Fig. 9
Magnitude and mass limits (5σ) up to 1′′ around Wray 15-788. The positions of the two rings and the gap are indicated in blue and gray, respectively. The magnitude contrast was converted to an upper mass limit by AMES-Cond models for 11 Myr old objects. Inside the gap we are sensitive to companions as massive as 10 Mjup (H band) and 15 Mjup (Ks band).
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