Frank L. H. Wolfs
Department of
Physics and Astronomy, University of Rochester
d + Au: PR03
¥The final repass of the d + Au data will
provide the required calibration information for the VME T0 Ors.
¥Current resolution is about 300 ps, but
this is based on an analysis of a series of runs ( ÉÉ ) with a single set of
calibration parameters for the T0 ORs.