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X-ray timing explorer missionThe XTE will address a number of fundamental questions about the nature of the cosmos. The large effective area (about 0.8 sq m total) and broad band of sensitivity (2-200 keV) of its three instruments make it especially valuable for timing of intensity variations and for the determination of broadband spectra from high-energy sources. For the first time, studies of variability ranging from about 1 microsecond to several years will be carried out. XTE's design and flexibility of operations will allow it to respond rapidly to changes in the X-ray sky (within hours) and will facilitate multifrequency observations. It is scheduled for launch on a Delta II vehicle prior to April 1996.
Document ID
19930044962
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Bradt, H. V.
(MIT Cambridge, MA, United States)
Rothschild, R. E.
(California Univ. La Jolla, United States)
Swank, J. H.
(NASA Goddard Space Flight Center Greenbelt, MD, United States)
Date Acquired
August 16, 2013
Publication Date
January 1, 1993
Publication Information
Publication: Astronomy and Astrophysics Supplement Series
Volume: 97
Issue: 1
ISSN: 0365-0138
Subject Category
Astronomy
Report/Patent Number
ISSN: 0365-0138
Accession Number
93A28959
Distribution Limits
Public
Copyright
Other

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