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This is in part also to track how we want to expose the corona to disc part of Gradus modelling to the end user.
If we can get it fast enough, we can trace the disc emissivity functions directly when fitting (maybe using automated caching or similar) instead of pre-computing more tables.
The text was updated successfully, but these errors were encountered:
This is in part also to track how we want to expose the corona to disc part of Gradus modelling to the end user.
If we can get it fast enough, we can trace the disc emissivity functions directly when fitting (maybe using automated caching or similar) instead of pre-computing more tables.
The text was updated successfully, but these errors were encountered: