Superconducting cameras for optical astronomy

D. Martin, P. Verhoeve, J. de Bruijne, A. Reynolds, A. van Dordrecht, J. Verveer, J. Page, N. Rando, A. Peacock
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Abstract

Superconducting Tunnel Junctions (STJs) have been extensively investigated as photon detectors covering the range from near-infrared to X-ray energies. A 6x6 array of Tantalum junctions has already been used in an optical spectro-photometer. With this camera, the European Space Agency has performed multiple astronomical observations of optical sources using the William Herschel 4.2m telescope at La Palma. Following the success of this programme, we are now developing a second generation camera. The goals of this programme are to increase the field of view of the instrument from 4x4 to 10.5x9, to optimize IR rejection filters, possibly extending the 'red' response to ∼lum and to increase the electronics readout speed. For these purposes, we are developing a new Superconducting Tunnel Junction Array consisting of 10x12 Tantalum/Aluminium devices as well as an improved readout system. In this paper, we review the instrument's architecture and describe the performance of the new detector.
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光学天文学用超导照相机
超导隧道结(stj)作为覆盖近红外到x射线能量范围的光子探测器已被广泛研究。一个6x6的钽结阵列已经在分光光度计中使用。有了这台相机,欧洲空间局利用拉帕尔马的威廉·赫歇尔4.2米望远镜对光源进行了多次天文观测。随着这个项目的成功,我们现在正在开发第二代相机。该计划的目标是将仪器的视野从4x4增加到10.5x9,优化红外抑制滤波器,可能将“红色”响应扩展到~ lum,并提高电子读出速度。为此,我们正在开发一种新的超导隧道结阵列,由10x12钽/铝器件以及改进的读出系统组成。在本文中,我们回顾了仪器的结构,并描述了新的探测器的性能。
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Superconducting cameras for optical astronomy A 4.2 K readout channel in a standard 0.7 /spl mu/m CMOS process for a photoconductor array camera Interaction of super high frequency radiation with superconducting Bi(Pb)-Sr-Ca-Cu-O thin-film structures Temperature dependence of generation-recombination noise in p-n junctions Degradation of hard MOS devices at low temperature
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