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Balloon-borne gamma-ray polarimetry
KTH, School of Engineering Sciences (SCI), Physics, Particle and Astroparticle Physics.ORCID iD: 0000-0001-7011-7229
2011 (English)In: European Space Agency, (Special Publication) ESA SP, 2011Conference paper, Published paper (Refereed)
Abstract [en]

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.

Place, publisher, year, edition, pages
2011.
Series
ESA Special Publications, ISSN 0379-6566 ; 700
Keyword [en]
Astrophysics - Instrumentation and Methods for Astrophysics
National Category
Astronomy, Astrophysics and Cosmology
Identifiers
URN: urn:nbn:se:kth:diva-80146ISI: 000324759000086Scopus ID: 2-s2.0-84859926210ISBN: 978-929092264-3 (print)OAI: oai:DiVA.org:kth-80146DiVA: diva2:496171
Conference
20th ESA Symposium on European Rocket and Balloon Programmes and Related Research. Hyere, France. 22-26 May 2011
Note

QC 20120330

Available from: 2012-02-09 Created: 2012-02-09 Last updated: 2014-10-06Bibliographically approved

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Pearce, Mark

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