Frank L. H. Wolfs
Department of
Physics and Astronomy, University of Rochester
Up to TOF PID. What
is needed?
¥PR03 TOF DV (especially the time calibration data)
included in the DV process.
¥Generate track DSTs (on a sequence by sequence basis)
to be able to apply TOF and T0 calibrations on a sequence-by-sequence
basis.
¥Sufficient TOF tracks to optimize the slewing
corrections for each scintillator (detailed numbers presented on the next
slide).