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Reduction of noise from multiple samples Non-destructive readout enables reduction of noise from multiple samples H2RG array 2.5 micron cutoff Temperature = 77K Measured Simple Theory (no 1/f noise) CDS = correlated double sample 38
Pixel Amplifier Options 39
Page 1 and 2: High Performance Imaging Sensors fo
Page 3 and 4: Hubble Space Telescope
Page 5 and 6: James Webb Space Telescope (JWST)
Page 7 and 8: NASA’s s Partner for Earth Scienc
Page 9 and 10: Orbiting Carbon Observatory (OCO) T
Page 11: The Technologies of High Performanc
Page 15 and 16: Hybrid CMOS Infrared Imaging Sensor
Page 17: Crystals are excellent detectors of
Page 20 and 21: Tunable Wavelength: Unique property
Page 22 and 23: Molecular Beam Epitaxy (MBE) Growth
Page 24 and 25: 6 Steps of CMOS-based Optical / IR
Page 26 and 27: Hybrid Imager Architecture HgCdTe l
Page 28 and 29: Quantum Efficiency of substrate-rem
Page 30 and 31: Dark Current Undesirable byproduct
Page 32 and 33: 6 Steps of CMOS-based Optical / IR
Page 34 and 35: IR multiplexer pixel architecture V
Page 36 and 37: IR multiplexer pixel architecture V
Page 40 and 41: High Performance Hybrid CMOS Arrays
Page 42 and 43: HyViSI Array Formats Ground-based A
Page 44 and 45: The SIDECAR ASIC - Focal Plane Elec
Page 46 and 47: Hubble Space Telescope Advanced Cam
Page 48 and 49: SIDECAR ASIC & large mosaic focal p
Page 50: Teledyne Enabling humankind to unde

James Beletic's presentation

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