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Fig. 3

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SED of V892 Tau measured from ALMA and VLA observations. The fluxes of the inner and outer discs are represented by the blue and green points, respectively. Our best-fit power-laws and their corresponding spectral index are represented by plain orange lines between 0.9 mm and 3.0 mm (i.e. 100-333 GHz), and in black between 3.0 mm and 9.8 mm (i.e. 30.5-100 GHz). αin and αout are the spectral indices of the inner and outer discs, respectively. The error bars for the outer disc are smaller than the markers at wavelengths shorter than 3.0 mm.

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