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The direct deconvolution of X-ray spectraThe method of deconvolution of proportional counter X-ray spectra as outlined by Blissett and Cruise is reviewed with particular emphasis on low-energy spectra. This method involves the expansion of the incident spectrum in terms of a set of orthonormal singular functions which propagate independently through the detector matrix. When applied to low-energy detectors which typically exhibit absorption features in their efficiency curves, the initial Blissett and Cruise prescription is shown to be unstable. Alternative methods for handling the efficiency are described and evaluated. In the deconvolution of steep spectra, additional distortions are shown to arise as a result of sidelobe oscillations in the effective response functions. A selective weighting procedure is thus introduced to suppress spurious features of this type. Finally, the role of filtering in the deconvolution procedure is discussed and several suitable forms for the filter are suggested.
Document ID
19800056502
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Kahn, S. M.
(California, University Berkeley, Calif., United States)
Blissett, R. J.
(London, University College, Mullard Space Science Laboratory, Dorking, Surrey, United Kingdom)
Date Acquired
August 10, 2013
Publication Date
May 15, 1980
Publication Information
Publication: Astrophysical Journal
Subject Category
Astronomy
Accession Number
80A40672
Funding Number(s)
CONTRACT_GRANT: CIT-44-466866
Distribution Limits
Public
Copyright
Other

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