Astronomy and Astrophysics – Astronomy
Scientific paper
Jul 2006
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2006spie.6276e..31k&link_type=abstract
High Energy, Optical, and Infrared Detectors for Astronomy II. Edited by Dorn, David A.; Holland, Andrew D.. Proceedings of th
Astronomy and Astrophysics
Astronomy
Scientific paper
We developed the new readout system for the pixel-readout μ-PIC (micro pixel chamber), which is one of the micro-pattern gas detectors that have been developed as a X-ray polarimeter so far. By using this system, we succeeded in achieving the sensitivity predicted by the simulation, i.e, the modulation factors, which is one of the most important factors for X-ray polarimeter as defined later in this paper, 0.24+/-0.08 at 8 keV, 0.18+/-0.07 at 15 keV in the neon-based gas mixture, and 0.18+/-0.04 in the argon-based gas although there still remain problems such as the pitch size among pixels and the non-uniformity of the response.
Hyodo Yosiaki
Katagiri Hideaki
Kubo Hidetoshi
Matsumoto Hironori
Miuchi Kentaro
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