Comparison of CIGALE fluxes to those measured with LiMe (Fernández et al. 2024). The full results on the CEERS catalogue redshifts and line measurements will be discussed in Arrabal Haro et al. (in preparation). The points corresponding to each emission line are colour-coded to better identify each species (see inside caption). AGN lines are identified by crosses. The most ultraviolet lines (CIV λ1549 Å and HeII λ1641 Å in the lower part of the plot) are not in agreement with those estimated by LiMe as shown by the offset from the solid 1-to-1 line. Instead, we find that other lines are systematically different by about about 20% (dashed line). The observed difference might find an origin in the subtraction of the continuum.