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Currently it is only possible to use the default value of the epsilon parameter for the gapfind and gapfill functions. Using the default value fails for some models that require very small fluxes to be viable.
The text was updated successfully, but these errors were encountered:
Currently it is only possible to use the default value of the epsilon parameter for the gapfind and gapfill functions. Using the default value fails for some models that require very small fluxes to be viable.
The text was updated successfully, but these errors were encountered: