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Fig. 12


Overview of the influence of the exposure time (: black bar, 2 h: transparent bar, 8 h: gray bar) and wavelength on the feasibility of detecting a gap in the disk. The underlying model contains all simulations (all disk masses, sizes, and stellar types) for a hydrodynamical simulation (SP1) with a planet (η = 0.001) and large dust grains. The observing probability is normalized to the maximum at 430 μm and an exposure time of 2 h.

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