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Hi Jeroen, thanks for this suggestion.
I looked at this grid in the past. They do not provide intensities, but only disk-integrated fluxes.
Therefore, it cannot be used for limb-darkening calculations.
Would it still be useful for you?
Hi, this is quite a surprise. Sorry for the delay in answering, as I have been busy.
I will try to revise these files next week and/or to include an option to use a database provided by the user.
Would it be possible to implement the model grid calculated by Husser et al 2013:
https://ui.adsabs.harvard.edu/abs/2013A%26A...553A...6H/abstract
This grid should also cover the mid-IR and low temperature stars,
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