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Fig. 8

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Left panels: fits to stellar-subtracted spectra of HD 69830 and HD 113766 A (top and bottom, respectively), without Fe-rich olivine grains. Right panels: same as left panels including Fe-rich olivine grains in the modelling. For each panel, residuals are shown at the bottom (see Sect. 5).

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

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