X-ray Polarimetry: a new window on the high energy sky
Ronaldo Bellazzini, Fabio Muleri

TL;DR
X-ray polarimetry, crucial for understanding high-energy astrophysical objects, has been limited by instrumentation but recent advances in detector technology now enable effective polarization measurements.
Contribution
The paper reports on the performance of a new imaging X-ray polarimeter based on photoelectric effect, enhancing capabilities for X-ray polarization measurements.
Findings
High sensitivity of the Gas Pixel Detector for polarization detection
Simultaneous imaging, moderate spectroscopy, and high-rate timing capabilities
Potential for future satellite missions to explore X-ray polarimetry
Abstract
Polarimetry is widely considered a powerful observational technique in X-ray astronomy, useful to enhance our understanding of the emission mechanisms, geometry and magnetic field arrangement of many compact objects. However, the lack of suitable sensitive instrumentation in the X-ray energy band has been the limiting factor for its development in the last three decades. Up to now, polarization measurements have been made exclusively with Bragg diffraction at 45 degrees or Compton scattering at 90 degrees and the only unambiguous detection of X-ray polarization has been obtained for one of the brightest object in the X-ray sky, the Crab Nebula. Only recently, with the development of a new class of high sensitivity imaging detectors, the possibility to exploit the photoemission process to measure the photon polarization has become a reality. We will report on the performance of an…
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