FM-LS Tests

16
Max-Planck-Institut für Astronomie Heidelberg PACS SVR 22./23. June 2006 MPE Garching J. Stegmaier, U. Grözinger, D. Lemke, O. Krause, H. Dannerbauer, T. Henning, R. Hofferbert, U. Klaas, J. Schreiber Ge:Ga Detector Arrays PACS SVR phase 1, MPE Garching 22.-23. June 2006

description

FM-LS Tests. Warm Functional Tests Separate warm functional test on each module Warm functional test after integration in MPIA test cryostat Cold Performance Tests Cold functional test Cold performance test Variation of Detector-Bias, C int , t int Using different Filter combinations - PowerPoint PPT Presentation

Transcript of FM-LS Tests

Page 1: FM-LS Tests

Max-Planck-Institut für AstronomieHeidelberg

PACS SVR 22./23. June 2006

MPE Garching

J. Stegmaier, U. Grözinger, D. Lemke, O. Krause, H. Dannerbauer, T. Henning,

R. Hofferbert, U. Klaas, J. Schreiber

Ge:Ga Detector Arrays

PACS SVR phase 1, MPE Garching 22.-23. June 2006

Page 2: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Warm Functional Tests- Separate warm functional test on each

module- Warm functional test after integration in

MPIA test cryostat

Cold Performance Tests- Cold functional test- Cold performance test

- Variation of Detector-Bias, Cint, tint

- Using different - Filter combinations- BB-temperatures- Detector temperatures

- Dark measurments

FM-LS Tests

MPIA Test Facility

f-ratio as in PACSIR-flux attenuation: ~ 2.5 · 10-6

Page 3: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

FM LS-Sevenpacks

FM-LS during integration into

MPIA test cryostat

FMmodul

e

Warm functional test

Cold performanc

e testcomments

LS 1 2 hot pixels

LS 2 - 2 non-confirming modules (dummy channel)

LS 2_2 1 open pixel

LS 3 - 1 non confirming module(output frame not stable, low VSS current)

LS 4 - 2 modules with weak pixels

LS 5 1 module under higher stress

LS 6 1 open (dummy) channel 2 modules under higher stress

Page 4: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

FM LS-Sevenpacks

FMmodul

e

Warm functional test

Cold performanc

e testcomments

LS 1 2 hot pixels

LS 2 - 2 non confirming modules (dummy channel)

LS 2_2 1 open pixel

LS 3 - 1 non confirming module(output frame not stable, low VSS current)

LS 4 - 2 modules with weak pixels

LS 5 1 module under higher stress

LS 6 1 open (dummy) channel 2 modules under higher stress

0 2 4 6 8 10 12 14 16 18 202,5

3,0

3,5

4,0

4,5

5,0

5,5

UBias

= 200mV, Cint

= 0

UBias

= 200mV, Cint

= 1FM 115

Ou

tpu

t Vo

ltag

e [V

]

CRE-Channel

channel #14

0 2 4 6 8 10 12 14 16 18 202,5

3,0

3,5

4,0

4,5

5,0

5,5

UBias

= 200mV, Cint

= 0

UBias

= 200mV, Cint

= 1

FM 122

Out

put V

olta

ge [V

]

CRE-Channel

channel #7

FM 122 (LS 2_2)

FM 115 (LS 1)

Page 5: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

ResponsivityNEP

Responsivity / NEP

Responsivity: 7.4 A/W ± 1.7 A/WNEP: 1.18 · 10-16 A/W ± 4.6 · 10-17 A/W

UBias = 200mV, TDet = 2.5K

FM 126, FM 135, FM 136:higher stress (mounting screw of

the test housing pressed the module) modules OK

LS 1 LS 2_2 LS 5 LS 6

Page 6: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Responsivity - Homogenity

LS 1 (FM 120, 118, 115, 114, 110, 108, 107) LS 2_2 (FM 122, 115, 121, 116, 113, 112, 111)

LS 5 (FM 132, 131, 123, 128, 126, 125, 119) LS 6 (FM 130, 137, 136, 135, 134, 133)

