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ZDD installation and performance

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ZDD installation and performance. BESIII Collaboration Meeting, December 2011 A. Calcaterra , for the ZDD group (LNF+TO). Talk outline. ZDD performance in Frascati, Spring 2011 Cosmic rays Single-electron beam ZDD installation, August 2011 ZDD tests with cosmic rays at IHEP, Fall 2011 - PowerPoint PPT Presentation
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ZDD installation and performance BESIII Collaboration Meeting, December 2011 A. Calcaterra, for the ZDD group (LNF+TO)
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Page 1: ZDD installation and performance

ZDD installation and performance

BESIII Collaboration Meeting, December 2011

A. Calcaterra, for the ZDD group (LNF+TO)

Page 2: ZDD installation and performance

Talk outline

• ZDD performance in Frascati, Spring 2011– Cosmic rays– Single-electron beam

• ZDD installation, August 2011• ZDD tests with cosmic rays at IHEP, Fall 2011• Outlook

– Short term– Next weeks

2011/11/30 A. Calcaterra 2

Page 3: ZDD installation and performance

The ZDD in the East area

A. Calcaterra

(2m)

ZDD: Pb/Sci.Fi Array, scintillating material 60% of total (in volume), two modules (up and down the beam) dimensions:14x4x6cm3

2011/11/30 3

γ beam axis

Fiber bundles

W screen

Gearbox for minical movement

Page 4: ZDD installation and performance

1

62

7

3

8

4

9

5

10 beam

14 cm4

cm

Each sector is sent to a PM, sectors 1&2 (6&7) are sent to the same PM (for now)

ZDD module segmentation

2011/11/30 A. Calcaterra 4

Page 5: ZDD installation and performance

One (out of two) ZDD module tested at BTF with 450, ~300, ~200 MeV e- bunches (Ne-=1,2,3)

Final Pb-scifi ZDD module, bundles guides,PM’s, TDC, at the moment not FADC but ADC caen V792N

Small scintillator (60x11x4) mm3 used to trigger and select electrons impact point

BTF test beam at LNF (may 16-22 2011)

2011/11/30 A. Calcaterra 5

Page 6: ZDD installation and performance

Setup in Cosmic rays (LNF)

2011/11/30 A. Calcaterra 6

Page 7: ZDD installation and performance

Setup in Cosmic rays

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Top “finger” scintillator, (11x5x50) mm3

Bottom “paddle” scintillator

Trigger coincidence rate = (2-3 minutes)-1

Page 8: ZDD installation and performance

Purpose of cosmic rays DAQ

• 2 types of data taking: integrated charge (QDC CAEN V792N) and lineshape (Flash ADC CAEN V1721). Timing information is also present (TDC CAEN V1190) but not systematic.

• QDC data used for:– inter-channel calibration – resolution studies– absolute scale, comparing cosmics to single-electron

• FADC data used for MeV/mV calibration

2011/11/30 A. Calcaterra 8

Page 9: ZDD installation and performance

Run 224: QDC cts for each PM

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Page 10: ZDD installation and performance

HV correction table for “up” calorimeter

Ch Ped(pC) Peak(pC) Delta(pC) G/Gref oldV newV0 15.962 38.968 46.011 0.978 1.434 1.4271 15.611 63.125 47.514 0.947 1.442 1.4262 13.941 63.929 49.988 0.900 1.432 1.4013 15.491 60.51 45.019 1.000 1.349 1.3494 15.059 37.434 44.75 1.006 1.399 1.4015 15.793 55.505 39.712 1.133 1.405 1.4436 14.558 58.434 43.876 1.026 1.451 1.4597 13.895 64.744 50.85 0.885 1.427 1.391

2011/11/30 A. Calcaterra 10

Page 11: ZDD installation and performance

Find passing tracks (left side)

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Page 12: ZDD installation and performance

4Q passing tracks (“up” calorimeter)

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Page 13: ZDD installation and performance

Absolute scale and E/E

• According to Montecarlo a passing cosmic track leaves 16 MeV of energy in the scintillator

• QDC scale (when “Happy Box” is used) is approximately 170 pC / 16 MeV = 11 pC / MeV.

• For E/E we find 20/180 = 11%, consistent with simulation (no shower fluctuations).

