Dichroic Filters For Astronomical X-Ray Polarimetry

被引:0
|
作者
N. P. Bannister
K. D. M. Harris
S. P. Collins
A. Martindale
P. S. Monks
G. Solan
G. W. Fraser
机构
[1] University of Leicester,Space Research Centre, Department of Physics and Astronomy
[2] Cardiff University,School of Chemistry, Main Building
[3] Rutherford Appleton Laboratory,Diamond Light Source Ltd
[4] University of Leicester,Department of Chemistry
来源
Experimental Astronomy | 2006年 / 21卷
关键词
Instrumentation; X-ray polarimetry; X-ray dichroism;
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学科分类号
摘要
We describe a programme of research to investigate materials which exhibit linear dichroism at X-ray wavelengths, and to assess their potential as astronomical X-ray polarimeters. The availability of polarising filters for X-rays would offer an efficient method of quantifying the polarisation of X-ray radiation from distant, cosmic sources. A polarising dichroic filter is expected to be a compact, low mass device which could add polarimetry capability to an instrument by being introduced into the optical path ahead of a detector. We provide estimates of sensitivity in the context of the proposed XEUS observatory, which compare favourably with those for the most promising alternative technology. We also discuss a number of astrophysical sources which are suited to polarimetric study at discrete energies offered by the X-ray dichroic filter design.
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页码:1 / 12
页数:11
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