0 2 4 6 8 10 12 14 16 180

5

10

15

20 200mV, Cint

= 1

Re

spo

nsi

vity

[A/W

]

channel

FM120 FM118 FM115 FM114 FM110 FM108 FM107

0 2 4 6 8 10 12 14 16 180

5

10

15

20 200mV, Cint

= 1

Re

spo

nsi

vity

[A/W

]

channel

FM122 FM115 FM121 FM116 FM113 FM112 FM111

Spiking pixel FM 115 ch. #14

FM 122 ch. #7 open

0 2 4 6 8 10 12 14 16 180

5

10

15

20

25

30

UBias

= 200mV, Cint

= 1

Re

sp

on

siv

ity [

A/W

]

Channel

FM132 FM131 FM123 FM128 FM126 FM125 FM119

0 2 4 6 8 10 12 14 16 180

5

10

15

20U

Bias = 200mV, C

int = 1

Re

sp

on

siv

ity [A

/W]

Channel

FM130 FM137 FM136 FM135 FM134 FM133

Spiking pixel FM 114 ch. #4

UBias = 200mV, TDet = 2.5K, Cint = 240 pF

higher stress on FM 126

higher stress on FM 135 and FM 136

Page 7: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Responsivity - Bias Scan

0 50 100 150 200 250 3000

5

10

15

20

25 Bias Scan, Cint

= 1

Re

spo

nsi

vity

[A/W

]

bias voltage [mV]

FM120 FM118 FM115 FM114 FM110 FM108 FM107

0 50 100 150 200 250 3000

5

10

15

20

25C

int = 1

Res

pons

ivity

[A/W

]

UBias

[mV]

FM122 FM115 FM121 FM116 FM113 FM112 FM111

0 50 100 150 200 250 3000

5

10

15

20

25C

int = 1

Re

spo

nsi

vity

[A

/W]

UBias

[mV]

FM132 FM131 FM123 FM128 FM126 FM125 FM119

0 50 100 150 200 250 3000

5

10

15

20

25C

int = 1

Re

sp

on

siv

ity [A

/W]

UBias

[mV]

FM130 FM137 FM136 FM135 FM134 FM133

LS 1 (FM 120, 118, 115, 114, 110, 108, 107) LS 2_2 (FM 122, 115, 121, 116, 113, 112, 111)

LS 5 (FM 132, 131, 123, 128, 126, 125, 119) LS 6 (FM 130, 137, 136, 135, 134, 133)

w/o spiking andopen pixels

TDet = 2.5K

FM 126 (LS 5),FM 135 (LS 6),FM 136 (LS 6):higher stress

caused by mounting in the

test housing

Page 8: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

NEP - Bias Scan

LS 1 (FM 120, 118, 115, 114, 110, 108, 107) LS 2_2 (FM 122, 115, 121, 116, 113, 112, 111)

LS 5 (FM 132, 131, 123, 128, 126, 125, 119) LS 6 (FM 130, 137, 136, 135, 134, 133)

TDet = 2.5K

0 50 100 150 200 250 300

0

1x10-16

2x10-16

3x10-16

4x10-16

5x10-16

6x10-16 Bias Scan, Cint

= 1

NE

P [W

/Hz1/

2 ]

bias voltage [mV]

FM120 FM118 FM115 FM114 FM110 FM108 FM107

0 50 100 150 200 250 300

0

1x10-16

2x10-16

3x10-16

4x10-16

5x10-16

6x10-16

Cint

= 1

NE

P

UBias

[mV]

FM122 FM115 FM121 FM116 FM113 FM112 FM111

0 50 100 150 200 250 300

0

1x10-16

2x10-16

3x10-16

4x10-16

5x10-16

6x10-16

Cint

= 1

NE

P

UBias

[mV]

FM132 FM131 FM123 FM128 FM126 FM125 FM119

0 50 100 150 200 250 300

0

1x10-16

2x10-16

3x10-16

4x10-16

5x10-16

6x10-16

Cint

= 1

NE

P

UBias

[mV]

FM130 FM137 FM136 FM135 FM134 FM133

w/o spiking andopen pixels

FM 126 (LS 5),FM 135 (LS 6),FM 136 (LS 6):higher stress

caused by mounting in the

test housing

Page 9: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Dark Current [e-/s]UBias = 200mV, TDet = 2.5K

