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Design of a 1k pixel Ge:Sb focal-plane array for far-IR astronomy

机译:1K像素GE:FAR-IR天文学的SB焦平面阵列的设计

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Development of large format, far infrared focal-plane arrays has been identified as a pressing need for futureastronomical instruments. In particular, array sizes as large as 128x128 with sensitivities equal to or better than 10-18W/√Hz are the goals to be achieved within the next fifteen years. As part of our continuing effort to further thistechnology, we are developing a 32x32 Ge:Sb photoconductor FPA with a CTIA cryogenic readout multiplexer. Anew, layered-hybrid architecture is employed to block the readout glow, improve heat dissipation and temperatureuniformity across the array, and alleviate the potential problems associated with the large CTE mismatch between theGe detector and the Si readout. This is the first 1k-pixel photoconductor FPA of its kind and is meant to be a pathfinderfor future large format FPAs. Based on the test results of a prototype 2x16 Ge:Sb array of similar design, we expect thesensitivity of this FPA to be as low as 10~(-18)W/√Hz. This paper presents the design, characteristics, and expectedperformance of this array.
机译:大幅度的发展,远红外焦平面阵列已被确定为未来的无效仪器的压力需求。特别是,阵列大小为128x128,敏感度等于或优于10-18W /√Hz是在未来十五年内实现的目标。作为我们持续努力进一步铸造的一部分,我们正在开发32x32 GE:SB光电导体FPA,具有CTIA低温读数多路复用器。重新使用分层混合架构来阻止读出发光,改善阵列的散热和温度均匀,并减轻与探测器之间的大CTE错配相关的潜在问题和SI读出。这是其种类的第一个1k像素光电导体FPA,并旨在成为未来大型FPA的探测器。基于原型2x16 GE:SB阵列类似设计的测试结果,我们预计该FPA的比例低至10〜(-18)W /√Hz。本文介绍了该阵列的设计,特点和预期格式。

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