Complete yields for AGB and super-AGB stars for 0.02 > Z > 1.e-4

We have calculated stellar evolution tracks for AGB and super-AGB stars for masses between 1 and 8Msun and metallicities between 
Z=1e-4 and 0.02, using the MESA stellar evolution code. All tracks involve standard mass loss assumptions, convective boundary 
mixing and detailed resolution of thermal pulse-induced nuclesosynthesis, mixing and feedback, for example from the hot dredge-up 
in massive, low-Z AGB and super-AGB stars. All stellar evolution tracks have been post-processed for nucleosynthesis yields of 
all elements, using the NuGrid codes.