Fig. B.1
Spectral-energy distributions of the 14 objects analysed in this paper. Light (dark) grey curves in each plot show models with P(χ2) > 32% from the best fit, considering four different SFH and fits with stellar (stellar+nebular) emission (see Sect. 3). The best-fit UV slope is shown as a blue dashed line. The bands that are not used in the SED-fitting are shown in red.
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