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Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

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Compton Kinematics studies and simulation results Paola Solevi 04/11/2009
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Page 1: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Compton Kinematics studies and simulation results

Paola Solevi04/11/2009

Page 2: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Energy distribution

- Run 1665, HL on trigger turned off.- Calibration with 1680 (ET) and 1681 (IT).

1 LYSO only selected. Small tagger guarantees low energy hit are focused at the centre of the module.

Page 3: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

General cluster overview with no selection

pp+63 keV

Page 4: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Cluster selection: amplitude [I]

By requiring only 1 cluster on the same layer of the fired LYSO (1 LYSO selected).

Run 01665

Selection for different energy ranges.

Page 5: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Cluster selection: amplitude [II]

By selecting all clusters whose amplitude is larger than a certain threshold (thres = 150 adc cnts * E1/Eme).

Run 01665

Selection for different energy ranges.

Page 6: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Cluster selection: # wls [I]

By requiring only 1 cluster on the same layer of the fired LYSO (1 LYSO selected).

Run 01665

Selection for different energy ranges.

Page 7: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Cluster selection: # wls [II]

By selecting all clusters whose amplitude is larger than a certain threshold (thres = 150 adc cnts * E1/Eme).

Run 01665

Selection for different energy ranges.

Page 8: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Cluster selection: # cluster [I]

By selecting all clusters whose amplitude is larger than a certain threshold (thres = 150 adc cnts * E1/Eme).

Run 01665

Selection for different energy ranges.

Page 9: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Energy distribution

Investigation of the reconstructed z coordinated for different energy ranges.

Run

0166

5

z coordinate for 1 LYSO fired, in different energy ranges, using WLS in cluster selected by Ncluster =1. The shown distribution are obtained by selecting events on layer 6.

The larger is the energy, more WLS are fired and the reconstructed z gets continuous.

Increasing energy

Page 10: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Efficiency study

Investigation of the efficiency of the cluster selection criteria.Ru

n 01

665

Energy[keV]

# events # clusters #cluster after

selection 1

# cluster after

selection 2

Ratio I/II

50-100 8843 1608 1590 1592 99.8

100-150 12195 6434 6274 5993 104.7

150-200 13911 11426 10846 9825 110.4

200-250 11221 10658 9679 9097 106.4

250-300 8544 8603 7392 7444 99.3

300-350 8606 8974 7218 7778 92.8

350-400 5281 5582 4069 4645 87.6

400-450 16924 20704 12802 16323 78.4

450-500 51285 65541 36870 49811 74.0

500-550 1657 2128 1008 1471 68.5

Page 11: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Studying WLS cluster for different WLS thresholdsRun 01665

Dependence on the WLS thr of the number of events with no WLS fired.

Different thresholds have been applied at WLS level: (20), 30, 40, 50 and 60 adc counts.

Page 12: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Run 01665

50-100

Cluster selection: amplitude [I]

30 adc cnts 40 adc cnts 50 adc cnts 60 adc cnts

150-150

150-200

200-250

250-300

300-350

350-400

400-450

450-500

500-550

Page 13: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Run 01665

50-100

Cluster selection: amplitude [II]

30 adc cnts 40 adc cnts 50 adc cnts 60 adc cnts

150-150

150-200

200-250

250-300

300-350

350-400

400-450

450-500

500-550

Ratio bin to bin of cluster selected with and without a threshold applied.

Page 14: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Run 01665

Dependence on the WLS thr of the size of cluster in different energy ranges.

Cluster selection: # wls

30 adc cnts 40 adc cnts 50 adc cnts 60 adc cnts

50-100

150-150

150-200

200-250

250-300

300-350

350-400

400-450

450-500

500-550

Page 15: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Run 01665

Dependence on the WLS thr of the number of cluster in different energy ranges.

Cluster selection: # cluster

30 adc cnts 40 adc cnts 50 adc cnts 60 adc cnts

50-100

150-150

150-200

200-250

250-300

300-350

350-400

400-450

450-500

500-550

Page 16: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Run 01665Study of cluster multiplicity

30 adc40 adc50 adc60 adc

0 cluster

1 cluster

2 cluster

Page 17: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

“Cleaned up” simulation: LYSO (Lu = 72%) [1]

I cleaned the source code from all changes done and the agreement with data is eventually good! Now changes have to be re-implemented by comparing data and simulation step after step.

- Small shift due to the calibration.- 63 keV is a bit under-estimated.

Page 18: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

“Cleaned up” simulation: LYSO (Lu = 72%) [2]

Page 19: Compton Kinematics studies and simulation results Paola Solevi 04/11/2009.

Understanding the intrinsic radioactivity spectrum

Energy in LYSO with energy blurring: only 300, 200 and 63 keV peaks are visible.

Υ3

Υ3-Kα

Υ2-Kα

Υ2

Υ1


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