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Atomic abundances are entered relative to solar abundances as defined in [Grevesse, Noels and Sauval 1996], with $1.0$ being defined as the solar value and the current default. Currently supported range for these values is $(0.0 \ldots 100.0)$.

The atomic species are all elements up to and including copper (Z=30). Note that as of version 2.2.0 many of these are treated using scaled hydrogenic atomic rate data.

Tim Kallman 2018-12-14