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G. Finger, R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

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Recent Performance Improvements, Calibration Techniques and Mitigation Strategies for Large-format HgCdTe Arrays. G. Finger, R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier. Introduction. Hawaii-2RG close to prefect wrt basic parameters noise, QE, darkcurrent - PowerPoint PPT Presentation
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Recent Performance Improvements, Calibration Techniques and Mitigation Strategies for Large-format HgCdTe Arrays G. Finger, R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier
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Page 1: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Recent Performance Improvements, Calibration Techniques and Mitigation

Strategies for Large-format HgCdTe Arrays

G. Finger, R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Page 2: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Hawaii-2RG close to prefect wrt basic parameters noise, QE, darkcurrent

comparison of 4 methods to determine conversion gain persistence of HgCdTe Hawaii-2RG arrays mitigation strategy to reduce persistence method to measure persistence in darkness

Introduction

Page 3: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Noise comparison H2RG #119 / H2RG #184

H2RG #119 (X-Shooter)25.3 erms on IR active pixels7.7 erms on reference pixels

H2RG #184 (KMOS)6,9 erms on IR active pixels5.8 erms on reference pixels

bond pad contact resistance improved noise reduced from 25.3 to 6.9 erms

Readout noise < 10 erms for DCS on 5 new science arrays (KMOS and SPHERE)

Page 4: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Noise of KMOS arrays with Fowler sampling

Reduce noise with multiple nodestructive sampling

Noise 2.2 erms for 32 Fowler pairs

Page 5: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Noise map of crossdispersed spectrum slit open / warm instrument shutter closed integration time = 600s ( 903 nondestructive readouts) limited by shot noise of photon background which is dominated

by scattered light of K-band (5E-2 e/s/pixel)

J order 26

K order 11

Page 6: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Dark current of c =2.5 m HgCdTe

Crossdispersed echelle spectrum with slit closed

Cut levels :

0 - 5E-3 e/s/pixelat T=81K , Vbias=1V

1

2

Page 7: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

dark current outside optical field:4.2 E-4 e/s/pixel

dark current in J1.3 E-3 e/s/pixel

T=81K, VBIAS = 1V

Dark current of c =2.5 m HgCdTe

Page 8: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Dark current versus temperature

Quantum efficiency high over the entire sensitive range of the array

Measurement at optical wavelengths pending

Page 9: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

IPC with single pixel reset

uniformly illuminate arraywith high flux integration time 1 s

Use guide mode of Hawaii-2RG muxguide window size 1x1

Reset single pixel before readoutintegration time < 500s

Page 10: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

uniformly illuminate arraywith high flux integration time 1 s

Use guide mode of Hawaii-2RG muxguide window size 1x1

Reset single pixel before readoutintegration time < 500s

Observe capacitive coupling on next neighbors

IPC with single pixel reset

Page 11: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

recent improvements of IPC

•improvements in multiplexer layout resulted in reduction of coupling coefficient :

#184=1.7% #226=1.4%

H2RG #184

H2RG #226

Page 12: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Conversion gain and single pixel reset

Assuming a

• Ori Fox method of classical propagation of errors: used also by Teledyne

Cij is covariancebetween pixels i and j

true variance

Page 13: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Conversion gain and single pixel reset

Assuming a

• Ori Fox method of classical propagation of errors: used also by Teledyne

Cij is covariancebetween pixels i and j

• =0.17 : correction factor 1+8 =1.13

true variance

Page 14: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Conversion gain and single pixel reset

variance versus signal:

2.26 e/ADU single pixel reset IPC

correction1.96 e/ADU

Page 15: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Conversion gain from integrated autocorreolation

variance versus signal:

2.26 e/ADU single pixel reset IPC

correction1.96 e/ADU

integrated autocorrelation versus signal: 2.04 e/ADU

Page 16: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Conversion gain by capacitance comparison method

Vreset

Dsub

CextC0

Reset SFD

V

Relais

Detector

01

,2,1, )( CVCVVnpixel

iinextextext

dc level drifton external capacitor

sum of signal of all pixels

slope = C0/Cext

Page 17: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Conversion gain by capacitance comparison method

Vreset

Dsub

CextC0

Reset SFD

V

Relais

Detector

Ccryo

Ccryo difficult to estimate without risk for detector:Ccryo includes capacitances of cable, preamplifier board and wirebond ceramics

Ceramic capacitors on HAWAII-2RG wirebond ceramics show strong temperature dependence:T=296 K C=1FT=77 K C=276 nF

Page 18: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Conversion gain by capacitance comparison method