LS1

LS 1

LS 5

Mean: 3550 e-/s ± 600 e-/s

Requirements: CD ≤ 5*104 e-/s

Page 10: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Higher stress on 3 FMs smaller band gap

LS 5 LS 6

1615141312111098765432

Band gap [meV]

Band Gap

0,25 0,30 0,35 0,40 0,45 0,50e-36

e-35

e-34

e-33

e-32

e-31

e-30

e-29

e-28

e-27

e-26

e-25

e-24

e-23

e-22

dark

cur

rent

[A]

1/TDet

[1/K]

ch2

0,25 0,30 0,35e-36

e-35

e-34

e-33

e-32

e-31

e-30

e-29

e-28

e-27

e-26

e-25

e-24

e-23

e-22

Parameter Wert Fehler------------------------------------------------------------A 2,46252 0,49093B -103,80926 1,6843------------------------------------------------------------

R SD N P-------------------------------------------------------------0,99934 0,14967 7 <0.0001------------------------------------------------------------

da

rk c

urr

en

t [A

]

1/T [1/K]

ch2 lin. fit

FM 120, Ch 2(LS 1)

photon flux on detector

Thermal excitation: Idark ~ exp (-E/kTDet)

Page 11: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Goal: High absolute photometric accuracy in the FIR during „quiet“ periods (~ 1%)

Essential: - Stable operation of Ge:Ga-detectors in PACS at L2- Optimize operating conditions: UBias, TDet

- Minimize curing and calibration frequency

Radiation Environment at L2:- Galactic CR particles (low level fluxes: 3-5 ions/cm²/s; typical energy: 500 MeV – few GeV)- Solar particles events (avg. sol max: 2.5 · 105 ions/cm²/s; Ep ≈ 100 MeV, Eions ≈ GeV range)

Radiation damage in extrinsic photoconductors- Generation of electron hole pairs in bulk of detector- Capture of minority carriers by compensating impurities

Effects on Detector Performance:- Spikes / glitches- Higher detector noise, dark current, detector output change of calibration

- Lower S/N

Ionizing Radiation and Curing

No stable operation of Ge:Ga detectors

Page 12: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Ionizing Radiation Tests

Conditions– Simulated PACS operation conditions – Realistic FIR background: 10-14 W/pix – Low stressed Ge:Ga detector array– ~48 hours each– Every 1 to 10 min a measurement

Without irradiation (preparatory test)– Performance of detector and the test setup – Analysis of systematic effects Measurments highly reproducible with stability < 1%

137Cs detector irradiation– L2 radiation environment: 137Cs source (Eγ = 0.662

MeV)– Hit rate (> 3σ): ~16/s/pix

Long term measurments with 137Cs

Generic charge ramp

Radioactive 137Cs source

Page 13: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Deglitching Method

Glitch detection & deglitching:- sigma clipping applied to pairwise differences (values >3σ)

Skewed distributions:- Robust estimator, e.g., Hodge-Lehmann estimator:

μ = median (Xi+Xj)/2 with 1 ≤ i ≤ j ≤ n

Glitches skewed distribution

Page 14: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

NEP and Responsivity

Glitch rate: Start irradiation: 9 ± 1 hits/s/pixplateau: 16 ± 2 hits/s/pix

Plateau: Accuracy: 4.5 %# > 3σ : 6%

5h

UBias = 160mV, TDet = 2.5K

Page 15: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Bias ScanTDet = 2.5K

Under Irradiation: Operating Ge:Ga detectors

at Ubias < 160mV

Page 16: FM-LS Tests

PACS SVR, MPE22.-23.06.2006 Ge:Ga Detector Arrays

Ionizing Radiation Tests

Preliminary Results:

Measurements w/o irradiation are highly reproducible

137Cs allows simulations of radiation environment at L2

Effective technique for CR rejection: Sigma clipping with robust estimator (e.g., HL)

So far:

- Operating Ge:Ga detectors at a lower bias voltage < 160mV- Long term knowledge of better 5%- Good curing by IR flash (~ 10-12 W/pixel)