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.
This figure is made of several images, please see below:
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