performance test of sts demonstrators

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Performance test of STS demonstrators Anton Lymanets 15 th CBM collaboration meeting, April 12 th , 2010

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Performance test of STS demonstrators. Anton Lymanets. 15 th CBM collaboration meeting, April 12 th , 2010. Outline. Demonstrators tested so far. n-XYTER energy calibration. ADC response. Pedestal position and effective amplitudes of - peaks. - PowerPoint PPT Presentation

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Page 1: Performance test of STS demonstrators

Performance test of STS demonstrators

Anton Lymanets

15th CBM collaboration meeting, April 12th, 2010

Page 2: Performance test of STS demonstrators

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OutlineOutline

Demonstrators tested so far. n-XYTER energy calibration. ADC response. Pedestal position and effective amplitudes

of -peaks. Pedestal profile dependence on current

consumption. Crosstalk studies.

Page 3: Performance test of STS demonstrators

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The demonstratorsThe demonstratorsFEB rev. B:• Every second channel bondable.• Still good for lab tests for timing studies or ADC response (without clustering).FEB rev. C:• All channels are usable• But thermal stability becomes an issue.Detector-FEB cable:• Turns out to work if shielded properly.Detectors of CBM01 and CBM02 type “behave” similarly (bad), poor charge collection at n-sides.FEB 4nx:• Cooling plates improve thermal stability• Problems with surviving potential of the chips on board.• Beam time : vastly different count rates in different stations caused by the beam.

Conclusion: depletion conditions should be controlled carefully.

Page 4: Performance test of STS demonstrators

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Energy calibrationEnergy calibrationis important for beam time data analysis and

estimates of signal-to-noise performance, charge collection efficiency, etc.

Cons: capacitance is small => strongly depends on stray capacitance.

CV Q

Q=C∙V

Create known voltage step over known capacitance

Use x-rays with Si strip detector

Pros: well defined energy. Range of 59 keV electrons

is ~ 15 μm => full energy is absorbed.

Page 5: Performance test of STS demonstrators

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Energy calibration with Energy calibration with 241241AmAmUsing 300 μm pitch detector => no significant charge sharing

Energy gain = 110.6 e-/ADC cnt+ one can obtain pedestal energy (not necessarily zero)

Noise 460 e- @ 6 pF

Page 6: Performance test of STS demonstrators

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Calibration lineCalibration line

Energy calibration is obtained, but extrapolated pedestal amplitude is ~3 kElectrons. Possible reasons: non-linearity, bias due to peak detector.

Page 7: Performance test of STS demonstrators

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Controlling detector depletionControlling detector depletion

X-ray characterization:count rate vs. bias Current-voltage measurement

241Am x-rays measured on p-side

Method works for • p-strips before type inversion or • n-strips after type inversion

Q6 Q6

Page 8: Performance test of STS demonstrators

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ADC response to the MIPsADC response to the MIPs

Landau peak with maximum corresponding to ~16.5 ke-

Expectation in ~300 μm Si: 23 ke-

Landau + Gaussian component

Page 9: Performance test of STS demonstrators

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Pedestal position crosses zero at ~1.4 VDynamic range is reduced!Indirect measurement: VbiasS is measured in test channel, not in ch.46

Measured inFEB B03,ch. #46

Pedestal positionPedestal position

Page 10: Performance test of STS demonstrators

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Peak1: 7.2 ke-Peak2: 16.3 ke-

Amplitude = peak position - pedestal

Hitting the lower rail Hitting the upper rail

Peak amplitudesPeak amplitudes

Page 11: Performance test of STS demonstrators

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Peak detect & hold

in out

Peak detect & hold circuit “remembers” the maximum amplitude and keeps it until it is transferred to analog FIFO.

