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Fig. 8.


Synthetic images of the two-belts model with an inner belt coplanar with the outer belt. The model parameters are the same as in the model shown in Fig. 7 except for the inclination and PA of the inner belt which are the same as for the outer belt. Panel a: model before convolution with the PSF. Panel b: model after processing with the KLIP algorithm. The flux is shown in arbitrary units.

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