Extended Data Fig. 6: SPHERE detection limits.
From: Evidence for a sub-Jovian planet in the young TWA 7 disk

Contrast 5-sigma confidence level curves of the SPHERE observation used to compute the upper limits on the candidate companion flux.
From: Evidence for a sub-Jovian planet in the young TWA 7 disk

Contrast 5-sigma confidence level curves of the SPHERE observation used to compute the upper limits on the candidate companion flux.