detection methods
DESCRIPTION
Detection Methods. Coherent ↔ Incoherent Photon Detection ↔ Bolometric Photon Counting ↔ Integrating. Radio Telescopes. Typical Designs Heterodyne Receivers. Jansky’s First Radio Telescope 1933. Grote Reber: 1937 Radio Telescope. Heterodyne Receivers. - PowerPoint PPT PresentationTRANSCRIPT
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Detection Methods
• Coherent ↔ Incoherent• Photon Detection ↔ Bolometric• Photon Counting ↔ Integrating
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Radio Telescopes
• Typical Designs• Heterodyne Receivers
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Jansky’s First Radio Telescope
1933
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Grote Reber: 1937 Radio Telescope
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Heterodyne Receivers
• Mix signal and local oscillator• Mixed signal contains
“intermediate frequency”f_signal – f_local but also the sum of the frequencies
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Heterodyne Signal Detection
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MM and Sub-MM Telescopes
• Use both coherent and incoherent detection
• Heterodyne receivers for emission-lines• Mostly bolometers for continuum
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Millimeter Valley on Mauna Kea
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NGC 6334
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Detection Methods
• Coherent ↔ Incoherent• Photon Detection ↔ Bolometric• Photon Counting ↔ Integrating
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Bolometers
• Absorb and thermalize photons• Measure temperature change• Balance between heating and cooling
results in long time constants• Typically used in chopped operation
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Transition Edge Sensors: Extreme sensitivity to small temperature changes allows to build very sensitive bolometer arrays
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Photocathods
• The photoelectric effect• Quantum nature of light• Photomultipliers, channel plates …
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Detection Methods
• Coherent ↔ Incoherent• Photon Detection ↔ Bolometric• Photon Counting ↔ Integrating
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Photocathod Devices
• Cathods• Photomultiplier• Image intensifiers• Microchannel plates
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In 1907 Joel Stebbins pioneered the use of photoelectric devices in Astronomy
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Photomultiplier tubes: pile up errors
Each detected photon produces a pulse of finite duration, t0, which causes a dead time in the detector. The number of pulses (exposure time) is reduced by the amount of overlapping deadtimes.
N = n/(1–t0n)N is the true rate, and n the apparent rate
Pile-up errors System blocks completely at
high light levels
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• 1840 J.W. Draper makes a photograph of the moon. Followed by photographs of the Sun by Foucault and Fizeau
• Sunspots photographed in 1858 by W. De La Rue• Jansen and Lockyer in the 1870s photographed the solar
spectrum and discovered the spectral lines of Helium.• Ainsee Common photographed Orion Nebula and these
revealed stars and details you could not see in a telescope • Photographs by Hubble in the early 1900‘s established that
some nebula where „island universes“ (i.e. galaxies). His spectral observations of galaxies (exposures of more than one night) led to the discovery of the expansion of the Universe.
• For 100 years photographic plates/film dominated the field of astronomical detectors.
A Revolution in Detectors: Photographic Plates
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Detection Methods
• Coherent ↔ Incoherent• Photon Detection ↔ Bolometric• Photon Counting ↔ Integrating
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Physics of Semiconductors
Basic Quantum PhysicsSolids
SemiconductorsPN Junctions
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Semiconductors
• Conduction in semiconductors• Doping
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Detection Methods
• Coherent ↔ Incoherent• Photon Detection ↔ Bolometric• Photon Counting ↔ Integrating
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PN Junctions
• Formation of pn junction• Rectifying properties• Charge separating properties
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Electronics
• PN junctions and photodiodes• Field Effect transistors• Logic devices• Analog switches• Operational amplifiers• A practical example
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Field Effect Transistor
• Junction FET (JFET)• Metal-Oxide-Semiconductor FET
(MOSFET)• CMOS circuits (Complementary Oxide
Semiconductor)
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Fabrication of Integrated Circuits
• Doping• Depositing metal• Growing oxides (as isolators)• All controlled by photoresist masking
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HAWAII-2: Photolithographically Abut 4 CMOS Reticles to Produce Each 20482 ROIC
Twelve 20482 ROICs per 8” Wafer
20482 Readout Provides Low Read Noise for Visible and MWIR
Canon 16mm x 14 mmGCA 20mm x 20 mm
ASML 22mm x 27.4 mmReticle-Stitching: 2048x2048 ROIC
Submicron Stepper Options
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3-D Barrier to Prevent Glow from Reaching the Detector
Metal 1
Metal 2
Metal 3
Poly 1
Analog Capacitor
Low
-Noi
se C
MO
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ultip
lexe
r
p-type
n+
HgCdTeDetector
IndiumInterconnect
Overglass
CMOS (LOCOS)
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