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Set 1

Baseline yields with standard physics assumptions.


Yields tables


The Set 1 yield tables are provided at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1/Yield_tables.
Set 1 extension yield tables together with a README file are provided at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1ext/Yield_tables
 Documentation of how to extract table data can be found in Analysis of yield tables

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Stellar evolution and nucleosynthesis post-processing output


Directory structure for each metallicity on the CADC data server:

see_wind
Stellar evolution (pre-SN = wind) data
see_exp Explosion data
ppd_wind Post-processing of see_wind data
ppd_exp Post-processing of see_exp

Set 1 extension (Ritter et al. 2017)

For Z=0.02 stellar evolution data and post-processing data can be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1ext/set1.2

For Z=0.01 stellar evolution data and post-processing data can in be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1ext/set1.1

For Z=0.006 stellar evolution data and post-processing data  can in be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1ext/set1.3a

For Z=0.001 stellar evolution data and post-processing data can in be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1ext/set1.4a

For  Z=0.0001 stellar evolution data and post-processing data can in be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1ext/set1.5a


Set 1 (Pignatari et al. 2016, ApJS)

For Z=0.02 stellar evolution data and post-processing data can in be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1/set1.2

For Z=0.01 stellar evolution data and post-processing data can in be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1/set1.1


Figures


Figures of Set 1 can be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1/Figures.

Figures of Set 1 extension can be found at http://www.canfar.phys.uvic.ca/vosui/#/nugrid/data/set1ext/Figures.



Acknowledgement

NuGrid acknowledges significant and sustained support by and collaboration with JINA and JINA-CEE. RH acknowledges support from the World Premier International Research Center Initiative (WPI Initiative), MEXT, Japan and funding from the European Research Council under the European Union's Seventh Framework Programme (FP/2007-2013) / ERC Grant Agreement n. 306901.



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