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Fig. A.2


Subsample of stars with fluxes available at λ  ≥  0.35 mm (log ν [GHz]  ≤  2.9, see Table A.3). The best graybody fits yielding the indicated values for tD and β are shown. Fluxes at λ ≤ 2.0 mm (log ν [GHz]  ≥  2.1) are weighted stronger in the fits.

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