexe B.2) qui déforme une petite source elliptique ayant un profil de brillance gaussien

. Avec-trois-filtres, de la répartition des objets dans un diagramme couleur-couleur. C'est la méthode plus précise que j'ai utilisé pour le superamas de galaxies MS0302+17 AyantàAyantà ma disposition trois filtres B, V et R (les deux premiersétantpremiersétant nettement moins profonds que letroisì eme), j'ai pu placer les objets dans un plan

L. De-même and E. So, La figure 3 de la publication associée page 120 fournit une illustration de la méthode. Tous ces objets sontévidemmentéliminéssontévidemmentsontévidemmentéliminés du catalogue des sources darrì ere-plan. Malheureusement trois filtres ne sont pas suffisants pour déterminer un décalage spectral d'une galaxie spirale latetype avec