Fig. 1

Ring system simulation for the satellites from Table 1. vorb = 13.3 km s-1, b = 17% of the Hill radius, which is filled with dust out to 50% of the Hill radius. Inclination i = 18° and tilt is 37°. The red rings are filled with dust blocking 6% of incident flux, white rings are gaps cleared of dust by the moons. The grey zone in the middle is not captured by the transit. The green stripe is the path of the star behind the ring system.
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