SSD beamtest analysis Stphane Plumeri Institut de Recherches Subatomiques IReS, Strasbourg - PowerPoint PPT Presentation

1 / 12
About This Presentation
Title:

SSD beamtest analysis Stphane Plumeri Institut de Recherches Subatomiques IReS, Strasbourg

Description:

SSD beamtest analysis. St phane Plumeri. Institut de Recherches Subatomiques (IReS) ... Noise, pedestal and common mode shift. Signal and signal to noise ratio ... – PowerPoint PPT presentation

Number of Views:42
Avg rating:3.0/5.0
Slides: 13
Provided by: splu
Category:

less

Transcript and Presenter's Notes

Title: SSD beamtest analysis Stphane Plumeri Institut de Recherches Subatomiques IReS, Strasbourg


1
SSD beamtest analysis Stéphane Plumeri
Institut de Recherches Subatomiques (IReS),
Strasbourg
ALICE collaboration
  • ITS week 20 23 October 2003

2
Outlook
  • StripTracking software
  • Noise, pedestal and common mode shift
  • Signal and signal to noise ratio
  • Cluster shape
  • Charge matching
  • Conclusion

3
StripTracking software
  • Authored by Dirk Meier at CERN (1997)
  • and modified by J. Baudot, C. Suire and S.Plumeri
    (IReS)
  • for STAR and ALICE SSD beamtests.
  • StripTracking is a C program linked with root
    libraries
  • StripTracking can
  • Measure noise and pedestal
  • Find hits
  • Correlate hits on each side

4
Noise
ITCs modules Module 3 357 e- P side 573 e-
N side Module 4 365 e- P side 573 e- N side
Canberras modules Module 1 440 e- P side
1458 e- N side Module 2 415 e- P side 1369 e-
N side
For each module V 45V
5
Pedestal
Pedestal mean value of charge over the run
2100 2200 ADC counts for all modules Nearly the
same for N and P side
6
Common mode shift
Standard deviation of cms distribution over
events, with
Seems to increase with distance from power supply
7
Signal
Charge in clusters (threshold seed strip S/Ngt5
neighboors S/Ngt3 )
8
Signal
Charge in clusters (Correlation between two sides
and geometrical cut)
9
Signal to noise ratio
Problem on canberras module N side
10
Cluster shape
Bad results on canberras N side
11
Charge matching
Default on ITCs module maybe due to noisy
strips ?
12
Conclusion
  • Good modules performances
  • But
  • Origin of high cms?
  • Too much noise on N side of canberras module
  • Next step Tracking
Write a Comment
User Comments (0)
About PowerShow.com