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arxiv: 1208.0610 · v1 · pith:2OOCYBCFnew · submitted 2012-08-02 · 🌌 astro-ph.IM · hep-ex

Measuring x-ray polarization in the presence of systematic effects: Known background

classification 🌌 astro-ph.IM hep-ex
keywords polarizationx-raymeasurementsassociatedbackgroundhiatuspresencesources
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The prospects for accomplishing x-ray polarization measurements of astronomical sources have grown in recent years, after a hiatus of more than 37 years. Unfortunately, accompanying this long hiatus has been some confusion over the statistical uncertainties associated with x-ray polarization measurements of these sources. We have initiated a program to perform the detailed calculations that will offer insights into the uncertainties associated with x-ray polarization measurements. Here we describe a mathematical formalism for determining the 1- and 2-parameter errors in the magnitude and position angle of x-ray (linear) polarization in the presence of a (polarized or unpolarized) background. We further review relevant statistics-including clearly distinguishing between the Minimum Detectable Polarization (MDP) and the accuracy of a polarization measurement.

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