Jan 31 2026: APP 2.0.0-beta40 will soon be released with many fixes especially for Linux, upgraded development platform and 10-20% performance boost !
Jan 15 2026: FIXED LICENSE SERVER VPN Tunnel issue
 The issue could have prevented APP to start when using a VPN tunnel or another complicated network configuration, like using APP on a remote computer on a different continent. This issue is fixed now and APP should start normally.
Jan 04 2026: Update on the 2.0.0 release & the full manual
We are getting close to the 2.0.0 stable release and the full manual. The manual will soon become available on the website and also in PDF format. Both versions will be identical and once released, will start to follow the APP release cycle and thus will stay up-to-date to the latest APP version. Unfortunately, Mabula was struck by a severe flu virus in the past couple of weeks and thus could not work. He is getting much better now and he has resumed work to release 2.0.0 as soon as possible. Once 2.0.0 is released, the price for APP will increase. Owner's license holders will not need to pay an upgrade fee to use 2.0.0, neither do Renter's license holders.
Nov 28 2025:Â APP 2.0.0-beta39 has been released !
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.
