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- Can we easily modify the AcdV2 cuts to increase background rejection with the current reconstruction? Basically, can we optimize these cuts?
- Right now AcdV2 is using the G4 propagated covariance matrix, which really isn't right for cosmic-rays (since it uses electron hypothesis). Would changing this make an improvement?
- How do the CalOnly events look? Can we develop some rough background rejection for them?
- Obviously this will improve as the upstream reconstruction improves. Can we provide any guidance for that?
- CTs are always the after-burner to get the boosted rejection power that we need.