Frank L. H. Wolfs
Department of
Physics and Astronomy, University of Rochester
TOF Energy
¥Using
the last calibration parameters of PR01, we gain-matched the PMTs and
reconstructed the TOF energy based on the measured pulse heights.
¥The
calibration is in terms of MIPS, but the calibration parameters depend on the
average angle of incidence, which is a function of position/orientation of the
walls and the field.
