Extended Data Fig. 2: Cluster light modelled with forward modelling from the source plane.
From: Bound star clusters observed in a lensed galaxy 460 Myr after the Big Bang
Observed JWST image of Img.1 is shown (far left) along with the best fit image plane from forward modelling (left centre) and weighted fit residuals (right). Weighted residuals are calculated as (data – model)/(uncertainty).
