Spectral energy distributions of point sources in the BRC12 field. We used the SED fitting-tool of ROB07. The filled circles represent the input fluxes and the black line shows the best fit. The grey lines show subsequent fits, all corresponding to χ² − χ²(best) per data point  ≤3. The dashed line shows the stellar photosphere corresponding to the central source of the best fitting model, as it would look in the absence of circumstellar dust, but including interstellar extinction.