- Timestamp:
- 05/31/01 08:52:48 (23 years ago)
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trunk/ICRC_01/mccontrib.tex
r821 r823 393 393 background rate (protons and light of night sky) is $396 \pm 88$ Hz. 394 394 395 It has been also studied the effect on the trigger rate ofthe discriminator396 threshold (see figure \ref{fig_rates}). The trigger rate decreases397 with increasing discriminator threshold. Notice that the expected rate398 for the discriminator value at 3 mV is more than 100 times larger than399 for the other values. 400 395 The dependence of the first level trigger rate from the discriminator 396 threshold is shown in figure \ref{fig_rates}. 397 The trigger rate decreases 398 with increasing discriminator threshold as expected. 399 The rate for the discriminator threshold of 3 mV is more than 100 400 times larger than for the other values. 401 401 \begin{figure}[hb] 402 402 \vspace*{2.0mm} % just in case for shifting the figure slightly down … … 407 407 \end{figure} 408 408 409 These results show that the MAGIC telesope will use a disriminator 410 threshold of about 4 mV. This value corresponds to a threshold of 411 about 8 photo electrons. 412 413 It has to be mentioned here, that all the results here are based on 414 the first level trigger. There is a big potiential to optimize the 415 settings here. I.e. the background rate can be reduced by 416 increasing the discriminator threshold for a few dedicated pixels, 417 that have a star in their field of view. Studies in this direction are 418 ongoing and will be presented on the conference. 409 419 410 420 \section{Conclusion} 421 422 We presented the actual status of Monte Carlo simulation for the MAGIC 423 telescope. 424 411 425 412 426 \begin{acknowledgements}
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