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Hubble Space Telescope Wide Field Camera 3 H1-R Quantum Efficiency = 85-90% Dark current (145K) = 0.02 e-/pix/sec Readout noise = 25 e- (single CDS) GSFC DCL Measurement • 1024×1024 pixels, 18.5 micron pitch • Substrate-removed 1.7 μm HgCdTe arrays • Nearly 30x increase in HST discovery efficiency
<strong>James</strong> Webb Space Telescope (JWST)
Page 1 and 2: High Performance Imaging Sensors fo
Page 3: Hubble Space Telescope
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 38 and 39: Reduction of noise from multiple sa
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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