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The White Dwarf cooling tracks are avalaible for the following photometric systems:
UBVRIJKL
ACS HST
Sloan
Additional models of massive CO WDs (1.1 and 1.2Mo)
1.1 Mo 1.2 Mo

Oxigen profiles for the computed White Dwarf models:
Oxigen profiles

The White Dwarf cooling isochrones are available for the following heavy element distributions:

scaled-solar
Non canonical models
α - enhanced
Non canonical models