Gas pixel detectors for X-ray polarimetry applications

被引:45
|
作者
Bellazzini, R.
Angelini, F.
Baldini, L.
Bitti, F.
Brez, A.
Cavalca, F.
Del Prete, M.
Kuss, M.
Latronico, L.
Omodei, N.
Pinchera, M.
Massai, M. M.
Minuti, M.
Razzano, M.
Sgro, C.
Spandre, G.
Tenze, A.
Costa, E.
Soffitta, P.
机构
[1] Ist Nazl Fis Nucl, Sez Pisa, I-56127 Pisa, Italy
[2] Univ Pisa, I-56127 Pisa, Italy
[3] Ist Nazl Fis Nucl, I-56127 Pisa, Italy
[4] INAF, Ist Astrofis Spatiale & Fis Cosm, I-00133 Rome, Italy
来源
NUCLEAR INSTRUMENTS & METHODS IN PHYSICS RESEARCH SECTION A-ACCELERATORS SPECTROMETERS DETECTORS AND ASSOCIATED EQUIPMENT | 2006年 / 560卷 / 02期
关键词
X-ray polarimetry; micro pattern gas detectors; pixel read-out;
D O I
10.1016/j.nima.2006.01.046
中图分类号
TH7 [仪器、仪表];
学科分类号
0804 ; 080401 ; 081102 ;
摘要
We discuss a new class of micro pattern gas detectors, the gas pixel detector (GPD), in which a complete integration between the gas amplification structure and the read-out electronics has been reached. An application-specific integrated circuit (ASIC) built in deep submicron technology has been developed to realize a monolithic device that is, at the same time, the pixelized charge collecting electrode and the amplifying, shaping and charge measuring front-end electronics. The CMOS chip has the top metal layer patterned in a matrix of 80 mu m pitch hexagonal pixels, each of them directly connected to the underneath electronics chain which has been realized in the remaining five layers of the 0.35 mu m VLSI technology. Results from tests of a first prototype of such detector with 2 k pixels and a full scale version with 22 k pixels are presented. The application of this device for Astronomical X-ray Polarimetry is discussed. The experimental detector response to polarized and unpolarized X-ray radiation is shown. Results from a full MonteCarlo simulation for two astronomical sources, the Crab Nebula and the Hercules X1, are also reported. (c) 2006 Elsevier B.V. All rights reserved.
引用
收藏
页码:425 / 434
页数:10
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