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The ~(55)Fe X-Ray Energy Response of Mercury Cadmium Telluride Near-Infrared Detector Arrays

机译:碲化汞镉近红外探测器阵列的〜(55)Fe X射线能量响应

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摘要

A technique involving ~(55)Fe X-rays provides a straightforward method to measure the response of a detector. The detector's response can lead directly to a calculation of the conversion gain (e~-ADU~(-1)), as well as aid detector design and performance studies. We calibrate the ~(55)Fe X-ray energy response and pair production energy of HgCdTe using 8 HST WFC3 1.7 pm flight grade detectors. The results show that each Kct X-ray generates 2273 ± 137 electrons, which corresponds to a pair-production energy of 2.61 ± 0.16 eV. The uncertainties are dominated by our knowledge of the conversion gain. In future studies, we plan to eliminate this uncertainty by directly mea_suring conversion gain at very low light levels.
机译:涉及〜(55)Fe X射线的技术提供了一种直接的方法来测量探测器的响应。检测器的响应可以直接导致转换增益的计算(e〜-ADU〜(-1)),以及辅助检测器的设计和性能研究。我们使用8个HST WFC3 1.7 pm飞行级检测器校准〜(55)Fe X射线能量响应和HgCdTe的成对生产能量。结果表明,每条Kct X射线产生2273±137个电子,这对应于2.61±0.16 eV的成对产生能量。不确定性由我们对转换增益的了解所决定。在未来的研究中,我们计划通过直接测量非常低的光照水平下的转换增益来消除这种不确定性。

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