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Träfflista för sökning "WFRF:(Bjornsson P.) srt2:(2005-2009)"

Sökning: WFRF:(Bjornsson P.) > (2005-2009)

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1.
  • Andersson, V., et al. (författare)
  • Large-Area Balloon-Borne Polarized Gamma Ray Observer (PoGO)
  • 2005
  • Ingår i: Proceedings of the 22nd Texas Symposium on Relativistic Astrophysics at Stanford. ; , s. 736-743
  • Konferensbidrag (refereegranskat)abstract
    • We are developing a new balloon-borne instrument (PoGO), to measure polarization of soft gamma rays (30-200 keV) using asymmetry in azimuth angle distribution of Compton scattering. PoGO is designed to detect 10 % polarization in 100mCrab sources in a 6-8 hour observation and bring a new dimension to studies on gamma ray emission/transportation mechanism in pulsars, AGNs, black hole binaries, and neutron star surface. The concept is an adaptation to polarization measurements of well-type phoswich counter consisting of a fast plastic scintillator (the detection part), a slow plastic scintillator (the active collimator) and a BGO scintillator (the bottom anti-counter). PoGO consists of close-packed array of 217 hexagonal well-type phoswich counters and has a narrow field-of-view (~ 5 deg2) to reduce possible source confusion. A prototype instrument has been tested in the polarized soft gamma-ray beams at Advanced Photon Source (ANL) and at Photon Factory (KEK). On the results, the polarization dependence of EGS4 has been validated and that of Geant4 has been corrected.
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  • Arimoto, M., et al. (författare)
  • Performance assessment study of the balloon-borne astronomical soft gamma-ray polarimeter PoGOLite
  • 2007
  • Ingår i: Physica. E, Low-Dimensional systems and nanostructures. - : Elsevier BV. - 1386-9477 .- 1873-1759. ; 40:2, s. 438-441
  • Tidskriftsartikel (refereegranskat)abstract
    • Measurements of polarization play a crucial role in the understanding of the dominant emission mechanism of astronomical sources. Polarized Gamma-ray Observer-Light version (PoGOLite) is a balloon-borne astronomical soft gamma-ray polarimeter at the 25-80 keV band. The PoGOLite detector consists of a hexagonal close-packed array of 217 Phoswich detector cells (PDCs) and side anti-coincidence shields (SASs) made of BGO crystals surrounding PDCs. Each PDC consists of a slow hollow scintillator, a fast scintillator and a BGO crystal that connects to a photomultiplier tube at the end. To examine the PoGOLite's capability and estimate the performance, we conducted experiments with the PDC using radioisotope 241Am. In addition, we compared this result with performance expected by Monte Carlo simulation with Geant4. As a result, we found that the actual PDC has the capability to detect a 100 m Crab source until 80 keV.
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  • Werner, M, et al. (författare)
  • Autoimmune hepatitis in Sweden.
  • 2007
  • Ingår i: SCANDINAVIAN JOURNAL OF GASTROENTEROLOGY. - 0036-5521. ; 42, s. 15-15
  • Konferensbidrag (övrigt vetenskapligt/konstnärligt)
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  • Resultat 1-8 av 8

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