NuGrid stellar data set I. Stellar yields from H to Bi for stars with metallicities Z = 0.02 and Z = 0.01

Understand

We provide a set of stellar evolution and nucleosynthesis calculations that applies established physics assumptions simultaneously to low- and intermediate-mass and massive star models.

• Our goal is to provide an internally consistent and comprehensive nuclear production and yield data base for applications in areas such as pre-solar grain studies.
• Our non-rotating models assume convective boundary mixing where it has been adopted before.
• We include 8 (12) initial masses for $Z = 0.01$ ($0.02$).