Fig. A.2
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SEDs for the five exozodi candidates. The red dots represent the observed photometry in the NIR and IR bands (J,H,Ks, W1,W2,W3 and W4). The inverted yellow triangles indicate upper limits, which are not used for the fitting. The blue dots represent the best-fit photospheric model flux, with the theoretical spectrum plotted behind it in gray.
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