一种实用的天文非扫描FTS

H. Butcher, N. Douglas, S. Frandsen, F. Maaswinkel
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引用次数: 3

摘要

传统的天文恒星光谱仪基于经典的狭缝/光栅设计,这种设计具有易于集成多通道阵列探测器的相当大的优势。利用现有的光学、衍射光栅和阵列探测器技术,为了保持恒定的光学效率,人们发现这种类型的高分辨率仪器的物理尺寸与望远镜孔径大致成线性关系。对于中等光谱分辨率和现有的望远镜来说,能够同时记录相当长度的光谱被普遍认为是一种优势,超过了仪器的不美观和适度昂贵的性质。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
A Practical Non-Scanning FTS for Astronomy
Astronomical stellar spectrometers have traditionally been based on classical slit/grating designs, which have the considerable advantage of easy incorporation of multi-channel array detectors. With current optical, diffraction grating, and array detector technologies, and for constant optical efficiency, high resolution instruments of this type are found to scale in physical size roughly linearly with telescope aperture. For moderate spectral resolutions and existing telescopes, the ability to record simultaneously a substantial length of spectrum has generally been thought to be an advantage outweighing the inelegant and moderately costly nature of the instruments.
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