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Timestamp:
05/29/01 17:14:26 (23 years ago)
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blanch
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  • trunk/ICRC_01/mccontrib.tex

    r811 r813  
    330330photons in the camera plane are needed to trigger the Telescope.
    331331And it helps the low energy showers to fulfil the required trigger
    332 conditions. In figure 3 one can see that the threshold energy decreases
    333 while lowering the discriminator. It is 25 GeV for 3 mV and 105 GeV
    334 for 7 mV. Since one of the aims of the Telescope is lowering as much
    335 as possible the energy threshold, a low discriminator value is
     332conditions. In figure  \ref{fig_enerthres} one can see that the threshold
     333energy decreases  while lowering the discriminator. It is 25 GeV for 3 mV
     334and 105 GeV  for 7 mV. Since one of the aims of the Telescope is lowering as
     335much as possible the energy threshold, a low discriminator value is
    336336preferred. But for 3 mV the expected rate due to protons increases a
    337337lot (see section 3.1.3), while it keeps under control at 4 mV.
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