Experimental Polarimetric Study of a Hard X-Ray (Articolo in rivista)

Type
Label
  • Experimental Polarimetric Study of a Hard X-Ray (Articolo in rivista) (literal)
Anno
  • 2003-01-01T00:00:00+01:00 (literal)
Alternative label
  • R. M. Curado da Silva, M. Ayoub, E. Caroli, A. Donati, M. Hage-Ali, F. Schiavone, P. Siffert, J. B. Stephen, and (2003)
    Experimental Polarimetric Study of a Hard X-Ray
    in IEEE transactions on nuclear science
    (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#autori
  • R. M. Curado da Silva, M. Ayoub, E. Caroli, A. Donati, M. Hage-Ali, F. Schiavone, P. Siffert, J. B. Stephen, and (literal)
Pagina inizio
  • 1198 (literal)
Pagina fine
  • 1203 (literal)
Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
  • 50 (literal)
Rivista
Note
  • ISI Web of Science (WOS) (literal)
Titolo
  • Experimental Polarimetric Study of a Hard X-Ray (literal)
Abstract
  • Polarimetry in astronomy for the hard X- and soft -ray energy range has not been developed much to date. Indeed no dedicated polarimeters have ever been launched either in space or as a balloon-borne experiment. We propose a polarimetry project for hard X-ray and soft gamma-ray astrophysics known as the Coded Imager and Polarimeter for High Energy Radiation (CIPHER) telescope. The novel design of this telescope, using a matrix of thick CdTe microspectrometers as the detection plane, will allow this type of measurement to be performed for the first time by a dedicated instrument. In order to compare the results already obtained from simulations with experiment, we have constructed a prototype detector of 4x4 pixels, to study the response of this concept of polarimeter to linearly polarized radiation in the 100 keV to 1 MeV energy range. The use of a beamline at the European Synchrotron Radiation Facility (ERSF) allowed us to study double event efficiency and distribution, for beams of nearly 100% linearly polarized radiation in the energy range from 100 keV to 1 MeV. Polarimetric Q factors higher than 0.4 for relative effiencies higher than 20% were observed. The photon beam energy and detector thickness dependencies will be discussed, comparing these experimental results with those calculated by Monte Carlo simulations. (literal)
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