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Optical design of CAOS: a high-resolution spectropolarimeter for the Catania Astrophysical Observatory 0.91-m telescope

机译:CAOS光学设计:Catania Astrophysical Meangetatory 0.91-M望远镜的高分辨率分布

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CAOS (Catania Astrophysical Observatory Spectrograph) is a high-resolution (R approx=60,000), fiber fed, bench-mounted, prism cross-dispersed, white-pupil R-4 echelle spectrograph with polarimetric capabilities, for the 0.91m telescope on Mt. Etna. Wavelengths from 390 to 710 nm are covered in one-shot with a 2K * 2K 13.5 micron CCD. Inherent high efficiency of the spectrograph and optimum matching between fibers and spectrograph will allow high throughput for the overall system. This instrument will replace the existing spectrograph, with a net gain in spectral resolution (about a factor 2) and in efficiency (about a factor 10), extending current studies undertaken by Catania Astrophysical Observatory in stellar physics.
机译:CAOS(卡塔尼亚天体物理观测器光谱仪)是一种高分辨率(R大约= 60,000),纤维喂食,台式安装,棱镜交叉分散,具有偏振能力的白色瞳孔R-4梯定光谱仪,用于MT上的0.91米望远镜。etna。从390到710 nm的波长覆盖,用2k * 2k 13.5微米ccd覆盖一次。纤维和光谱仪之间的光谱仪和最佳匹配的固有高效率将使整个系统的吞吐量高。该仪器将取代现有的光谱仪,具有谱分辨率的净增益(约束2)和效率(约10系数10),延长了恒星物理学中的卡塔尼亚天体物理天文台进行的当前研究。

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