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Fig. C.1

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SEDs of YSO candidates with well-fitted Robitaille (2017) YSO models. The best-fit model is indicated with the black solid line. Gray lines show the YSO models with χ2 between and , where n is the number of data points and F is a threshold parameter which we set to 3 (Sewiło et al. 2019). Filled circles and triangles are valid flux values and flux upper limits, respectively. The values of a reduced χ2 and interstellar visual extinction for the best-fit model are indicated in the plots.

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