An Unfolding Method for X-ray Spectro-Polarimetry
arXiv:1411.5037 · doi:10.1016/j.astropartphys.2014.11.003
Abstract
X-ray polarimetry has great scientific potential and new experiments, such as X-Calibur, PoGOLite, XIPE, and GEMS, will not only be orders of magnitude more sensitive than previous missions, but also provide the capability to measure polarization over a wide energy range. However, the measured spectra depend on the collection area, detector responses, and, in case of balloon-borne experiments, the absorption of X-rays in the atmosphere, all of which are energy dependent. Combined with the typically steep source spectra, this leads to significant biases that need to be taken into account to correctly reconstruct energy-resolved polarization properties. In this paper, we present a method based on an iterative unfolding algorithm that makes it possible to simultaneously reconstruct the energy spectrum and the polarization properties as a function of true photon energy. We apply the method to a simulated X-Calibur data set and show that it is able to recover both the energy spectrum and the energy-dependent polarization fraction.
arXiv comment12 pages, 7 figures, accepted for publication in Astropart. Phys
References in corpus (6)
- The 22-Month Swift-BAT All-Sky Hard X-ray Survey
- Polarization of the Crab pulsar and nebula as observed by the Integral/IBIS telescope
- XIPE: the X-ray Imaging Polarimetry Explorer
- Scientific Prospects for Hard X-ray Polarimetry
- Optimization of the Design of the Hard X-ray Polarimeter X-Calibur
- Balloon-borne hard X-ray polarimetry with PoGOLite
Cited by in corpus (6)
- Analyzing the Data from X-ray Polarimeters with Stokes Parameters
- Determination of X-ray pulsar geometry with IXPE polarimetry
- X-ray Spectro-polarimetry with Photoelectric Polarimeters
- Complex variations of X-ray polarization in the X-ray pulsar LS V +44 17/RX J0440.9+4431
- Performance of the X-Calibur Hard X-Ray Polarimetry Mission during its 2018/19 Long-Duration Balloon Flight
- Properties of magneto-dipole X-ray lines in different radiation models