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. Compiègne, Pour une composition donnée, avec les valeurs liées aux propriétés des grains choisis (Q, C, distribution de taille DustEM calcule l'extinction et l'émission de la poussière considérée, soumise à un champ de rayonnement (par défaut, celui de Mathis et al. 1983, à 10 kpc) Le modèle de MC11) et THEMIS sont utilisés dans cette étude. Ils divergent par la nature des grains pris en compte (MC11 utilise une population de PAH, tandis que THEMIS modélise ceci par des manteaux aromatiques), la pente dans l'IR lointain (grains silicatés et carbonés ont le même indice spectral dans MC11, Outils utilisés Afin de créer les spectres d'émission à ajuster aux données et leurs propriétés optiques et thermiques. Dans chaque cas, les paramètres libres sont : les abondances de chaque population de grains (3 par modèle), l'intensité du champ de rayonnement incident, et une composante stellaire (modélisée par un corps noir), soit au moins 5 degrés de liberté. Chaque spectre est intégré dans les mêmes bandes photométriques que les observations, 2011.