The Optical Design for the Ultraviolet Explorer (UVEX) Mission: a next-generation wide-field UV telecope

被引:0
作者
Fucik, Jason [1 ]
机构
[1] CALTECH, Opt Observ, 1200 E Calif Blvd, Pasadena, CA 91125 USA
来源
SPACE TELESCOPES AND INSTRUMENTATION 2024: ULTRAVIOLET TO GAMMA RAY, PT 1 | 2024年 / 13093卷
关键词
Ultraviolet; Wide-Field; Space-Telescope; NUV/FUV Imager; Long-Slit Spectrometer;
D O I
10.1117/12.3020427
中图分类号
P1 [天文学];
学科分类号
0704 ;
摘要
The Ultraviolet Explore (UXEX) mission is a wide-field two band imager with a long multi-width slit spectrometer to study the dynamic ultraviolet universe. The UVEX mission will provide an all-sky survey in the ultraviolet to complement Rubin, Euclid, and Roman operating in the optical/infrared. The telescope will be capable of deep imaging and spectroscopic follow-up within hours of an event for study of targets of opportunity. The telescope optical design provides a continuous 5.0 degrees x3.5 degrees Field of View (FoV) that achieves an rms spot radius of <10 mu m. The optical design is a compact unobstructed freeform f/2.7 Three Mirror Anastigmat (TMA) with a 75 cm virtual entrance pupil. The all-reflective design is driven to support imaging into the far UV down to 115 nm. The telescope provides light to three instrument channels: a NUV imager (200 - 260 nm), a FUV imager (130 - 190 nm), and a Long-Slit Spectrometer (LSS) operating over the entire wavelength range (115 - 265 nm). The spectrometer is an all-reflective re-imager based on an Offner-Chrisp design where the secondary convex mirror is the dispersing element. The spectrometer has a 2 '' long-slit length with three discrete slit widths of 2 '', 4 '', and 8 '' wide. With a 2 '' slit width, the spectrometer has a spectral resolving power of 1400 - 3200 from 115 - 265 nm wavelength range.
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页数:10
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