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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 9.

Distribution of GD-corrected positional residuals (ΔXNGC 2298, ΔYNGC 2298) as a function of g-band magnitude. The grayscale shading represents the local density of points, with darker shades indicating higher densities. The red solid lines with error bars show the mean positional offsets and the corresponding 1σ dispersions, computed within 0.5 mag bins.

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