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Analysis of observational spectraThe first step in the analysis of gamma ray energy loss spectra is their conversion to differential energy and differential angular photon spectra. This conversion can be carried out if the detector response and the background are both known. Once these parameters are known, there are many techniques that can be used to convert pulse height spectra to photon spectra. These techniques are discussed and background problems are considered. Emphasis is placed on the analysis of energy loss spectra in the lower gamma ray energy domain. Problems of transportations from pulse height to photon space are most complex in this domain and the methods shown illustrate many of the problems which arise in the general analysis of energy loss spectra.
Document ID
19820013257
Acquisition Source
Legacy CDMS
Document Type
Other
Date Acquired
August 10, 2013
Publication Date
January 1, 1981
Publication Information
Publication: Gamma Ray Astrophys.
Subject Category
Astrophysics
Accession Number
82N21131
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.

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