  Type Ia supernova explosions (SNIa) are fundamental sources of elements for
the chemical evolution of galaxies. They efficiently produce intermediate-mass
(with Z between 11 and 20) and iron group elements - for example, about 70% of
the solar iron is expected to be made by SNIa. In this work, we calculate
complete abundance yields for 39 models of SNIa explosions, based on three
progenitors - a 1.4M deflagration detonation model, a 1.0 double detonation
model and a 0.8 M double detonation model - and 13 metallicities, with 22Ne
mass fractions of 0, 1x10-7, 1x10-6, 1x10-5, 1x10-4, 1x10-3, 2x10-3, 5x10-3,
1x10-2, 1.4x10-2, 5x10-2, and 0.1 respectively. Nucleosynthesis calculations
are done using the NuGrid suite of codes, using a consistent nuclear reaction
network between the models. Complete tables with yields and production factors
are provided online at Zenodo: Yields. We discuss the main properties of our
yields in the light of the present understanding of SNIa nucleosynthesis,
depending on different progenitor mass and composition. Finally, we compare our
results with a number of relevant models from the literature.
