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Performances of the Imaging Proportional Counter of the Stellar X-ray PolarimeterThe Stellar X-ray Polarimeter (SXRP) will be mounted on the focal plane of one of the two SODART telescopes aboard the Russian mission Spectrum-X-gamma. The SXRP employs the same Imaging Proportional Counters for both the Bragg and the scattering stages. An account is presently given of the main characteristics of these detectors and their performance, on the basis of tests at the technical-model and engineering model levels of development.
Document ID
19930045490
Acquisition Source
Legacy CDMS
Document Type
Conference Paper
Authors
Costa, E. (NASA Headquarters Washington, DC United States)
Di Persio, G. (NASA Headquarters Washington, DC United States)
Feroci, M. (NASA Headquarters Washington, DC United States)
Piro, L. (NASA Headquarters Washington, DC United States)
Martino, B. (NASA Headquarters Washington, DC United States)
Rubini, A. (NASA Headquarters Washington, DC United States)
Soffitta, P. (CNR Ist. di Astrofisica Spaziale, Frascati, Italy)
Massaro, E. (NASA Headquarters Washington, DC United States)
Perola, G. C. (Roma I, Univ. Rome, Italy)
Manzo, G. (CNR Ist. di Fisica Cosmica con Applicazioni all'Informatica, Palermo, Italy)
Date Acquired
August 16, 2013
Publication Date
January 1, 1992
Publication Information
Publication: In: EUV, X-ray, and gamma-ray instrumentation for astronomy III; Proceedings of the Meeting, San Diego, CA, July 22-24, 1992 (A93-29476 10-35)
Publisher: Society of Photo-Optical Instrumentation Engineers
Subject Category
Spacecraft Instrumentation
Accession Number
93A29487
Distribution Limits
Public
Copyright
Other

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