Advanced image slicers for integral field spectroscopy with UKIRT and GEMINI

被引:50
作者
Content, R [1 ]
机构
[1] Univ Durham, Dept Phys, Astron Instrumentat Grp, Durham DH1 3LE, England
来源
INFRARED ASTRONOMICAL INSTRUMENTATION, PTS 1-2 | 1998年 / 3354卷
关键词
integral field spectroscopy; large telescope instrumentation;
D O I
10.1117/12.317262
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The new design of image slicer developed at Durham University for two-dimensional area spectroscopy is described. The unit acts as a coupler between the telescope and a spectrograph to reformat a square or rectangular field into a long slit. Its advantages over previous designs of image slicers and other methods using fibres, lenses or narrow-band filtering are discussed mainly: Large field, high spatial. resolution, large number of spectral resolution elements, high transmission, and the small size of the instrument. The system is also easy to cool and is then well suited for infrared spectroscopy. The proposed design is a new type of image slicer in which the original two-dimensional image is sliced into narrow sub-images that are re-imaged side by side to form a long one-dimensional image at the spectrograph input. The flexibility of the concept at the base of this new design is highlighted through the description of 5 different slicer designs. Three of these are for future instruments now at the design phase: The CGS4 slicer (UKIRT), the UIST slicer (UKIRT) and the GNIRS slicer (GEMINI); the two others are studies for possible future slicers on GMOS (GEMINI) and NGST. These designs show how easily our slicer can be added to an existing instrument, how it can be incorporated to the slit wheel of future instruments, and how multi-slit reformatting permits a much larger field of view.
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页码:187 / 200
页数:14
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