Frank L. H. Wolfs
Department of Physics and Astronomy, University of Rochester
Summary
¥Time-delay calibrations require not a simple overall shift.

¥We need to address the need to apply gain corrections too.

¥The T0 can in principle be calibrated directly based on the prompt peak, as was done in PR01, but for the TOF we do not have a choice but to use the time calibrator procedure.

¥Tracking works fine, and background does not appear to be an issue.
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¥We are currently producing required DSTs for our TOF studies.