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The long slit spectrograph onboard the World Space Observatory-Ultraviolet

机译:紫外世界空间天文台上的长缝光谱仪

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The World Space Observatory - Ultraviolet (WSO-UV) is a space astronomy project led by Russia, with contributions from China, Germany, Italy, Spain, United Kingdom and a number of other countries in the world. WSO-UV consists of a 1.7-meter diameter telescope and three focal plane science instruments. The Long Slit Spectrograph instrument onboard WSO-UV will produce moderate spectral resolution (R=1000-2500) spectra in the 102nm ~ 320nm wavelength range along a slit of 75 arcsec in length and 1 arcsec in width. The spatial resolution of the instrument will be ~1 arcsec. A two-channel scheme is proposed to optimize performance, with each of these using a Rowland Circle optical design with MicroChannel Plate detectors in the focal plane. Based on preliminary results of feasibility study we will discuss the detailed design of the spectrograph and its expected performance in this paper.
机译:世界紫外线观测站(WSO-UV)是俄罗斯领导的一个太空天文学项目,来自中国,德国,意大利,西班牙,英国和世界其他许多国家的贡献。 WSO-UV包括一个1.7米直径的望远镜和三个焦平面科学仪器。 WSO-UV上的Long Slit Spectrograph仪器将沿着长度为75 arcsec和宽度为1 arcsec的狭缝在102nm〜320nm波长范围内产生中等光谱分辨率(R = 1000-2500)光谱。仪器的空间分辨率为〜1 arcsec。提出了一种两通道方案来优化性能,其中每一种方案都使用Rowland Circle光学设计,其焦平面中带有MicroChannel Plate检测器。基于可行性研究的初步结果,我们将在本文中讨论光谱仪的详细设计及其预期性能。

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