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Tunable laser techniques for improving the precision of observational astronomy

机译:可调谐激光技术,用于提高观察天文学的精度

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Improving the precision of observational astronomy requires not only new telescopes and instrumentation, butalso advances in observing protocols, calibrations and data analysis. The Laser Applications Group at the NationalInstitute of Standards and Technology in Gaithersburg, Maryland has been applying advances in detectormetrology and tunable laser calibrations to problems in astronomy since 2007. Using similar measurement techniques,we have addressed a number of seemingly disparate issues: precision flux calibration for broad-bandimaging, precision wavelength calibration for high-resolution spectroscopy, and precision PSF mapping for fiberspectrographs of any resolution. In each case, we rely on robust, commercially-available laboratory technologythat is readily adapted to use at an observatory. In this paper, we give an overview of these techniques.© (2012) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
机译:提高观察天文学的精度不仅需要新的望远镜和仪器,丁塔索在观察方案,校准和数据分析方面的进步。 Maryland的标准和技术国家标准与技术研究所的激光应用组一直在自2007年以来的天文学中探测探测器学和可调激光校准的进步。使用类似的测量技术,我们已经解决了一些看似不同的问题:精确的助焊剂校准用于宽带,高分辨率光谱的精密波长校准,以及任何分辨率的纤维谱的精密PSF映射。在每种情况下,我们依赖于稳健的,商业上的实验室技术,容易适应在天文台上使用。在本文中,我们概述了这些技术。©(2012)光学仪表工程师(SPIE)的版权协会。仅供个人使用的摘要下载。

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