SFH model corresponding to the analysis in Fig. 9, but for region 2 of warhol, as it is characterized by Palencia et al. (2025). Again, the inclusion of B/R ratio as a model constraint on top of the SED predicts a different SFH. The disagreement between the two solutions of SFH when the B/R ratio is incorporated as a constraint, however, is more drastic in the case confined to region 2 than in the case for the whole Warhol arc. This demonstrates the spatial variation of the SFH in the lensed galaxy, and the constraining power of B/R at different regions.