Hi Sander,
I realise that - and that was why I wondered if a 'false image' made up from star locations and magnitudes (extracted from a suitable star catalogue) could be used as the 'reference' frame in the Star Alignment process - in much the same way as you would do 'astrometry' in the likes of AIP4WIN, etc.
Then, once all your 'real' images were aligned to the 'false reference', you would just dump the reference frame prior to stacking.
In my mind, and with a very simplistic analysis, the 'perfect' stars from the 'star catalogue' at least give PI a good 'head start' for trying to locate the same stars in the 'real' images. But, perhaps I haven't fully thought this through - maybe I am missing something 'obvious' here. It wouldn't be the first time

Cheers,