Correction to: Resolving cosmic star formation histories of present-day bulges, discs, and spheroids with P ro F use.

This document is a correction to a previous article by Bellstedt et al. regarding the cosmic star formation histories of bulges, discs, and spheroids in galaxies. The correction addresses an error in the dust parameters presented in tables 2, 3, and 4 of the original paper. Specifically, the |$\\tau _{\\rm birth}$| and |$\\tau _{\\rm screen}$| values were mistakenly swapped for each component. The corrected values are provided in updated tables 1, 2, and 3. These corrections do not impact any other aspect of the original paper and reflect the settings used to generate the original results. [Extracted from the article]