2011/11/30 A. Calcaterra 13

Page 14: ZDD installation and performance

Number of photoelectrons

• Assuming a PM gain ≈ 1.2·106, the number of photoelectrons per cosmic track is:

• The factor 2 in the denominator is due to the “Happy Box”

• Approximately 1/7th of these 443 p.e. develop in the first PM, 2/7th in each of the other 3 PMs

443102.1106.12

10170619

12

peN

2011/11/30 A. Calcaterra 14

Page 15: ZDD installation and performance

Photoelectrons/MeV (cosmics)

• According to Montecarlo 16 MeV are deposited in the scintillator by cosmic track, 50 MeV in all. This means:

• 28 photoelectrons/MeV in the fibers (14 cm)• 9 photoelectrons/MeV in the whole

calorimeter

2011/11/30 A. Calcaterra 15

Page 16: ZDD installation and performance

2011/11/30

ZDD as a new luminometer(luminosity monitor)

• The old luminometer on east side of BESIII was uninstalled and replaced by ZDD.• ZDD signal is fanned out as luminometer. The electronics and DAQ for luminometer are kept the same.• Tested by the noise, the new luminometer system is working properly. Its performance as a luminometer

shall be checked under colliding mode of BEPCII.

Frascati cosmic ray test shows:

The time resolution is 0.97ns, which meets the requirement of a luminometer ( <4ns) The signal width is only 5.2ns, so dead time is very little.

Slide by Xue Zhen16

Page 17: ZDD installation and performance

Tests at the BTF

2011/11/30 A. Calcaterra 17

• The BTF: few-electrons, 50Hz pulses from DANE Linac

• Minicalorimeters rotated, fibers vertical• Trigger on AND of RF signal and «finger»• Data taken mostly with QDC (FADC electronics

available only at the end of our beam time)

trigger (6.0x1.1x0.4)cm3

finger scintillator

Single-electron beam from Frascati Beam Test Facility

Page 18: ZDD installation and performance

Purpose of single-electron DAQ

2011/11/30 A. Calcaterra 18

• Study response to single electrons of different energies

• Study • resolution with single electrons• absolute scale factor, MeV/pC• photoelectron statistics

• How does these data compare to cosmic-rays ones?

Page 19: ZDD installation and performance

QDC 8Q, 450 MeV, PM equalized

38.43/294 = 13%

36.84/296 = 12.4%

192011/11/30 A. Calcaterra

Page 20: ZDD installation and performance

Absolute scale

• According to Montecarlo a 450 MeV electron leaves 12%·450 = 54 MeV of energy in the scintillator

• If the absolute scale from cosmics is right, we should see 54 MeV·5.5pC/MeV=297 pC (“Happy Box” X2 preamp was not in use yet)

• ….and we do! Perfect!

202011/11/30 A. Calcaterra

Page 21: ZDD installation and performance

Number of photoelectrons

• Assuming a PM gain ≈ 1.2·106, the number of photoelectrons at 450 MeV is:

• According to MC (12%·450 = 54 MeV deposited in the scintillator) this means 30 photoelectrons per MeV (28 in cosmics)

• How are these divided among the strata?

1600102.1106.1

10300619

12

peN

2011/11/30 A. Calcaterra 21

Page 22: ZDD installation and performance

Run 4 at 450 MeV

22

32/300=10% 150/300=50%

86/300=30% 31/300=10%

2011/11/30 A. Calcaterra

Page 23: ZDD installation and performance

The ZDD installation war!

2011/11/30 A. Calcaterra 23

Arrival at IHEP

Page 24: ZDD installation and performance

The ZDD installation war!

2011/11/30 A. Calcaterra 24

Page 25: ZDD installation and performance

The ZDD installation war!

2011/11/30 A. Calcaterra 25

Page 26: ZDD installation and performance

The ZDD installation war!

2011/11/30 A. Calcaterra 26

Page 27: ZDD installation and performance

The ZDD installation war!

2011/11/30 A. Calcaterra 27

Thanks Mario and Zhen for a fantastic effort!

