Frank L. H. Wolfs
Department of Physics and Astronomy, University of Rochester
d + Au: PR03
¥Status:

¥All required modifications to the software have been made.

¥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.