2026-07-072026-07-07http://salesiana.dossiersoluciones.com/handle/123456789/117188We examine new methods of producing and analyzing the empirical initial-final mass relation for open cluster white dwarfs (WDs). We re-determine initial and final masses for the complete sample of published cluster WDs and then pare this sample using stringent criteria. We create an empirical initial-final mass relation by binning all WDs in individual clusters to a single point. Despite potentially significant systematics arising from this approach, we are comfortable concluding that, to within current observational constraints, the initial-final mass relation is linear, any intrinsic scatter in the relation is <~0.05 solar masses, and there is no metallicity dependence. More exploration of these issues is clearly warranted.6 pages, 2 figures, uses included style file, for publication in the proceedings of the 15th European White Dwarf Workshop. Corrected version fixes a typo that kept a reference from appearing properlyAstrophysicstext