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HgCdTe APD Arrays for Astronomy: Natural Guide Star Wavefront Sensing and Space Astronomy

arXiv: Instrumentation and Methods for Astrophysics(2018)

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Abstract
This dissertation describes work I have conducted over five academic years 2013/14 through 2017/18 as a NASA Space Technology Research Fellow at the University of Hawai'i Institute for Astronomy. The focus has been the characterization and improvement of the Selex Avalanche Photodiode HgCdTe InfraRed Array (SAPHIRA), a 320 x 256@24um pitch metal organic vapor phase epitaxy mercury cadmium telluride array that provides new capabilities and performance for near infrared (NIR) astronomy. This has involved more than a dozen arrays, working closely with the manufacturer so as to provide feedback for improvement of the next generation.
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要点】:本文主要研究了HgCdTe APD阵列在自然导星波前感应和空间天文学中的应用,并对Selex Avalanche Photodiode HgCdTe InfraRed Array(SAPHIRA)进行了特性化和改进,提高了其在近红外天文学中的性能。

方法】:作者通过特性化测试和与制造商的紧密合作,对SAPHIRA进行了性能评估和反馈改进。

实验】:实验使用了超过十几个SAPHIRA阵列,通过连续的测试和优化,取得了在近红外天文学领域的性能提升。