A low noise, high gain (> 106), photon counting detector, with
fast time response (risetimes < a few ns) matched to the intrinsic
temporal width of the gamma-ray induced air shower is necessary to
increase the signal-to-noise ratio and to operate VERITAS at the
lowest possible energy threshold. These requirements are presently
satisfied only by PMTs and 25 years of experience with these devices
leads us to base the VERITAS system upon them. The focal plane will
contain 499 hexagonally packed PMTs providing an effective FoV of
.
The spacing between the PMTs corresponds to a focal
plane angular distance of
.
The active light collection
diameter of the PMTs is 25mm. The collection efficiency is
increased by the use of Winston light concentrators. Tests have
identified the Hamamatsu R7056, with a bialkali photocathode and a UV
glass window, as one PMT which satisfies our requirements.