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Given that we are observing at a non-standard broadband filter, we need to instruct the OpticalTrain to adjust the PSF strehl ratio. This is done with the !INST.psf dictionary.
MICADO_Sci however, does use AnisocadoConstPSF, and I suppose there the parameter would be taken into account (didn't check).
The notebooks have an instructional purpose, so maybe it is best to resolve this in a way that does actually make the strehl ratio relevant. If the comment in notebook 2 is right, that "we need to adjust the PSF strehl ratio because we are observing at a non-standard broadband filter", then the best course of action might be to copy the example in the FAQ notebook to notebook 2.
Various of the MICADO notebooks set the Strehl ratio.
E.g. https://github.com/AstarVienna/irdb/blob/dev_master/MICADO/docs/example_notebooks/2_scopesim_SCAO_1.5mas_astrometry.ipynb
However, MICADO uses a FieldConstantPSF as PSF, which does not use this parameter. The AnisocadoConstPSF does use the Strehl ratio, and is described in the FAQ https://github.com/AstarVienna/irdb/blob/dev_master/MICADO/docs/example_notebooks/MICADO_FAQs.ipynb
MICADO_Sci however, does use AnisocadoConstPSF, and I suppose there the parameter would be taken into account (didn't check).
The notebooks have an instructional purpose, so maybe it is best to resolve this in a way that does actually make the strehl ratio relevant. If the comment in notebook 2 is right, that "we need to adjust the PSF strehl ratio because we are observing at a non-standard broadband filter", then the best course of action might be to copy the example in the FAQ notebook to notebook 2.
The example in the MICADO FAQ:
Thoughts @astronomyk / @oczoske ?
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