Difference between revisions of "CDC Pedestal Studies"

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In the case of no signal the the distribution D is expected to be around zero with a sigma that reflects the resolution and depends on the number
 
In the case of no signal the the distribution D is expected to be around zero with a sigma that reflects the resolution and depends on the number
 
samples <math>N_{i}</math> used in determining the pedestal.
 
samples <math>N_{i}</math> used in determining the pedestal.
 +
{| class="wikitable"
 +
|-
 +
! <math>N_{i}</math> !! mean F !! sigma F !! mean I !! sigma I
 +
|-
 +
|  4 || 102.2 || 1293 || 96.5 || 1276
 +
|-
 +
| 16 || 119.0 || 1121 || 163.4 || 1120
 +
|-
 +
| 20 || 121.1 || 1080 || 145.1 || 1080
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|-
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| 32 || 102.4 ||  984 || 159.0 ||  978
 +
|-
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| 64 ||  40.9 ||  680 ||  84.6 ||  685
 +
|}

Revision as of 16:20, 23 June 2015

Pedestal Subtraction

Based on cosmic ray data with BCAL trigger Look for events with the following signature in the CDC:

  • Wave form of CDC signal

The first test was done by using the region P_{{i}} (blue) to determine a pedestal and the region I (red) to determine an Integral and then subtract the proper pedestal from the Intergral as follows: D=I-P_{{i}}/N_{{i}}*80. where N_{{i}} is the number of samples used to calculate the pedestal and 80 is the number of samples in the Integral I. In the case of no signal the the distribution D is expected to be around zero with a sigma that reflects the resolution and depends on the number samples N_{{i}} used in determining the pedestal.

N_{{i}} mean F sigma F mean I sigma I
4 102.2 1293 96.5 1276
16 119.0 1121 163.4 1120
20 121.1 1080 145.1 1080
32 102.4 984 159.0 978
64 40.9 680 84.6 685