English

Broad-Band Soft X-ray Polarimetry

Instrumentation and Methods for Astrophysics 2015-05-13 v1 High Energy Astrophysical Phenomena

Abstract

We developed an instrument design capable of measuring linear X-ray polarization over a broad-band using conventional spectroscopic optics. A set of multilayer-coated flats reflects the dispersed X-rays to the instrument detectors. The intensity variation with position angle is measured to determine three Stokes parameters: I, Q, and U -- all as a function of energy. By laterally grading the multilayer optics and matching the dispersion of the gratings, one may take advantage of high multilayer reflectivities and achieve modulation factors > 50% over the entire 0.2 to 0.8 keV band. This instrument could be used in a small orbiting mission or scaled up for the International X-ray Observatory. Laboratory work has begun that would demonstrate the capabilities of key components.

Keywords

Cite

@article{arxiv.0908.0677,
  title  = {Broad-Band Soft X-ray Polarimetry},
  author = {Herman L. Marshall and Ralf Heilmann and Norbert Schulz and Kendrah Murphy},
  journal= {arXiv preprint arXiv:0908.0677},
  year   = {2015}
}

Comments

6 pages, 3 figures (2 color); to appear in proceedings of "The Coming of Age of X-ray Polarimetry"

R2 v1 2026-06-21T13:32:42.967Z