DA white dwarfs are characterized by a surface composition that consists almost entirely of H with at most traces of other elements. They comprise about 85% of all white dwarfs. Below, we provide links to a complete set of evolutionary (including colors and magnitudes) and pulsational computations of our DA white dwarf models. Our calculations cover a wide mass range. In order to make easier the search for a given set of computations, the files are classified into three categories according to the core chemical composition of the star:

He-core white dwarfs

CO-core white dwarfs

ONe-core white dwarfs


Periods and chemical profiles for asteroseismology


In addition, we provide colors and magnitudes for H-rich white dwarfs: colors and magnitudes