Frank L. H. Wolfs
Department of Physics and Astronomy, University of Rochester
Conclusions and concerns
¥The data for both TOF and T0 look good.  The critical change that was made in the RHIC operation that changed the TOF from a BLM to a good detector was the reduction in background.
¥It will need 1 - 2 weeks before the TOF and T0 calibration procedures are finalized, and it would be bad if DV was frozen before then.  Note that none of the Au - Au calibration procedures work at the moment due to changes in triggering and changes in multiplicities.
¥Can we keep time calibrator events in the PhoHit files?  We need to get more experience with how to correct the data collected on the fly.