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Detector noise statistics in the non-linear regimeThe statistical behavior of an idealized linear detector in the presence of threshold and saturation levels is examined. It is assumed that the noise is governed by the statistical fluctuations in the number of photons emitted by the source during an exposure. Since physical detectors cannot have infinite dynamic range, our model illustrates that all devices have non-linear regimes, particularly at high count rates. The primary effect is a decrease in the statistical variance about the mean signal due to a portion of the expected noise distribution being removed via clipping. Higher order statistical moments are also examined, in particular, skewness and kurtosis. In principle, the expected distortion in the detector noise characteristics can be calibrated using flatfield observations with count rates matched to the observations. For this purpose, some basic statistical methods that utilize Fourier analysis techniques are described.
Document ID
19940018053
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Shopbell, P. L.
(Rice Univ. Houston, TX, United States)
Bland-Hawthorn, J.
(Rice Univ. Houston, TX, United States)
Date Acquired
September 6, 2013
Publication Date
January 1, 1992
Publication Information
Publication: NASA, Washington, Second Annual Conference on Astronomical Data Analysis Software and Systems. Abstracts
Subject Category
Communications And Radar
Accession Number
94N22526
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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