That post is talking about the effort to quantify the upper limits SETI@home can set, the actual reason stated is more like that they just scanned everything they could think of and it wouldn't be very cost effective to go over things again given the probabilities involved:
> Posted Mar 2020, 21:16:23 UTC
> On March 31, the volunteer computing part of SETI@home will stop distributing work and will go into hibernation.
> We're doing this for two reasons:
> 1) Scientifically, we're at the point of diminishing returns; basically, we've analyzed all the data we need for now.
> 2) It's a lot of work for us to manage the distributed processing of data. We need to focus on completing the back-end analysis of the results we already have, and writing this up in a scientific journal paper.
https://setiathome.berkeley.edu/forum_thread.php?id=85267
Description of the final job remaining:
> The final output of Nebula is a bunch of score-ranked lists of multiplets. We already know that some fraction of these will be RFI of the sort that's apparent to a human observer, but hard to identify algorithmically. That's OK. The goal our RFI algorithms is not to remove 100% of RFI; doing so would probably remove ET signals too. The goal is to remove enough RFI that a good fraction (say, at least half) of the top-ranking multiplets are not obvious RFI.
The final (post-Nebula) stages of SETI@home are
> Manually examine the top few thousand multiplets, in all the various categories and score variants, and remove the ones that are obvious RFI. At least initially we'll do this as a group, on Zoom, to make sure we agree on what constitutes obvious RFI.
> Make a list of the multiplets that remain; re-observe those spots in the sky (hopefully using FAST), analyze the resulting data (probably using the SETI@home client running on a cluster) and see if we find detections consistent with the multiplets. If we do, maybe that's ET.
https://setiathome.berkeley.edu/forum_thread.php?id=85756