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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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The Arecibo 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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SMA Receivers
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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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Photocathod Devices Cathods Photomultiplier Image intensifiers Microchannel plates
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Physics of Semiconductors Basic Quantum Physics Solids Semiconductors PN Junctions
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Semiconductors Conduction in semiconductors Doping
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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 2048 2 ROIC Twelve 2048 2 ROICs per 8” Wafer 2048 2 Readout Provides Low Read Noise for Visible and MWIR
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3-D Barrier to Prevent Glow from Reaching the Detector
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