Status of the stellar x-ray polarimeter for the Spectrum-X-Gamma mission

Philip E. Kaaret, Robert Novick, Ping Shine Shaw, Shaul Hanany, Yee Liu, Judith R. Fleischman, Rashid Sunyaev, I. Lapshov, Martin C. Weisskopf, Ronald F. Elsner, Brian D. Ramsey, Eric H. Silver, Klaus P. Ziock, Enrico Costa, Luigi Piro, Salvatore Giarrusso, Andrea E. Santangelo, Livio Scarsi, George W. Fraser, James F. PearsonJohn E. Lees, G. C. Perola, Enrico Massaro, Giorgio Matt

Research output: Chapter in Book/Report/Conference proceedingConference contribution

4 Scopus citations

Abstract

The Stellar x-ray polarimeter (SXRP) uses the polarization sensitivity of a graphite Bragg crystal and a lithium Thomson scattering target to measure the polarization of x-rays from astrophysical sources. The SXRP is a focal plane detector for the Soviet-Danish SODART telescopes that will be launched on the Soviet Spectrum-X-Gamma mission. The SCRP will be the third orbiting stellar x-ray polarimeter and should provide an order of magnitude increase in polarization sensitivity over it predecessors.

Original languageEnglish (US)
Title of host publicationProceedings of SPIE - The International Society for Optical Engineering
PublisherPubl by Int Soc for Optical Engineering
Pages106-117
Number of pages12
ISBN (Print)0819406767
StatePublished - Dec 1 1991
Externally publishedYes
EventProduction and Analysis of Polarized X Rays - San Diego, CA, USA
Duration: Jul 23 1991Jul 24 1991

Publication series

NameProceedings of SPIE - The International Society for Optical Engineering
Volume1548
ISSN (Print)0277-786X

Other

OtherProduction and Analysis of Polarized X Rays
CitySan Diego, CA, USA
Period7/23/917/24/91

Fingerprint

Dive into the research topics of 'Status of the stellar x-ray polarimeter for the Spectrum-X-Gamma mission'. Together they form a unique fingerprint.

Cite this