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(55)Fe X-ray Response of HgCdTe NIR Detector ArraysConversion gain is a fundamental parameter in detector characteristics that is used to measure many identifying detector properties, including read noise, dark current, and quantum efficiency (QE). Charge coupling effects, such as inter-pixel capacitance, attenuate photon shot noise and result in an overestimation of of conversion gain when implementing the photon transfer technique. The (55)Fe X-ray technique is a direct and simple method by which to measure the conversion gain by comparing the observed instrumental counts (ADU) to the known charge (e-) liberated by a single X-ray photon. Here we present the calibrated pair production energy for 1.7 micron HgCdTe infrared detectors.
Document ID
20080047745
Acquisition Source
Goddard Space Flight Center
Document Type
Conference Paper
Authors
Fox, Ori
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Rauscher, Bernard J.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 24, 2013
Publication Date
May 15, 2008
Subject Category
Instrumentation And Photography
Meeting Information
Meeting: SuperNova Acceleratio Probe Collaboration Meeting
Location: Batavia, IL
Country: United States
Start Date: May 15, 2008
End Date: May 17, 2008
Sponsors: California Univ., Lawrence Berkeley National Lab.
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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