Hi all! I have a quick question regarding the Solar System Processing Pipeline and how HelioLinC3D will be implemented going forward. I have been experimenting with HelioLinC on some simulated data I generated using Sorcha, and of course in order to run HelioLinC on my tracklet file, I had to create a file containing the hypotheses about heliocentric radial motion (this is the file that is input using the -heliodist flag, as described here: GitHub - lsst-dm/heliolinc2: Solar System Processing using HelioLinC2 algorithm).
So I was just curious – during live Rubin observing, what hypothesis file(s) will be used when running HelioLinC3D? If this question is unclear, please let me know. Many thanks! 