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7 - The GPD as a polarimeter: theory and facts

from Part I - Polarimetry techniques

Published online by Cambridge University Press:  06 July 2010

P. Soffitta
Affiliation:
Iasf-Roma/Inaf, Italy
E. Costa
Affiliation:
Iasf-Roma/Inaf, Italy
S. Fabiani
Affiliation:
Iasf-Roma/Inaf, Italy
F. Lazzarotto
Affiliation:
Iasf-Roma/Inaf, Italy
F. Muleri
Affiliation:
Iasf-Roma/Inaf, Italy
A. Rubini
Affiliation:
Iasf-Roma/Inaf, Italy
R. Bellazzini
Affiliation:
Infn-Pisa, Italy
A. Brez
Affiliation:
Infn-Pisa, Italy
M. Minuti
Affiliation:
Infn-Pisa, Italy
M. Pinchera
Affiliation:
Infn-Pisa, Italy
G. Spandre
Affiliation:
Infn-Pisa, Italy
Ronaldo Bellazzini
Affiliation:
Istituto Nazionale di Fisica Nucleare (INFN), Rome
Enrico Costa
Affiliation:
Istituto Astrofisica Spaziale, Rome
Giorgio Matt
Affiliation:
Università degli Studi Roma Tre
Gianpiero Tagliaferri
Affiliation:
Osservatorio Astronomico di Brera
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Summary

The advent of a new generation of X-ray polarimeters based on the photoelectric effect poses the problem of their calibration. We devised and built a calibration facility aimed at the study of the performances of photoelectric X-ray polarimeters such as the Gas Pixel Detector (GPD). The calibration facility exploits the 45° Bragg diffraction from crystals of both X-ray lines characteristic of X-ray tubes and from continuum. A set of linear and rotary stages allows the GPD to be calibrated on its whole surface. We successfully tested the GPD filled with a mixture of He-DME 30-70 at one atmosphere. We measured the modulation factor at 2.69 keV and 4.51 keV. We also studied the homogeneity of the modulation factor, of the angular phase and of the position reconstruction capability on the surface of the GPD.

Introduction

Since early 2000 we have been developing true 2-D X-ray polarimeters based on the photoelectric effect. The Gas Pixel Detector (GPD), an evolution based on the use of an ASICCMOS readout chip, has been calibrated at energies greater then 5 keV with a Thomson based X-ray polarizer. However, the sensitivity of the GPD at the focus of conventional X-ray optics peaks below 5 keV. In this regime the photoelectric effect severely competes with Thomson scattering. For this reason we developed a facility aimed at the production of polarized X-rays in the few keV band.

Type
Chapter
Information
X-ray Polarimetry
A New Window in Astrophysics
, pp. 54 - 59
Publisher: Cambridge University Press
Print publication year: 2010

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