Frank L. H. Wolfs
Department of Physics and Astronomy, University of Rochester
T0 studies
Summary
¥As of yet, the source of the correlations has not been identified.
¥This is what we know:
¥No problems for Au + Au
¥No problems for beam-gas events
¥Correlations for d Au collisions
¥Correlations are not present in the MC data
¥What do these observations have in common?
¥Events with a large number of primaries look OK
¥Events for which there is significant probability of seeing no primaries show correlations.
¥What are we going to do?
¥In parallel to continuing studies of the data collected, a number of experts are looking at the hardware.
¥I plan to switching to TOF integration next week, using the collision time of the ORs to correct for the START jitter.