Fig. 19.
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Completeness calculated based on objects from the KYSO, SPICY, M19, and G19 catalogues as a function of Planck dust opacity (τ) and the absolute median Gaia G band magnitude. Colour coding presents the fraction of objects that are in any of the mentioned catalogues and also in the Gaia DR3 YSO sample in 5 × 10−5 × 0.25 mag size bins on a logarithmic scale.
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