首页 | 本学科首页   官方微博 | 高级检索  
     检索      


A scattering polarimeter for X-ray astronomy
Authors:E Costa  A Emanuele  A Rubini  E Massaro  G Matt  G Medici  G C Perola and M Salvati
Institution:(1) Istituto di Astrofisica Spaziale, C.N.R., Via E. Fermi 23, 00044 Frascati;(2) Istituto Astronomico, Università ?La Sapienza?, Via G. Lancisi 29, 00161 Roma;(3) Osservatorio Astrofisico di Arcetri, Largo E. Fermi 5, 50125 Firenze
Abstract:Summary We describe a high sensitivity X-ray Thomson polarimeter for astrophysical research, particularly designed for the XMM mission. The efficiency, the modulation factor and the performances of this instrument have been estimated by means of a Monte Carlo simulation. The predicted sensitivity for the high eccentricity Orbit of XMM should allow the detection of the Crab Nebula polarization (3σ, (5÷11)keV) in 15 seconds only. To speed up publication, the proofs were not sent to the authors and were supervised by the Scientific Committee.
Keywords:Cosmic rays
本文献已被 SpringerLink 等数据库收录!
设为首页 | 免责声明 | 关于勤云 | 加入收藏

Copyright©北京勤云科技发展有限公司  京ICP备09084417号