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A Robust Geometric Distortion Solution for the Main Survey Camera of CSST

  • Authors: Yibo Yan, 一波 闫, You Wu, 优 吴, Jundan Nie, 俊丹 聂, Tianmeng Zhang, 天萌 张, Chao Liu, 超 刘, Zhang Ban, 章 班, Zihuang Cao, 子皇 曹, Wei Du, 薇 杜, Yuedong Fang, 越东 方, Yi Hu, 义 胡, Guoliang Li, 国亮 李, Xiaobo Li, 晓波 李, Chenxiaoji Ling, 晨晓骥 凌, Jiaqi Lin, 家琪 林, Dezi Liu, 德子 刘, Yu Luo, 煜 罗, Bin Ma, 斌 马, Xianmin Meng, 宪民 孟, Juanjuan Ren, 娟娟 任, Li Shao, 立 邵, Hao Tian, 浩 田, Chengliang Wei, 成亮 韦, Peng Wei, 鹏 魏, Shoulin Wei, 守林 卫, Yun-Ao Xiao, 云奥 肖, Zhou Xie, 洲 谢, Su Yao, 苏 姚, Yan Yu, 彦 吁, Shengwen Zhang, 圣文 张, Xin Zhang, 鑫 张, Bowei Zhao, 博伟 赵, Zhimin Zhou, 志民 周, Hu Zou, 虎 邹

Yibo Yan et al 2026 The Astronomical Journal 171 .

  • Provider: AAS Journals

Caption: Figure 1.

The distortion map of the MSC’s 18 photometric detectors, derived from a subset of the CSST 25 deg2 simulation program. Detector name and number are shown in blue on the central region of each detector box. The size of the distortion vector marked in red is magnified by a factor of 10.

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