Fig. A.1.
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SED for DFK 52, including total ALMA flux measured in this work. Archival photometric measurements were corrected for foreground interstellar extinction by the same amounts as Humphreys et al. (2020). The lines are shown denoting the stellar blackbody (dashed red) as well as a spectral index of 3 extrapolated from the ALMA point (dotted green).
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