Open Access

Fig. 7


Fluxdensity distribution for a typical DEB target (HD 203, cf. Fig. 6). Photometric data are shown as red circles, and the Spitzer IRS spectrum is shown as a black solid line with uncertainties in grey. The best-fit model (orange line) has stellar (blue) and blackbody (green, for the DEB) components (see Sect. 3.3 for details).

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