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Fig. A.1


SEDs of the stars in the sample. Triangles are photometric upper limits. For each panel, the best fit is the black-solid line and the models fitting with are the grey-solid lines, where n is the number of datapoints per star (see Robitaille et al. 2007). The best stellar (de-redenned) photosphere is indicated with a dashed line.

This figure is made of several images, please see below:

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