SVP data and codes
These data (for C, N, O, Ne, Na, Mg, Al, Si, S, Ar, Ca and Fe) and codes have been released in 2020, and are discussed by Alecian & LeBlanc, 2020 (MNRAS, in press).
Instructions to use the codes and data (content of the READme file).
To install the standalone code with the data needed to compute radiative accelerations, download the following file:
The figures showing calculated radiative accelerations for all elements and all models mentionned in Alecian & LeBlanc (2020), are gathered in the following tar.gz:
This package includes the codes and data necessary for the implementation of the SVP method in stellar evolution programs.
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Update: August 2020