Wide-Field X-ray Polarimetry for High Energy Astronomical Transients: First results of the pathfinder CXPD Cubesat Mission
Hong-Bang Liu, Zu-Ke Feng, Huan-Bo Feng, Di-Fan Yi, Li-Rong Xie, Yan-Jun Xie, Zong-Wang Fan, Jin Zhang, Wen-Jin Xie, Xue-Feng Huang, Wei Deng, Fei Xie, Dong Wang, Zi-Li Li, Hui Wang, Ran Chen, Shi-Qiang Zhou, Kai Chen, Jin Li, Qian Liu, Shi Chen, Rui-Ting Ma, Bin-Long Wang

TL;DR
The CXPD CubeSat successfully demonstrated in-orbit X-ray polarization measurements of bright sources, validating key technologies for future wide-field soft X-ray polarimetry missions like POLAR-2.
Contribution
This work presents the first in-orbit validation of a wide-field X-ray polarimeter prototype with innovative anti-coincidence detection technology.
Findings
Successful in-orbit polarization measurements of Sco X-1 and Swift J1727.8-1613.
First implementation of anti-coincidence detector in an X-ray polarimeter.
Validation of background rejection algorithms in space environment.
Abstract
The Low Energy Polarization Detector (LPD) is a key component of the next-generation large-scale Gamma-Ray Burst polarimeter, POLAR-2. It is designed for polarization observations of transient sources in the soft X-ray energy range with a wide field of view (FOV). To validate the key technologies required for wide-FOV X-ray polarization measurements, the Cosmic X-ray Polarization Detector (CXPD) CubeSat was developed as a prototype for the LPD. The CXPD is equipped with two Gas Microchannel Plate Pixel Detectors (GMPDs) that measure X-ray polarization via the photoelectric effect, where ejected photoelectrons produce ionization tracks in the gas which are imaged to reconstruct their emission directions. Laboratory calibrations of the modulation factor and energy spectra were successfully performed using linear polarized X-ray sources at 2.98 keV, 4.51 keV, 6.40 keV, and 8.05 keV. Since…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Particle Detector Development and Performance · Astrophysical Phenomena and Observations