Offset in peak detector outputmay cause pedestal ≠ 0

The role of peak detectorThe role of peak detector

Observed pedestal/peak shifts are not reproducible Observed pedestal/peak shifts are not reproducible in device simulationsin device simulations

Page 12: Performance test of STS demonstrators

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n-XYTER chipn-XYTER chip

Inpu

t pa

ds

Out

put

pads

Power lines

Power lines

current

current

Channel 127

Channel 0Test channel

Page 13: Performance test of STS demonstrators

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Pedestal profile over channelsPedestal profile over channels

Pedestal “sag” is observed with maximum in channel #64To be addressed in the upcoming engineering run done in Heidelberg Univ. (H. K. Soltveit)

Page 14: Performance test of STS demonstrators

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Crosstalk problem – looking into the test Crosstalk problem – looking into the test

channelchannel

Look with scope into test channel and fire pulses in its neighbor ch. 0

analog part digital part

Page 15: Performance test of STS demonstrators

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Default chip settings, test pulses in 32 Default chip settings, test pulses in 32 channelschannels

Questions: digital or analog pickup? dependence on channel number? local effect?

Page 16: Performance test of STS demonstrators

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Part of the channels masked, Part of the channels masked, pulses in 16 channels.pulses in 16 channels.

Channels 0..63 masked Channels 64..127 masked

Crosstalk is not related to activity in neighboring channel,but to number of active channels => Non-local effect

Page 17: Performance test of STS demonstrators

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Does the effect have analog nature?Does the effect have analog nature?

cal = 128

Change test pulse height (cal setting)

cal = 256

Very small effect of amplitude seen => Mostly digital effect

Page 18: Performance test of STS demonstrators

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Crosstalk problem – using laser pulsesCrosstalk problem – using laser pulses

XT - signal transmitted in one channel creates undesired effect in another channel.

Crosstalk in detector vs. crosstalk in read-out chip. n-XYTER review meeting: December 11th, 2009. The way to go: create signals using laser in isolated

channels, look for the response in neighboring channels.

?

?

?

? AdvantageAdvantage:

Study crosstalk in the chip avoiding crosstalk in the detector.

detectorread-out chip

Page 19: Performance test of STS demonstrators

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Channel hit occupancyChannel hit occupancy

Channel number

Cou

nts

• Big laser spot - equal number of hits in each channel.• Hit count rate corresponds to pulse rate.

Page 20: Performance test of STS demonstrators

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ADC distributionADC distribution

Raw spectrum Baseline subtracted. Line shape corresponds to intensity distribution in the laser spot.

Using automatic baseline correction

Page 21: Performance test of STS demonstrators

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Method: look at signal peak mean Method: look at signal peak mean and RMS with noise presentand RMS with noise present

High noise Low noise

With low noise in the channel of interest the observed effects are With low noise in the channel of interest the observed effects are caused by increased occupancy in other channelscaused by increased occupancy in other channels

Page 22: Performance test of STS demonstrators

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Signal mean and RMS Signal mean and RMS vs. n-XYTER occupancyvs. n-XYTER occupancy

Channel 69Channel 69

Signal peak width increases vs. total chip occupancy.Signal peak width increases vs. total chip occupancy.

Signal amplitude drops down linearly with increasing Signal amplitude drops down linearly with increasing total count rate.total count rate.

Page 23: Performance test of STS demonstrators

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Conclusions I

Energy calibration has been done.

Energy gain = 110 e-/ADC count.

Pedestal “amplitude” depends on VbiasS voltage.

Conditions for pedestal zero “amplitude” have been determined, but then the dynamic range is reduced.

Page 24: Performance test of STS demonstrators

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N-XYTER Gain depends on VbiasS voltage.

“Sag” in pedestal profile depends on chip power consumption => to be addressed in n-XYTER engineering run.

Crosstalk in the chip has digital nature and depends on overall chip activity.

Conclusions II

Page 25: Performance test of STS demonstrators

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Conclusions III – Demonstrator Systems Problems with charge collection in CBM01

and CBM02 – need to control sensor bias. Front-end boards: no operational 4nx-

boards and few 1nx-bords are left (this poses a threat to the upcoming beam time).