Beam test of a prototype phoswich detector assembly for the PoGOLite astronomical soft gamma-ray polarimeter
Creators
- Kanai, Y.1
- Ueno, M.1
- Kataoka, J.1
- Arimoto, M.1
- Kawai, N.1
- Yamamoto, K.2
- Mizuno, T.2
- Fukazawa, Y.2
- Kiss, M.3
- Ylinen, T.3
- Marini Bettolo, C.3
- Carlson, P.3
- Klamra, W.3
- Pearce, M.3
- Chen, P.4
- Craig, B.4
- Kamae, T.4
- Madejski, G.4
- Ng, J.S.T.4
- Rogers, R.4
- Tajima, H.4
- Thurston, T.S.4
- Saito, Y.5
- Takahashi, T.5
- Gunji, S.6
- Bjornsson, C.-I.7
- Larsson, S.7
- Ryde, F.7
- Bogaert, G.8
- Kishimoto, S.9
- 1. Tokyo Institute of Technology, 2-12-1 Ookayama, Meguro, Tokyo 152-8551 (Japan)
- 2. Hiroshima University, Higashi-Hiroshima (Japan)
- 3. Royal Institute of Technology, Stockholm (Sweden)
- 4. Stanford Linear Accelerator Center, Menlo Park, CA (United States)
- 5. Institute of Space and Astronautical Science, Japan Aerospace Exploration Agency, Sagamihara (Japan)
- 6. Yamagata University, Yamagata (Japan)
- 7. Stockholm University, Stockholm (Sweden)
- 8. Ecole Polytechnique, Palaiseau (France)
- 9. Institute of Materials Structure Science, High Energy Accelerator Research Organization, Tsukuba (Japan)
Description
We report about the beam test on a prototype of the balloon-based astronomical soft gamma-ray polarimeter, PoGOLite (Polarized Gamma-ray Observer - Light Version) conducted at KEK Photon Factory, a synchrotron radiation facility in Japan. The synchrotron beam was set at 30, 50, and 70 keV and its polarization was monitored by a calibrated polarimeter. The goal of the experiment was to validate the flight design of the polarimeter. PoGOLite is designed to measure polarization by detecting a Compton scattering and the subsequent photo-absorption in an array of 217 well-type phoswich detector cells (PDCs). The test setup included a first flight model PDC and a front-end electronics to select and reconstruct valid Compton scattering events. The experiment has verified that the flight PDC can detect recoil electrons and select valid Compton scattering events down to 30 keV from background. The measure azimuthal modulations (34.4%, 35.8% and 37.2% at 30, 50, and 70 keV, respectively) agreed within 10% (relative) with the predictions by Geant4 implemented with dependence on the initial and final photon polarizations
Additional details
Identifiers
- DOI
- 10.1016/j.nima.2006.09.109;
- PII
- S0168-9002(06)01756-6;
Publishing Information
- Journal Title
- Nuclear Instruments and Methods in Physics Research. Section A, Accelerators, Spectrometers, Detectors and Associated Equipment
- Journal Volume
- 570
- Journal Issue
- 1
- Journal Page Range
- p. 61-71
- ISSN
- 0168-9002
- CODEN
- NIMAER
INIS
- Country of Publication
- Netherlands
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38038284
- Subject category
- S46: INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY;
- Descriptors DEI
- BALLOONS; BEAMS; COMPTON EFFECT; DESIGN; GAMMA RADIATION; HARD X RADIATION; KEK PHOTON FACTORY; KEV RANGE 10-100; POLARIMETERS; POLARIZATION; SYNCHROTRON RADIATION; TESTING
- Descriptors DEC
- AIRCRAFT; BASIC INTERACTIONS; BREMSSTRAHLUNG; ELASTIC SCATTERING; ELECTROMAGNETIC INTERACTIONS; ELECTROMAGNETIC RADIATION; ENERGY RANGE; INTERACTIONS; IONIZING RADIATIONS; KEV RANGE; RADIATION SOURCES; RADIATIONS; SCATTERING; SYNCHROTRON RADIATION SOURCES; X RADIATION
Optional Information
- Copyright
- Copyright (c) 2006 Elsevier Science B.V., Amsterdam, The Netherlands, All rights reserved.