UPDATE FROM MABULA
I have had a very rough 2 months unfortunately health wise. I was struck 3x in a row with bacterial infections. The second infection occurred  after a routine hospital checkup and I became very sick. I had to rest and take a lot of antibiotics. Once I was recovering and restarting work 1 month ago, I again became sick. The infection was not yet gone, so even more antibiotics and rest was needed. Needless to say, it took a lot of my energy and I needed a lot of rest.
Finally, the infection is really gone and my energy is coming back step-by-step now and I have started work again. I am terribly sorry to have kept you waiting for support. I will address all outstanding questions and e-mails step-by step and will be on the forum daily from today.
APP 2.0.0-beta47 will come soon as well, a lot of work was already completed before I became very ill, so the release is also nearly ready for you. Beta47 will be much faster actually. Many workflows will be more than 2x faster, mosaics can even be 10x faster than before because registration really received a major boost... all compared to beta46. Â Before I release it, I will make sure that everything is working properly and then I will release it.
Attached is a stack of 55 images of comet C/2019 L3 ATLAS from two nights ago.
I used 1-star registration, and also local normalized rejection during integration.
Note that the faintest background stars are trailed, which makes sense because the 1-star registration data showed that the comet drifted about five pixels (in the X direction, zero rate in Y direction) during the imaging run. But the brighter stars are not trailed at all.
I presume this is a feature of local normalized rejection?...it is only invoked above a certain threshold that is defined by the local background level?
Anyway, I just wanted to share this result. (When I first looked at the image I knew something was different, but it took me a bit of time to realize the difference in bright/faint stars that did/didn't trail.)
But the brighter stars are not trailed at all.
It is difficult to see with such a strongly compressed image, but the bright stars are trailed as well. Compared to the displayed size of the stars, however, the trailing of the bright stars is much less noticeable than that of the faint stars.
