Dr. Suresh Seshadri
Senior Engineer at JPL
SPIE Involvement:
Author
Publications (9)

PROCEEDINGS ARTICLE | August 6, 2010
Proc. SPIE. 7731, Space Telescopes and Instrumentation 2010: Optical, Infrared, and Millimeter Wave
KEYWORDS: Staring arrays, Thermography, Near infrared, Monochromatic aberrations, Point spread functions, Electronics, Sensors, Interfaces, Photometry, Galactic astronomy

PROCEEDINGS ARTICLE | July 22, 2008
Proc. SPIE. 7021, High Energy, Optical, and Infrared Detectors for Astronomy III
KEYWORDS: Staring arrays, Infrared imaging, Point spread functions, Visible radiation, Imaging systems, Sensors, Diffusion, Capacitance, Infrared radiation, Multiplexers

PROCEEDINGS ARTICLE | September 14, 2007
Proc. SPIE. 6690, Focal Plane Arrays for Space Telescopes III
KEYWORDS: Staring arrays, Near infrared, Indium gallium arsenide, Mercury cadmium telluride, Imaging systems, Sensors, Quantum efficiency, Data conversion, Multiplexers, Imaging arrays

PROCEEDINGS ARTICLE | July 5, 2006
Proc. SPIE. 6265, Space Telescopes and Instrumentation I: Optical, Infrared, and Millimeter
KEYWORDS: Near infrared, Point spread functions, Optical filters, Mercury cadmium telluride, Radon, Sensors, Error analysis, Quantum efficiency, Space telescopes, Detector development

PROCEEDINGS ARTICLE | June 20, 2006
Proc. SPIE. 6276, High Energy, Optical, and Infrared Detectors for Astronomy II
KEYWORDS: Signal to noise ratio, Near infrared, Mercury cadmium telluride, Statistical analysis, Sensors, Video, Interference (communication), Amplifiers, Capacitance, Multiplexers

PROCEEDINGS ARTICLE | June 20, 2006
Proc. SPIE. 6276, High Energy, Optical, and Infrared Detectors for Astronomy II
KEYWORDS: Near infrared, Indium gallium arsenide, Mercury cadmium telluride, Imaging systems, Sensors, Quantum efficiency, Sensor performance, Detector development, Data conversion, Multiplexers

Showing 5 of 9 publications
SIGN IN TO:
  • View contact details

UPDATE YOUR PROFILE
Is this your profile? Update it now.
Don’t have a profile and want one?

Back to Top