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

Le résumé fourni par la source

This is a correction to Bellstedt et al. (2024), ammending the stated dust parameters presented in tables 2, 3, and 4. Specifically, the |$\tau _{\rm birth}$| and |$\tau _{\rm screen}$| values in tables 2, 3, and 4 were erroneously swapped for each component. The updated rows in each of the original columns are provided in Tables 1, 2, and 3. These updates do not affect any other aspect of the original paper, and reflect the settings used to generate the original results. Updated |$\tau$| parameters from table 2 in Bellstedt et al. (2024). Updated |$\tau$| parameters from table 2 in Bellstedt et al. (2024). Updated |$\tau$| parameters fitted from table 3 in Bellstedt et al. (2024). Updated |$\tau$| parameters fitted from table 3 in Bellstedt et al. (2024). Updated |$\tau$| parameters fitted from table 4 in Bellstedt et al. (2024). Updated |$\tau$| parameters fitted from table 4 in Bellstedt et al. (2024).

Ce résumé expose les affirmations des auteurs. BNTIC ne l’interprète pas comme une validation indépendante des résultats.