1 Detectors RIT Course Number 1051-465 Lecture CMOS Detectors.

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1 Detectors RIT Course Number 1051-465 Lecture CMOS Detectors
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Transcript of 1 Detectors RIT Course Number 1051-465 Lecture CMOS Detectors.

Page 1: 1 Detectors RIT Course Number 1051-465 Lecture CMOS Detectors.

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Detectors

RIT Course Number 1051-465Lecture CMOS Detectors

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Aims for this lecture• To describe CMOS hybrid and monolithic detectors

– physical principles– operation– and performance of CMOS detectors

• Given modern examples of CMOS detectors

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Lecture Outline• CMOS detector definition

• CMOS detector principles of operation

• Performance of modern CMOS detectors

• Examples of CMOS detectors

• Historical context of CMOS detectors

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CMOS Detector Architectures

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CMOS Detector Definition• CMOS detectors are made of complimentary MOSFET

circuits connected to light-sensitive materials.

• The voltage change due to integrated photogenerated charge is generally sensed directly through a source follower amplifier in each pixel, instead of via a charge transfer process, i.e. in CCDs.

• Charge is sensed as a voltage directly in the pixel and is not reset every time it is sensed, unlike in a CCD.

• The readout circuit is often called a “multiplexer” because it can sequentially direct signals from multiple pixels to an individual output amplifier.

• Historically, they have been developed later than CCDs, and first for infrared astronomy detectors.

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CMOS vs. CCD Readout• CMOS has “direct readout (DRO)” random access

architecture.

• (Note that the CMOS device in the figure has readout circuitry that takes up some real estate – it is frontside illuminated, producing non-ideal fill factor.)

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CMOS Detector Types• Monolithic (“one piece”)

– readout and photodiode integrated in same part, which means that light sensitive layer is made of silicon (only sensitive to optical photons)

– frontside or backside illuminated– can be made with mostly standardized CMOS processes that are

common to the commercial semiconductor industry

• Hybrid (“two pieces”)– readout circuit is separate from photodiode– readout is made of silicon– photodiode is made of semiconductor with suitable cutoff wavelength– requires many custom steps

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Hybrid Architecture

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Hybrid Array Benefits• Hybrid arrays are used when one wants to detect light of

wavelengths that are not absorbed by silicon, i.e. wavelengths beyond ~1um.

• Infrared arrays are “hybrids” – they use one material to detect light and silicon for the readout circuit.

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Hybrid Array Detection Flow

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Hybrid Array Architecture

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Hybrid Array Bonding

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Hybrid Array Summary

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Hybrid Array Key Technologies

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CMOS Hybrid Detector Example: InSb Array

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CMOS Hybrid Detector Example: NICMOS Array

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Infrared Hybrid Array Substrate Removal

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Readout Integrated Circuit (ROIC)also known as the Multiplexer

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Detector Unit Cell

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Detector Multiplexer

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Detector Operation

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NICMOS MUX

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Light-sensitive Materials

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• Semiconductors occupy column IV of the Periodic Table• Outer shells have four empty valence states• An outer shell electron can leave the shell if it absorbs

enough energy

Periodic Table

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Periodic Table Continued• The column number gives the number of valence electrons per

atom. Primary semiconductors have 4.

• Compounds including elements from neighboring columns can be formed. These alloys have semiconductor properties as well (e.g. HgCdTe & InSb).

• Mercury-cadmium-telluride (HgCdTe; used in NICMOS) and indium-antimonide (InSb; used in SIRTF) are the dominant detector technologies in the near-IR.

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(1) .EGc

c

hch

The Band Gap Determines the Red Limit

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Performance

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Dark Current• Dark current is the signal that is seen in the absence of any

light.

• The dominant components are diffusion across the pn junction, thermal generation-recombination (G-R) of charges within the bulk of the semiconductor, and leakage currents typically through surfaces.

• Dark current adds an effective noise due to the shot noise of the dark charge.

• Dark current can be reduced by cooling.

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Dark Current Example

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Dark Current vs. Temperature

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Read Noise• Read noise is the uncertainty in the signal measurement due to

electrical fluctuations produced by the detector.

• For CMOS devices, it is due to:– Johnson noise of FETs– random telegraph signal (a.k.a. popcorn noise) in the output FET– interface states at material surfaces

• Typical read noise values for CMOS devices are around 10 electrons.

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Read Noise Example

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Sampling Schemes• By being a bit clever about reading out the array, one can

minimize or eliminate some of these noise modes.

• During an exposure, typically each pixel is sampled several times.

• The most common approaches are correlated double sampling (CDS), multiple non-destructive reads (aka “Fowler Sampling”), & fitting a line (aka “up the ramp”).

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N

1f

N

1i V

N1

VN1

Vjj

jj

Fowler Sampling

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• Fit best line to multiple non-destructive samples.• Sample spacing does not need to be uniform.• Not clear whether this or Fowler sampling is best.• This is what is done in NICMOS MULTIACCUM mode.

“Up the Ramp”

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Hybrid Array Optimization – Quantum Efficiency

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Well Depth and Non-linearity• Well capacity is defined as the maximum charge that can be

held in a pixel.

• “Saturation” is the term that describes when a pixel has accumulated the maximum amount of charge that it can hold.

• The “full well” capacity in a CCD is typically a few hundred thousand electrons per pixel for today’s technologies.

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Well Depth and Non-linearity Example

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Non-linearity Example

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Persistence• Persistence is the afterimage that a detector can produce if it

traps charge from a previous exposure and releases it during the current exposure.

• It is produced by charge traps.

• Charge traps will decay with an exponential timescale.

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Persistence Example

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Persistence Movie

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Pixel-to-pixel Crosstalk• Crosstalk is the generic term that describes signal

contamination due to the presence of a signal in another pixel or electrical channel.

• Charge diffusion from one pixel to a neighbor is an important crosstalk mechanism in IR arrays and CCDs.

• Once charge carriers are created, their motion is governed by charge diffusion.

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IPC• Interpixel capacitance (IPC) is a form of crosstalk.

• In this case, charge in a pixel induces a voltage change in a neighbor, just like the behavior between parallel plates in a capacitor.

• The effect is to blur the point spread function.

• The induced voltage does not have noise.

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IPC• In this example, IPC is very large for the H4RG SiPIN device

(10 um pixel size).

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Arrays in Use Today

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Teledyne H4RG Si PIN• This is an image of the H4RG device in the Rochester

Imagingn Detector Laboratory (RIDL).

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Raytheon Family Arrays

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Hybrid Visible Silicon Imager - HyViSI

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HyViSI

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HyViSI

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Modern Array Examples

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History of Hybrid Infrared Arrays

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History of Infrared Detection• Herschel’s detection of IR from Sun in 1800

• Johnson’s IR photometry of stars (PbS) mid 60’s

• Neugebauer & Leighton: 2m Sky Survey (PbS), late 60’s

• Development of bolometer (Low) late 60’s

• Development of InSb (mainly military) early 70’s

• IRAS 1983

• CMOS Hybrid Arrays (InSb, HgCdTe, Si:As IBCs) mid-80’s

• NICMOS, 2MASS, IRTF, UKIRT, KAO, common-user instruments, Gemini, etc.

• JWST

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Science Motivation• Exploration & discovery

– Neugebauer, Leighton, Low, Fazio, Townes

• Technological opportunities– Bolometer (Low), PbS (Neugebauer), balloons (Fazio), IR lasers &

interferometry (Townes)

• A few, key problems– Bolometric luminosities (Herschel, Johnson)– The Galactic Center (Becklin)– Star formation