Dear
astrometry.net community,
I have very narrow band of images for which I am trying to solve the pattern (roughly 0.1deg x 1deg).
Looking at the documentation for the available database indexes, I feel like I might need to build custom indexes with skymark diameters even smaller than xx00 series (2-2.8arcmin).
In your experience, would you agree with the above? Would you have an order of magnitude of how small the skymark diameter needs to be with regard to the shorter field-of-view side?
Thank you so much in advance!
Regards,
Aaron