0

0

0

1extcryoext CCCC

C0=32.8 fF Ccryo=394 nF

C0/e=205e/mV (in our setup: 1.89e/ADU)

Vreset

Dsub

CextC0

Reset SFD

V

Relais

Detector

Ccryo

0 measured with Cext removed

Page 19: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

comparison of methods to obtain conversion gain

method conversion gain C

[e/ADU] [e/mV] [fF]

variance versus signal 2.26 245 39.2

integrated autocorrelation (Moore et al) 2.04 221 35.4

single pixel reset (Fox et al) 1.96 212 34.0

capacitance comparison 1.89 205 32.8

Remarks:

•first three methods are stochastic (rely on noise measurement)•single pixel reset measures coupling coefficient but assumes only coupling to next neighbors•capacitance comparison is direct and robust method

taking into account coupling to all pixels taking into account cable capacitance and cold ceramic capacitors at detector

Page 20: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence: X-Shooter as test bench

•with slit closed: instrumental background: 4.2E-4 e/s/pixel

•ideal for persistence tests

Page 21: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence: lamp on

DIT=1.65s slit open ThAr lamp

Page 22: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence: slit closed

first dark exposure with DIT=128s after 2048s exposure with open slit

Page 23: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence versus stimulus

Persistence of first 2 min. dark exposure is ~6.3e-4 of stimulus

Page 24: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence at different wavelengths

Persistence almost the same at

=1.07 m

and =2.2 m

Page 25: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence model of Roger Smith

p npn -junction

charge trapped when location of trapbecomes undepleted and is released in next dark exposure

traps populated when exposed to mobileelectrons and holes

Page 26: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

p npn -junction

charge trapped when location of trapbecomes undepleted and is released in next dark exposure

traps populated when exposed to mobileelectrons and holes

Persistence model of Roger Smith

Page 27: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Mitigation of persistence: global reset detrapping

p npn -junction

charge trapped when location of trapbecomes undepleted and is released in next dark exposure

traps populated when exposed to mobileelectrons and holes

keep global reset switch closed after science exposure allow de-trapping of charge

Page 28: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

28

•Slit open

Mitigation of persistence: global reset detrapping

Page 29: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

29

•First 2 minute dark exposure without global reset de-trapping

Mitigation of persistence: global reset detrapping

Page 30: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

30

•Keep reset switch of all pixels permanently closed with global reset for 128 s at the end of bright exposure

to force depletion width to stay wide avoiding population of traps• de-trapping time is 128 s• close slit and return to normal operating mode taking dark exposures•Persistence in first dark exposure reduced by factor of 9

•First 2 minute dark exposure with global reset de-trapping

Mitigation of persistence: global reset detrapping

Page 31: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

31

• if reset closed before switching on bright source and kept closed until slit closed again persistence is zero•global reset is an electronic shutter which protects detector from persistence while exposed to bright illumination

•First 2 minute dark exposure with global reset always closed during bright exposure

Mitigation of persistence: global reset detrapping

Page 32: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

32

• In first 2 minute dark exposure intensity of persistence is reduced by a factor of 9 with global reset de-trapping•Duration of detrapping 128 s

without global reset de-trapping

with global reset de-trapping

reset always closed during bright exposure

Mitigation of persistence: global reset detrapping

Page 33: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Method to measure persistence in darkness

hypothesis:

persistence is generated by the change of the voltage across pn junction of pixel diode

instead of using light to shrink depletion region reduce bias voltage in selected area of array using the window mode of the Hawaii-2RG multiplexer and the global rest

outside window normal operation of the array

Page 34: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence electrical /optical

•Generated with bias change in selected area using global reset

•Generated with light source

Page 35: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence electrical /optical

• red diamonds: persistence generated with light source on /off•black triangles: in selected area using global reset persistence generated with bias low / high• decay with similar time constants

Page 36: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence measured in darkness

•Measure persistence of all 3 KMOS detectors in one gouniformity, cosmetics, dark current. readout noise, persistence

•GL scientific mosaic mount •128 channel cryo-preamps , flex boardsand vacuum connectors

Page 37: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence measured in darkness

•Mosaic test facility:no windowno opticsdetector covered by black plateflux < 1E-3 e/s/pixel

Page 38: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence measured in darkness

•integration time 120 sec•operating temperature 66K•generated with bias change in darkness on selected area using global reset

Page 39: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence versus time

•persistence lasts for > 1500s•persistence is device dependent•array # 184 is better

Page 40: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence versus temperature

•persistence is device dependent•persistence of devices #211 and #212 has a maximum at T=66K•persistence of device #184 does not have this temperature maximum

Page 41: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence versus detrapping time

