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Ondřej Svoboda for the ECAL group HADES collaboration meeting XXV, 19 – 23 November 2012 GSI.

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Presentation on theme: "Ondřej Svoboda for the ECAL group HADES collaboration meeting XXV, 19 – 23 November 2012 GSI."— Presentation transcript:

1 Ondřej Svoboda for the ECAL group HADES collaboration meeting XXV, 19 – 23 November 2012 GSI

2 Summary of ECAL test setup development since last collaboration meeting: -continuous delivery of new 3 inch photomultipliers (Hamamatsu R6091) -new mounting construction designed, manufactured and tested -prototype of HV divider for R6091 photomultipliers constructed and tested -one module with optical fiber and LED diode assembled and successfully tested (8/2012) -based on this 5 modules with 1.5 inch EMI 9903KB photomultipliers and 5 modules with 3 inch R6091 photomultipliers assembled, all with optical fiber -light guide system to drive all 10 modules with one diode assembled -tests of new TRB based Front-End – see talk of Behruz Kardan -first test of 3 inch photomultipliers – Yuri Sobolev 2

3 Layout of HV divider for 3 inch photomultipliers (Hamamatsu R6091) -Reason for development and manufacture of own HV divider is the price of original ones… -First tests show that the divider is comparable with the original Hamamatsu divider (same current, comparable pulse shape and amplitude from the detector). -To confirm this further tests are needed and will be done in close future. 3 Produced by CPM Jičín, CZ

4 New housing for R6091 3 inch photomultipliers 4 Magnetic shielding produced in IP Bratislava

5 Cosmics measurement 3 inch photomultiplier (Hamamatsu R6091) 1.5 inch photomultiplier (EMI 9903KB) Energy resolution: 5.9% (best case up to now) 5 Energy resolution: 5.4 % (best case) ADC (channels) For measurement used CAMDA system and shaper MA8000

6 Tests of diodes for stability monitoring of the ECAL modules Continuous search for optimal solution from many possibilities: -one diode per module, coupled to lead glass via optical Si fiber (20 cm) -different light output from each diode (+-50%) -one diode per sector, light guides to each module -how to distribute the light homogenously to each module? -which fibers, connectors will be used (question of price)? -light source to “power” all sector - common diode will be most probably weak - high power diode needs higher voltage and current – hard for 10 ns pulses - laser sources – up to now tested one for single mode fibers -red light (not ideal for photomultiplier) -slow (not able to produce 10 ns pulse of the same amplitude) -very expensive 6

7 Layout of the ECAL testing setup with LED 7

8 Light guide system for 10 modules 8 Diode with light distribution system and 10 fibers Light output from diode Fiber to lead glass transition

9 Measurement with LED diode - very fast measurement (kHz) in comparison with cosmics (~1 signal /3 minutes) - signal from pulser set to get the same detector response as from cosmics 9 3 inch photomultiplier (Hamamatsu R6091) 1.5 inch photomultiplier (EMI 9903KB) after Front-end board Yellow curve – detector output Green curve – diode input (second peak is reflection on diode)

10 Measurements made by Y. Sobolev on CAMDA system 10 Measurement with LED diode and 3 inch photomultiplier Hamamatsu R6091

11 Summary: - LED can be used for regular stability monitoring of ECAL during beamtime - basic assembly of ECAL module driven by LED diode successfully tested - search for final LED system design - new housing for R6091 3 inch detectors - first tests of own HV dividers for R6091 3 inch photomultipliers - tests of ECAL modules with both types of PMT‘s on cosmics and with LED diode performed 11

12 Thank you for your attention… 12


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