Mass-age relation for star clusters. The hollow-green circles correspond to the heterogeneous compilation from Baumgardt et al. (2013, and references therein) for LMC star clusters. The hollow-purple squares show a similar compilation for the SMC, from Bica et al. (2022, and references therein). The hollow-orange diamonds refer to the characterization of Bridge clusters by Oliveira et al. (2023). The result for SL 2 from this work using PARSEC-COLIBRI isochrones is highlighted in the figure. The two black-dashed lines show the ages of 4 and 10 Gyr (the same as shown in Fig. 2), serving as limit indicators of the age gap.