Evolution of the SFR of the target galaxy (as a solid red line). The best fit of the evolution obtained from the CEERS (Cole et al. 2025) – which explicitly excluded sources potentially contaminated by AGNs – and the GLASS (Calabrò et al. 2024) surveys are shown below z ≃ 9 as dot-dashed green and dashed turquoise lines, respectively. We also report the 1σ scatter as shaded areas, following the same colour scheme. The dotted purple line corresponds instead to the best fit to the empirical model by Behroozi et al. (2013).