Future and Suggestions

The initial motivation for this work was to provide me with the tools toadequately model the present telescope. I now need to determine if I havesucceed. If so, this scheme could then quickly be used to model the new camerawith it smaller pixels. Further, it will be of great use in modeling the detailed response of FADC's for VERITAS.

I reiterate that this study indicates the we should be using theMultiplicity trigger for determining the timing of the ADC gate and that thetrigger fraction of the Multiplicity CFD should be set to 66%.