15 July 2008 The long slit spectrograph onboard the World Space Observatory-Ultraviolet
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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 on-board 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. We will discuss the detailed design of the spectrograph and its expected performance in this paper.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Maohai Huang, Maohai Huang, Martin A. Barstow, Martin A. Barstow, Zhiyuan Chen, Zhiyuan Chen, Jon S. Lapington, Jon S. Lapington, Mikhail E. Sachkov, Mikhail E. Sachkov, Boris Shustov, Boris Shustov, Qian Song, Qian Song, Sen Wang, Sen Wang, } "The long slit spectrograph onboard the World Space Observatory-Ultraviolet", Proc. SPIE 7011, Space Telescopes and Instrumentation 2008: Ultraviolet to Gamma Ray, 70111Y (15 July 2008); doi: 10.1117/12.788851; https://doi.org/10.1117/12.788851


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