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The Wide Field Survey Telescope (WFST) is a 2.5m diameter telescope proposed by the University of Science and Technology of China and the Purple Mountain Observatory. The telescope is located at the summit of the Saishiteng Mountain near Lenghu City. The WFST equipped with a mosaic camera on the primary focus plane that includes 9 scientific imaging CCDs, 8 wave-front CCDs, and 4 guiding CCDs. The CCDs are placed in vacuum Dewar, and electronic signals are transmitted through the PCB boards and the vacuum Dewar connectors to the readout electronics outside Dewar. We provided a low-noise readout solution and a high-speed reliable data upload solution for the mosaic CCD camera, and evaluate and tests the performance.
(2024) Published by SPIE. Downloading of the abstract is permitted for personal use only.
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Qi Feng, Hui Wang, Hong-fei Zhang, Jian Wang, Zhi-yue Wang, Zhe Geng, Jun Zhang, Feng Zeng, Ying-fan Guo, "Design of the electronics for the WFST camera," Proc. SPIE 13096, Ground-based and Airborne Instrumentation for Astronomy X, 130963V (18 July 2024); https://doi.org/10.1117/12.3018237