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Performance of the GHRS Pt-Ne Hollow-cathode Lamps after their Return from Space and Comparison with Archival Data

机译:GHRS Pt-Ne空心阴极灯返回太空后的性能以及与档案数据的比较

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The Space Telescope European Co-ordinating Facility (ST-ECF) and National Institute of Standards and Technology (NIST) are collaborating to study hollow cathode calibration lamps as used onboard the Hubble Space Telescope (HST). As part of the STIS Calibration Enhancement (STIS-CE) Project we are trying to improve our understanding of the performance of hollow cathode lamps and the physical processes involved in their long term operation. The original flight lamps from the Faint Object Spectrograph (FOS) and the Goddard High Resolution Spectrograph (GHRS) are the only lamps that have ever been returned to Earth after extended operation in space. We have taken spectra of all four lamps using NIST's 10.7-m normal-incidence Spectrograph and Fourier transform spectrometer (FTS) optimized for use in the ultraviolet (UV). These spectra, together with spectra archived from six years of on-orbit operations and pre-launch spectra, provide a unique data set - covering a period of about 20 years - for studying aging effects in these lamps. Our findings represent important lessons for the choice and design of calibration sources and their operation in future UV and optical spectrographs in space. Our results will be directly used for planning science operations of the Cosmic Origins Spectrograph (COS) which is going to be installed on the HST during the next servicing mission.
机译:欧洲太空望远镜协调中心(ST-ECF)和美国国家标准与技术研究院(NIST)正在合作研究哈勃太空望远镜(HST)上使用的空心阴极校准灯。作为STIS校准增强(STIS-CE)项目的一部分,我们正在努力增进对空心阴极灯性能及其长期运行所涉及的物理过程的了解。来自微弱物体光谱仪(FOS)和戈达德高分辨率光谱仪(GHRS)的原始飞行灯是在太空中扩展运行后唯一返回地球的灯。我们已使用NIST的10.7米法向入射光谱仪和傅里叶变换光谱仪(FTS)采集了所有四盏灯的光谱,这些光谱仪已针对紫外线(UV)进行了优化。这些光谱,连同在轨运行六年和发射前光谱中存档的光谱,提供了一个独特的数据集(涵盖大约20年的时间),用于研究这些灯的老化效应。我们的发现代表了校准源的选择和设计及其在未来空间紫外和光学光谱仪中的操作中的重要教训。我们的结果将直接用于计划宇宙起源光谱仪(COS)的科学操作,该光谱仪将在下一次维修任务中安装在HST上。

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