2011
DOI: 10.5194/astra-7-43-2011
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POLAR: A Space-borne X-Ray Polarimeter for Transient Sources

Abstract: Abstract. POLAR is a novel compact Compton X-ray polarimeter designed to measure the linear polarization of the prompt emission of Gamma Ray Bursts (GRB) and other strong transient sources such as soft gamma repeaters and solar flares in the energy range 50−500 keV. A detailed measurement of the polarization from astrophysical sources will lead to a better understanding of the source geometry and emission mechanisms. POLAR is expected to observe every year several GRBs with a minimum detectable polarization sm… Show more

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Cited by 10 publications
(2 citation statements)
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“…One of the most significant obstacles has been the scarcity of polarization data for GRBs due to the unfortunately small number of orbital polarimeters and the typical difficulties in observing these luminous events. Despite that, advances have been made in the area, and thanks to efforts like the POLAR project (Orsi 2011), it is expected that in future years we should have an abundance of data for the test of different models.…”
Section: Introductionmentioning
confidence: 99%
“…One of the most significant obstacles has been the scarcity of polarization data for GRBs due to the unfortunately small number of orbital polarimeters and the typical difficulties in observing these luminous events. Despite that, advances have been made in the area, and thanks to efforts like the POLAR project (Orsi 2011), it is expected that in future years we should have an abundance of data for the test of different models.…”
Section: Introductionmentioning
confidence: 99%
“…Though photoelectric polarimeters are expected to provide sensitive polarization measurements, these instruments are effective primarily in soft X-rays where radiation from the source is expected to be less polarized because of the dominance of thermal radiation. Consequently, many groups across the globe are now involved in developing Compton polarimeters effective in hard X-ray regime where the expected polarization is above the typical sensitivity level of the instruments [56,31,29,8,40]. For the same reason, there have been several attempts during the last decade in retrieving polarization information from instruments, not specifically designed for polarimetry but could be sensitive to it [35,14,33,27,19,17,38,21,20,36,37,32,12,50].…”
Section: Introductionmentioning
confidence: 99%