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HyViSI Array Formats Ground-based Astronomy (Rochester Institute of Technology) Mars Reconnaissance Orbiter (MRO) Crab Nebula (M1) NGC2683 Spiral Galaxy Hercules Cluster (M13) TCM 6604A 640×480 pixels 27 µm pitch CTIA 1K×1K H1RG-18 2K×2K H2RG-18 4K×4K H4RG-10 J-MAPS Astrometry Mission 4K×4K H4RG-10 Mosaic of 4 arrays TEC Package by Judson 42
HAWAII-2RG 2048×2048 pixels HAWAII-2RG (H2RG) • 2048×2048 pixels, 18 micron pitch • 1, 2, 4, 32 ports • “R” = reference pixels (4 rows/cols at edge) • “G” = guide window • Low power:
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 38 and 39: Reduction of noise from multiple sa
Page 40 and 41: High Performance Hybrid CMOS Arrays
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

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