Gamma-ray Polarimetry of Transient Sources with POLAR
Merlin Kole, Jianchao Sun

TL;DR
POLAR is a dedicated gamma-ray polarimeter designed to measure the polarization of transient sources like Gamma-Ray Bursts, overcoming challenges of low signal-to-noise and systematic errors through careful calibration and analysis methods.
Contribution
This paper introduces the POLAR instrument and its calibration, along with two analysis methods to improve polarization measurement sensitivity for transient gamma-ray sources.
Findings
POLAR observed 55 Gamma-Ray Bursts in orbit.
14 bursts allowed for polarization constraints.
Two analysis methods were developed and described.
Abstract
Polarization measurements of the gamma-ray component of transient sources are of great scientific interest, they are however, also highly challenging. This is due to the typical low signal to noise and the potential for significant systematic errors. Both issues are made worse by the transient nature of the events which prompt one to observe a large portion of the sky. The POLAR instrument was designed as a dedicated transient gamma-ray polarimeter. It made use of a large effective area and large field of view to maximize the signal to noise as well as the number of observed transients. Additionally, it was calibrated carefully on ground and in orbit to mitigate systematic errors. The main scientific goal of POLAR was to measure the polarization of the prompt emission of Gamma-Ray Bursts. During the 6 months operation in orbit POLAR observed 55 Gamma-Ray Bursts of which 14 were bright…
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Taxonomy
TopicsGamma-ray bursts and supernovae · Nuclear Physics and Applications
