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Gamma-ray burst astrometry III - More resultsIn continuation of previous work, new computations are presented for the PVO/Ulysses/GRO/GRANAT case. Since timing errors dominate this problem, error distributions are computed analytically for the source position direction cosines. Taff's method is shown to be numerically robust, accurate, and analytically convenient.
Document ID
19930056117
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Taff, L. G.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Holfeltz, S. T.
(Space Telescope Science Inst. Baltimore, MD, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: Gamma-ray bursts; Proceedings of the Workshop, Univ. of Alabama, Huntsville, Oct. 16-18, 1991 (A93-40051 16-93)
Publisher: American Institute of Physics
Subject Category
Astronomy
Accession Number
93A40114
Funding Number(s)
CONTRACT_GRANT: NAS5-26555
Distribution Limits
Public
Copyright
Other

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