Dust entrainment in photoevaporative winds: Synthetic observations of transition disks

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Fig. B.7

Synthesised instrument response for TD20 for SPHERE IRDIS in J-band, assuming a reduction of the instrument noise by a factor of 10; all else equal to Fig. 15. In contrast to said Fig. 15, there are visible differences between the ‘wind’ and ‘no wind’ models, for both fixTD20 and varTD20.

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