http://www.cnr.it/ontology/cnr/individuo/prodotto/ID5694
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
- Pagina fine
- Http://www.cnr.it/ontology/cnr/pubblicazioni.owl#numeroVolume
- 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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