I talked with Kawanomoto-san a bit about his models and it seems to me that his code has flexibility to provide data in any format, so if we want to compare with his model, please specify what values we need in what format.

Would csv be fine ?
I'm mostly interested in two things :
one is the non-uniformity of the pupil illumination for PFS which can be confirmed hopefully using twilight data.
The other would be his model regarding the dot penumbra itself, I did see figures on some slides, but I don't how complex is the model, does it vary wrt the position on the pfi ?

I guess csv format should be possible and I think his model is a function of position of PFI focal plane, but I heard that his model is a bit simplified (e.g. axial symmetry on the focal plane is assumed, obscuration by PFI and telescope spiders is not included, and so on...), so not sure if it's fully useful. Anyway, I think I should invite Kawanomoto Satoshi (not sure if this is notified) here and start the coordination.

I've added my draft pdf report and also the list of visits I've used.

I'm closing this ticket now, I'll open new one for further actions :
comparing with Kawanomoto-san model ... etc