Fig. 5
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Spectral energy distribution of the circumstellar disk around L1527. Our galario best-fit total flux of the compact Gaussian component for each band, in green, along with longer wavelength VLA measurements from Melis et al. (2011, see Table 4). The protoplanetary disk of L1527 is optically thick up to 3.4 mm (αB7−B3 ~ 2), likely due to its edge-on nature.
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