An X-ray polarimeter for hard X-ray optics

被引：2

作者：

Muleri, Fabio ^{[1
]}

Bellazzini, Ronaldo ^{[1
]}

Costa, Enrico ^{[1
]}

Soffitta, Paolo ^{[1
]}

Lazzarotto, Francesco ^{[1
]}

Feroci, Marco ^{[1
]}

Pacciani, Luigi ^{[1
]}

Rubini, Alda ^{[1
]}

Morelli, Ennio ^{[1
]}

Baldini, Luca ^{[1
]}

Bitti, Francesco ^{[1
]}

Brez, Alessandro ^{[1
]}

Cavalca, Francesco ^{[1
]}

Latronic, Luca ^{[1
]}

Massai, Marco Maria ^{[1
]}

Omodei, Nicola ^{[1
]}

Pinchera, Michele ^{[1
]}

Sgro, Carmelo ^{[1
]}

Spandre, Gloria ^{[1
]}

Matt, Giorgio ^{[1
]}

Perola, Giuseppe Cesare ^{[1
]}

Citterio, Oberto ^{[1
]}

Pareschi, Giovanni ^{[1
]}

Cotroneo, Vincenzo ^{[1
]}

Spiga, Daniele ^{[1
]}

Canestrari, Rodolfo ^{[1
]}

机构：

[1] Ist Astrofis Spaziale & Fis Cosm, I-00133 Rome, Italy

来源：

Space Telescopes and Instrumentation II: Ultraviolet to Gamma Ray, Pts 1 and 2 | 2006年 / 6266卷

关键词：

hard X-rays; telescopes; polarimetry;

D O I：

10.1117/12.671975

中图分类号：

V [航空、航天];

学科分类号：

08 ; 0825 ;

摘要：

Development of multi-layer optics makes feasible the use of X-ray. telescope at energy up to 60-80 keV: in this paper we discuss the extension of photoelectric polarimeter based on Micro Pattern Gas Chamber to high energy X-rays. We calculated the sensitivity with Neon and Argon based mixtures at high pressure with thick absorption gap: placing the MPGC at focus of a next generation multi-layer optics, galatic and extragalactic X-ray polarimetry can be done up till 30 keV.

引用

页码：X2662 / X2662

页数：12

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