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Multiband Weighting of X-ray Polarization Data

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arxiv 2012.01283 v1 pith:MU4OJL2U submitted 2020-12-02 astro-ph.IM

Multiband Weighting of X-ray Polarization Data

classification astro-ph.IM
keywords datafactorimprovementmodulationpolarizationx-raycountinstrument
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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An optimal estimate for Stokes parameters is derived for the situation in X-ray astronomy where the instrument has a modulation factor that varies significantly with energy but the signals are very weak or mildly polarized. For such sources, the band of analysis may be broadened in order to obtain a significant polarization measurement. Optimal estimators are provided for the cases of binned and unbinned data and applied to data such as might be obtained for faint or weakly polarized sources observed using the Imaging X-ray Polarimetry Explorer (IXPE). For a sample situation, the improvement in the minimum detectable polarization is 6-7% using a count weighted root-mean-square of the modulation factor, when compared to a count weighted average. Improving the modulation factor, such as when using a neural network approach to IXPE event tracks, can provide additional improvement up to 10-15%. The actual improvement depends on the spectral shape and the details of the instrument response functions.

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    Cr/Sc and W/B4C laterally graded multilayer mirrors modulate soft X-ray reflection with polarization angle, showing ~100% modulation at Brewster angle and ~80% at 30° incidence.