Index: /trunk/ICRC_01/mccontrib.tex
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--- /trunk/ICRC_01/mccontrib.tex	(revision 812)
+++ /trunk/ICRC_01/mccontrib.tex	(revision 813)
@@ -330,8 +330,8 @@
 photons in the camera plane are needed to trigger the Telescope. 
 And it helps the low energy showers to fulfil the required trigger 
-conditions. In figure 3 one can see that the threshold energy decreases 
-while lowering the discriminator. It is 25 GeV for 3 mV and 105 GeV 
-for 7 mV. Since one of the aims of the Telescope is lowering as much 
-as possible the energy threshold, a low discriminator value is 
+conditions. In figure  \ref{fig_enerthres} one can see that the threshold 
+energy decreases  while lowering the discriminator. It is 25 GeV for 3 mV 
+and 105 GeV  for 7 mV. Since one of the aims of the Telescope is lowering as 
+much as possible the energy threshold, a low discriminator value is 
 preferred. But for 3 mV the expected rate due to protons increases a 
 lot (see section 3.1.3), while it keeps under control at 4 mV.