•peristence is decreases with increasing detrapping time

Page 42: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence versus duration of illumination

•persistence increases when detector is exposed to the bright source for a longer time

Page 43: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Persistence versus signal intensity

•persistence increases with increasing stimulus•bias = DSUB – VRESET VRESET=0.5V

increasing signal ( brighter light source)

Page 44: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Global reset de-trapping: on sky test

• after global reset detrapping vertical stripes in first difference images of two 1200s exposures • intensity of stripes in first difference ~ 0.03 e/s/pixel

Page 45: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Global reset de-trapping: on sky test

• profile of vertical stripes in difference images of two 1200s exposures• intensity of stripes in first difference ~ 0.03 e/s/pixel

Page 46: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Global reset de-trapping: on sky test

• vertical stripes in first difference images of two 1200s exposures• intensity of stripes in first difference ~ 0.03 e/s/pixel• stripes located at start of fast shift register

Page 47: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Global reset de-trapping: on sky test

• keep clocks running during global reset detrapping• no vertical stripes in first difference images of two 600s exposures

Page 48: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Global reset de-trapping: on sky test

• profile of vertical stripes in difference images of two 1200s exposures• intensity of stripes in first difference ~ 0.03 e/s/pixel•intensity of stripes in second difference ~ negligible•to be further investigated

Page 49: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Global reset de-trapping: on sky test

• automatic flexure compensation: line intensity 45000 e/s/pixel

Page 50: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Global reset de-trapping: on sky test

• automatic flexure compensation: line intensity 45000 e/s/pixel•First 1500 s dark exposure : no persistence !

Page 51: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

readout noise improved by a factor of 2 on new H2RG (6.9 erms single DCS)

shot noise limited operation achieved in cross dispersed spectrometer in J PTF corrected by single pixel reset factor yields conversion gain

which agrees with capacitance comparison method within 3% persistence model confirmed by experiment:

traps at edge of valence and conduction bands persistence is a consequence of changing bias voltage no persistence is expected with CTIA since bias voltage constant

new method to measure persistence in darkness global reset detrapping successfully tested on sky without residuals

Conclusion

Page 52: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

HAWK-I first light

Tarantula Nebula

THE END

Page 53: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

TLI: Threshold Limited Integration

Multiple nondestructive readouts scheme

Set saturation level If signal exceeds

saturation level, readout not used to calculate slope of integration ramp

Extrapolate signal to DIT In effect different

integration times for pixels exceeding saturation level

Page 54: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

TLI: Threshold Limited Integration

Multiple nondestructive readouts scheme

Set saturation level If signal exceeds

saturation level, readout not used to calculate slope of integration ramp

Extrapolate signal to DIT In effect different

integration times for pixels exceeding saturation level

Page 55: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

TLI: Threshold Limited Integration

Multiple nondestructive readouts scheme

Set saturation level If signal exceeds saturation

level, readout not used to calculate slope of integration ramp

Extrapolate signal to DIT In effect different integration

times for pixels exceeding saturation level

Signal can be >> 107 e Gain of

> 2 orders of magnitude in dynamic range

Page 56: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

TLI: Threshold Limited Integration

Multiple nondestructive readouts scheme

Set saturation level If signal exceeds

saturation level, readout not used to calculate slope of integration ramp

Extrapolate signal to DIT In effect different

integration times for pixels exceeding saturation level

Full well 1E5 electrons With TLI it is possible to

integrate > 1E7 electrons

with TLI

without TLI

Saturation level

Page 57: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Trapping model

P

N

-- - -

-

++++

+

next dark exp.

(small bias reduction)

The released charge reduces the bias voltage. persistence

- - -

+ + +

-- - -

-

++++

+

high flux signal

(low bias)

As signal accumulates the depletion width is reduced. Traps newly exposed to charge can capture some mobile carriers.

Trapped holes

Trapped electrons

- - -

+ + +

++++

+

-- - -

-

reset

(large reverse bias)

At “reset” the wider depletion region is restored, but trapped charge stays behind.

Depleted

Mobile electrons

Mobile holes

dark idle

(large reverse bias)

All traps have released their charge in depletion region

++++

+

-- - -

-

-+

R.Smith, SPIE 7021-22, Marseille 2008-06-24

Page 58: G. Finger,  R. Dorn, S. Eschbaumer, D. Ives, L. Mehrgan, M. Meyer, J. Stegmeier

Dark current versus temperature

generation-recombination limited above 110K

Idark exp(-Teff/T)

Idark exp(-Egap/(1.7 KT)) surface leakage and

tunneling below 100K

1.7E-3 e/s/pixel


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