Page 28: ZDD installation and performance

Cosmic rays at IHEP• There is no external trigger• Auto-generated trigger: ≥2 out of 8 FlashADC

channels must have a minimum below some threshold (baseline-3cts = baseline-12mV)

2011/11/30 A. Calcaterra 28

Page 29: ZDD installation and performance

Analysis still very preliminary• Fitting the waveforms we obtain for each

channel a minimum and a time of minimum– Noise shows up mainly in 2-hits events (peak

times differ randomly)– 3-hits events are much cleaner

• …still, very difficult to define a passing track, due to the very small solid angle

• No control over the track length, many different track lengths in the samples

2011/11/30 A. Calcaterra 29

Page 30: ZDD installation and performance

Tue 2011/11/22, 6.5 hours of data

2011/11/30 A. Calcaterra 30

Horizontal scale ns, 1bin=2ns.We plot t if majority=2, or the biggest time difference out of 3 (majority=3) or out of 6 (majority=4)

Page 31: ZDD installation and performance

Next steps (very soon)

• Use BESIII signals into our own DAQ instead of auto-generated one but read data onto our separate PC.

• Implement the TDC (100 ps resolution)• Estimate data size in real running conditions

– Expected size = 1 byte per channel per BESIII trigger per window size (1 sample/2 ns)

– 200 ns window 16 bytes*100 samples

2011/11/30 A. Calcaterra 31

Page 32: ZDD installation and performance

Next steps (not much later)

• After data size is known (and accepted )…• …and we demonstrate that the data may be

useful…• …then, we will finally ask to incorporate VME

readout into BESIII general dataflow• At this point, help will be needed from expert

BESIII DAQ- and offline-reconstruction persons

2011/11/30 A. Calcaterra 32

Page 33: ZDD installation and performance

Conclusions

• The ZDD has been designed, built, and tested in record-time

• The design is sound and the performances are acceptable given the relatively little time and effort left for data taking and analysis

• The installation was hard but the final result is satisfactory

• Next stop…….physics results

2011/11/30 A. Calcaterra 33

Page 34: ZDD installation and performance

A final thought of wisdom

“One knows very well that, in reducing ideals to practice, great latitude of tolerance is needful; very great”

T. Carlyle

2011/11/30 A. Calcaterra 34

Page 35: ZDD installation and performance

Spares

2011/11/30 A. Calcaterra 35

Page 36: ZDD installation and performance

The HV correction

• Let’s choose a “target” amplification (45 pC)• In column 5 we find the factor to correct for• According to

• We compute

)/log()log()log( 00nnnn VVGG

/)/log()log()log( 00nnnn GGVV

2011/11/30 A. Calcaterra 36

Page 37: ZDD installation and performance

PM HV calibration

• Initial 8-channel equalization done on the basis of Hamamatsu individual datasheets

• For all events, find pedestals and peaks• Choose one channel as normalization• Assuming (Hamamatsu datasheets)

• Invert formula and find new Vn’s

)/log(74.4)log()log( 00nnnn VVGG

2011/11/30 A. Calcaterra 37

Page 38: ZDD installation and performance

FADC scale calibration

2011/11/30 A. Calcaterra 38

Page 39: ZDD installation and performance

Run 228, cosmics, QDC data

Ch Ped (pC) Peak (pC) Signal (pC) (pC) /E(%)

0 16.1 (27.2±0.3) 11.1 (4.2±0.3) 38%

1 15.7 (36.2±0.9) 20.5 (7.2±1.0) 35%

2 14.1 (35.9±1.0) 21.9 (6.8±0.7) 31%

3 15.6 (37.6±0.7) 22.0 (5.5±0.8) 25%

392011/11/30 A. Calcaterra

Page 40: ZDD installation and performance

Run 228, cosmics, FADC data

Peak in channels 1,2,3 is a factor 2 higher than in channel 0, just as expected. This is a good thing!

40

Ch Peak (mV) (mV) /E (%)

0 (142±10) (63±20) 44

1 (323±23) (109±34) 38

2 (383±25) (102±40) 27

3 (316±57) (162±91) 512011/11/30 A. Calcaterra

Page 41: ZDD installation and performance

Conversion factors at 1.4 kV

• Run 228: no “Happy Box”: 5.5 pC/MeV of scintillator-deposited energy

• QDC+FADC cosmics data: unfortunately, a small sample (1 day only)

Ch Peak (pC) Peak (mV) Factor (mV/pC) Factor (mV/MeV)

0 11.1 142 12.8 70.4

1 20.5 323 15.8 86.9

2 21.9 383 17.5 96.25

3 22.0 316 14.4 79.2

412011/11/30 A. Calcaterra


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