SED fits for our NIR excess sources. NX Pup is omitted as it has been previously modelled (see text). The filled circles are the observed fluxes and the triangles mark the fluxes where there is only an upper limit. The solid line marks the best fit, and the grey lines shows fits with per each data point. The dashed line indicates the unreddened SED of the stellar photosphere of central source in the best fitting model.
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