CUBES phase a design overview
نویسندگان
چکیده
We present the baseline conceptual design of Cassegrain U-Band Efficient Spectrograph (CUBES) for Very Large Telescope. CUBES will provide unprecedented sensitivity spectroscopy on a 8 - 10 m class telescope in ground ultraviolet (UV), spanning bandwidth > 100 nm that starts at 300 nm, shortest wavelength accessible from ground. The has been optimized end-to-end efficiency and provides spectral resolving power R 20000, unlock broad range new topics across solar system, Galactic extraglactic astronomy. also features second, lower-resolution (R \sim 7000) mode option fiberlink to UVES instrument simultaneous observations longer wavelengths. Here we optical, mechanical software various subsystems after Phase A study project. discuss expected performances layout choices highlight some performance trade-offs considered best meet top-level requirements. introduce model-based system engineering approach used organize manage project activities interfaces, context it is increasingly necessary integrate such tools development complex astronomical projects.
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ژورنال
عنوان ژورنال: Experimental Astronomy
سال: 2022
ISSN: ['0922-6435', '1572-9508']
DOI: https://doi.org/10.1007/s10686-022-09837-w