The impact of the white dwarf initial-final mass relation on star clusters' ages inferred from their cooling sequence
This study quantifies how the choice of white dwarf initial-final mass relations introduces systematic uncertainties in star cluster age determinations, finding that while the impact is negligible for young clusters, it can cause age offsets of up to 0.6 Gyr for intermediate-age clusters and up to 0.8 Gyr for old, metal-poor clusters if metallicity dependence is neglected.