JWST MIRI and NIRCam images of AT 2011kp. Panels are as follow: (a): F770W, (b): F560W, (c): F444W, (d): F335M, (e): F187N, and (f): F115W. In the MIR, a bright source is clearly visible 12.5 years after the first peak. In the top row stamps, the green circles are centred at the position of the transient and have a radius of 0.5″. In the F335M stamp, the circle has a radius of 0.3″, while in the F187N and F115W stamps it has a radius of 0.1″. The latter two stamps are more zoomed-in to better identify the counterpart.