Fig. B.1.
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SED models obtained with the GalaPy software for the sources studied in this work (see Appendix A). Points correspond to the photometric measurements obtained from the VizieR photometry viewer (see Appendix B), while solid lines correspond to the unattenuated stellar emission (green), molecular cloud component (MC, purple), stellar emission considering extinction (extinct, red), and diffuse dust (DD, yellow).
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