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Mid-IR photon counting array using HgCdTe APDs and the Medipix2 ROIC
John Vallerga and Jason McPhate Space Sciences Laboratory University of California, Berkeley Larry Dawson and Maryn Stapelbroek DRS Sensors & Targeting Systems, Cypress CA
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Photon counting Charge integrating Events Q V ± sv Events ± sEvents
Threshold Events Count (x,y,t) Charge integrating Q ADC V ± sv Events ± sEvents
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Motivation for photon counting
Reduction of readout noise in infrared imaging Advantageous in applications where imaging is not background dominated: High frame rate (adaptive optics, interferometry) Short integration times (Lidar etc.) Low background (spectrophotometry, space based)
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Signal in presence of noise
8 x 8 Noiseless 35% QE 10 photons - 100 photons 1000 photons 8 x e- rms 90% QE 6 x e- rms 90% QE 4 x e- rms 90% QE
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Imaging IR photon counting detector concept
Use an IR sensitive absorber with gain HgCdTe APDs Large arrays Count events at the pixel level “Medipix2” CMOS ASIC 55m pixels, 256x256 format Readout binary data at 100MHz fast (~1 kHz framerate)
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Avalanche Photodiodes (APDs)
Geiger mode Biased above breakdown High, saturated gain - easy to count Long recovery time per event Afterpulsing and higher background Linear mode Biased near breakdown Lower gain -harder to count Distribution of pulse sizes - “excess noise”
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High Density Vertically Integrated Photodiode (HDVIP)
DRS Infrared Technologies
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HDVIP IR APDs from DRS HgCd1-xTex with adjustable c
Electron induced avalanche Ion-milled via allows backside readout Linear gains as high as 1000 (c < 4.3m) Excess noise ~ 1 ! Arrays have been fabricated (128x128)
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Gain vs. bias voltage l = 4.3 mm, 77K, 53 of 54 in array
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Excess noise factor k=0, only electrons involved in amplification
Excess noise factor of 1.0 implies a deterministic amplification process Low noise factor allows a higher threshold in pulse sensing electronics
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Medipix2 ROIC Each pixel has amp, discriminator, gate & counter.
256 x 256 with 55 µm pixels (buttable to 512 x 512). Counts integrated at pixel. No charge transfer! Amplifier noise 110 e- rms ~ 500 transistors/pixel
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Medipix readout of semiconductor arrays
Developed at CERN for Medipix collaboration (xray) radiography tomography mammography neutron detection gamma imaging MCP readout gaseous detectors electron microscope
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Medipix2 readout architecture
3584 bit Pixel Column 0 3584 bit Pixel Column 255 3584 bit Pixel Column 1 256 bit fast shift register 32 bit CMOS output LVDS out Pixel values are digital (14 bit) Bits are shifted into fast shift register Choice of serial or 32 bit parallel output Maximum designed bandwidth is 100MHz Corresponds to 284µs frame readout
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HDVIP - Medipix2 Hybrid Characteristics well matched: HDVIP Medipix2
64 m pixel (8x8) mm pixel Gain up to Minimum threshold 900e- Backside output Frontside input Low dark current nA/pxl compensation However 77K operation Room temp. design IR sensitive Very active chip
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Test Setup Simple test - drop Medipix2 chip into LN2
Mounted on ceramic header used for 350C tests Attached to brass heat sink and copper cold finger Accurate diode thermometer glued to header
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Ceramic Header & Thermal Testing
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Test thermal profile
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Individual DACs vs. Temp.
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Threshold Variation (noise)
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Threshold Variation (noise)
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Threshold Variation (noise)
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Feasibility Test at DRS
Used existing 8x8 APD array mounted on fan-out header Wirebonded 8 APD outputs to 8 Medipix2 input pads Hybrid assembly mounted on larger header Large header mounted in test dewar Expect higher amplifier noise due to increased capacitance Use IR photodiode as photon light source to input light pulses Use photon-transfer curve to characterize gain and noise
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Medipix2 and APD array APD array Medipix2 Wirebonds
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Test Hybrid in dewar
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IR photodiode to illuminate APD
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Future work Start/continue feasibility tests
Quantify noise, gain and threshold sensitivity Extrapolate results to realistic APD mounting Investigate APD fabrication techniques onto Medipix wafer Model/simulate APD pixel to match Medipix Seek funding to pursue full chip fabrication
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If successful, this effort could lead to a sensor with:
Summary If successful, this effort could lead to a sensor with: HgCdTe QE (c < 4.3 m) Large arrays (512 x n*256) Zero readout noise kHz frame rates or higher Electronic shutter Which should prove very useful for many niche applications with low background in the IR
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