Balloon-borne gamma-ray polarimetry
Mark Pearce (for the PoGOLite Collaboration)

TL;DR
This paper introduces PoGOLite, a balloon-borne instrument designed to measure gamma-ray polarization in the 25-80 keV range, aiming to study high-energy astrophysical sources.
Contribution
It presents the design and planned deployment of a novel balloon-borne gamma-ray polarimeter utilizing Compton scattering for polarization measurement.
Findings
Design of a polarimeter with plastic and BGO scintillators
Scheduled maiden flight in summer 2011 from Esrange
Targeting Crab and Cygnus X-1 for polarization observations
Abstract
The physical processes postulated to explain the high-energy emission mechanisms of compact astrophysical sources often yield polarised soft gamma rays (X-rays). PoGOLite is a balloon-borne polarimeter operating in the 25-80 keV energy band. The polarisation of incident photons is reconstructed using Compton scattering and photoelectric absorption in an array of phoswich detector cells comprising plastic and BGO scintillators, surrounded by a BGO side anticoincidence shield. The polarimeter is aligned to observation targets using a custom attitude control system. The maiden balloon flight is scheduled for summer 2011 from the Esrange Space Centre with the Crab and Cygnus X-1 as the primary observational targets.
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Taxonomy
TopicsParticle Detector Development and Performance · Gamma-ray bursts and supernovae · Astrophysics and Cosmic Phenomena
