Fig. 4
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5σ detection limits. Planet contrast (top) with respect to the star as a function of separation to the star, and planet mass detection limits (bottom) as a function of the separation from the star for the SPHERE/IRDIS_EXT data of 51 Eri b. The mass limit for the IFS data is cut to the lowest mass computed by the model grid (1 MJup) for both ANDROMEDA and TRAP.
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