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arXiv physics/0604114physics.ins-detastro-ph
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利用自触发CMOS模拟芯片直接读取电荷倍增器,像素为105 k,间距为50微米

Direct reading of charge multipliers with a self-triggering CMOS analog chip with 105k pixels at 50 micron pitch

R. Bellazzini, G. Spandre, M. Minuti, L. Baldini, A. Brez, F. Cavalca, L. Latronico, N. Omodei, M. M. Massai, C. Sgro, E. Costa, P. Soffitta F. Krummenacher, R. DeOliveira

摘要:

我们报告了一个大的有效面积(15 × 15 mm ~ 2),高通道密度(470像素/mm ~ 2),自触发CMOS模拟芯片,我们已经开发的像素化的电荷收集电极的微图案气体检测器。该器件在尺寸和性能方面都向前迈出了一大步,是复杂性不断增加的三代定制ASIC的最后一个版本。CMOS像素阵列具有以50微米间距在105600个六边形像素的矩阵中图案化的顶部金属层。每个像素都直接连接到下面的完整电子链,该电子链已在0.18微米VLSI技术的剩余五个金属层和两个多晶硅层中实现。该芯片具有可定制的自触发能力,并包括用于事件坐标自动定位的信号预处理功能。以这种方式,可以通过将信号输出仅限于属于感兴趣区域的那些像素来显著减少读出时间和数据量。非常小的像素面积和深亚微米CMOS技术的使用使噪声降低到50电子ENC。从这个设备的深度测试时,耦合到一个细间距(50微米的三角形图案)气体电子倍增器的结果。读出和气体放大间距的匹配允许获得最佳结果。讨论了该探测器在天文X射线偏振测量中的应用。实验探测器响应偏振和非偏振X射线辐射时,与两种气体混合物和两种不同的光子能量的工作示出。从一个完整的蒙特卡罗模拟几个银河系和河外atronomic源的结果也有报道。

英文摘要:

We report on a large active area (15x15mm2), high channel density (470 pixels/mm2), self-triggering CMOS analog chip that we have developed as pixelized charge collecting electrode of a Micropattern Gas Detector. This device, which represents a big step forward both in terms of size and performance, is the last version of three generations of custom ASICs of increasing complexity. The CMOS pixel array has the top metal layer patterned in a matrix of 105600 hexagonal pixels at 50 micron pitch. Each pixel is directly connected to the underneath full electronics chain which has been realized in the remaining five metal and two poly-silicon layers of a 0.18 micron VLSI technology. The chip has customizable self-triggering capability and includes a signal pre-processing function for the automatic localization of the event coordinates. In this way it is possible to reduce significantly the readout time and the data volume by limiting the signal output only to those pixels belonging to the region of interest. The very small pixel area and the use of a deep sub-micron CMOS technology has brought the noise down to 50 electrons ENC. Results from in depth tests of this device when coupled to a fine pitch (50 micron on a triangular pattern) Gas Electron Multiplier are presented. The matching of readout and gas amplification pitch allows to get optimal results. The application of this detector for Astronomical X-Ray Polarimetry is discussed. The experimental detector response to polarized and unpolarized X-ray radiation when working with two gas mixtures and two different photon energies is shown. Results from a full MonteCarlo simulation for several galactic and extragalactic atronomical sources are also reported.

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