Mock Observations for the CSST Mission: Multi-Channel Imager--Instrument Simulation

Fuente: arXiv
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Auteurs principaux: Yan, Zhao-Jun, Shan, Huan-Yuan, Zheng, Zhen-Ya, Peng, Xi-Yan, Qi, Zhao-Xiang, Xu, Chun, Lin, Lin, Wen, Xin-Rong, Jiang, Chun-Yan, Zheng, Li-Xin, Zhong, Jing, Yuan, Fang-Ting, Chen, Zhen-Lei, Chen, Wei, Wu, Mao-Chun, Fu, Zhen-Sen, Li, Ke-Xin, Nie, Lin, Liu, Chao, Li, Nan, Wang, Qiao, Cao, Zi-Huang, Feng, Shuai, Li, Guo-Liang, Wang, Lei, Wei, Cheng-Liang, Li, Xiao-Bo, Ban, Zhang, Yang, Xun, Jiang, Yu-Xi, Liu, De-Zi, Chen, Yong-He, Liu, Xiao-Hua, Xu, Fang, Cheng, Xue, Su, Yue, Duan, Tong-Fang, Qi, Chao, Li, Na, Zheng, Geng, Ma, Chong, Tang, Jing, Li, Ran
Format: Preprint
Publié: 2025
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_version_ 1866917084049440768
author Yan, Zhao-Jun
Shan, Huan-Yuan
Zheng, Zhen-Ya
Peng, Xi-Yan
Qi, Zhao-Xiang
Xu, Chun
Lin, Lin
Wen, Xin-Rong
Jiang, Chun-Yan
Zheng, Li-Xin
Zhong, Jing
Yuan, Fang-Ting
Chen, Zhen-Lei
Chen, Wei
Wu, Mao-Chun
Fu, Zhen-Sen
Li, Ke-Xin
Nie, Lin
Liu, Chao
Li, Nan
Wang, Qiao
Cao, Zi-Huang
Feng, Shuai
Li, Guo-Liang
Wang, Lei
Wei, Cheng-Liang
Li, Xiao-Bo
Ban, Zhang
Yang, Xun
Jiang, Yu-Xi
Liu, De-Zi
Chen, Yong-He
Liu, Xiao-Hua
Xu, Fang
Cheng, Xue
Su, Yue
Duan, Tong-Fang
Qi, Chao
Li, Na
Zheng, Geng
Ma, Chong
Tang, Jing
Li, Ran
author_facet Yan, Zhao-Jun
Shan, Huan-Yuan
Zheng, Zhen-Ya
Peng, Xi-Yan
Qi, Zhao-Xiang
Xu, Chun
Lin, Lin
Wen, Xin-Rong
Jiang, Chun-Yan
Zheng, Li-Xin
Zhong, Jing
Yuan, Fang-Ting
Chen, Zhen-Lei
Chen, Wei
Wu, Mao-Chun
Fu, Zhen-Sen
Li, Ke-Xin
Nie, Lin
Liu, Chao
Li, Nan
Wang, Qiao
Cao, Zi-Huang
Feng, Shuai
Li, Guo-Liang
Wang, Lei
Wei, Cheng-Liang
Li, Xiao-Bo
Ban, Zhang
Yang, Xun
Jiang, Yu-Xi
Liu, De-Zi
Chen, Yong-He
Liu, Xiao-Hua
Xu, Fang
Cheng, Xue
Su, Yue
Duan, Tong-Fang
Qi, Chao
Li, Na
Zheng, Geng
Ma, Chong
Tang, Jing
Li, Ran
contents The Chinese Space Station Survey Telescope (CSST), a two-meter aperture astronomical space telescope under China's manned space program, is equipped with multiple back-end scientific instruments. As an astronomical precision measurement module of the CSST, the Multi-Channel Imager (MCI) can cover a wide wavelength range from ultraviolet to near-infrared with three-color simultaneous high-precision photometry and imaging, which meets the scientific requirements for various fields. The diverse scientific objectives of MCI require not only a robust airborne platform, advanced optical systems, and observing facilities but also comprehensive software support for scientific operations and research. To this end, it is essential to develop realistic observational simulation software to thoroughly evaluate the MCI data stream and provide calibration tools for future scientific investigations. The MCI instrument simulation software will serve as a foundation for the development of the MCI data processing pipeline and will facilitate improvements in both hardware and software, as well as in the observational operation strategy, in alignment with the mission's scientific goals. In conclusion, we present a comprehensive overview of the MCI instrument simulation and some corresponding performances of the MCI data processing pipeline.
format Preprint
id arxiv_https___arxiv_org_abs_2511_12481
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Mock Observations for the CSST Mission: Multi-Channel Imager--Instrument Simulation
Yan, Zhao-Jun
Shan, Huan-Yuan
Zheng, Zhen-Ya
Peng, Xi-Yan
Qi, Zhao-Xiang
Xu, Chun
Lin, Lin
Wen, Xin-Rong
Jiang, Chun-Yan
Zheng, Li-Xin
Zhong, Jing
Yuan, Fang-Ting
Chen, Zhen-Lei
Chen, Wei
Wu, Mao-Chun
Fu, Zhen-Sen
Li, Ke-Xin
Nie, Lin
Liu, Chao
Li, Nan
Wang, Qiao
Cao, Zi-Huang
Feng, Shuai
Li, Guo-Liang
Wang, Lei
Wei, Cheng-Liang
Li, Xiao-Bo
Ban, Zhang
Yang, Xun
Jiang, Yu-Xi
Liu, De-Zi
Chen, Yong-He
Liu, Xiao-Hua
Xu, Fang
Cheng, Xue
Su, Yue
Duan, Tong-Fang
Qi, Chao
Li, Na
Zheng, Geng
Ma, Chong
Tang, Jing
Li, Ran
Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
The Chinese Space Station Survey Telescope (CSST), a two-meter aperture astronomical space telescope under China's manned space program, is equipped with multiple back-end scientific instruments. As an astronomical precision measurement module of the CSST, the Multi-Channel Imager (MCI) can cover a wide wavelength range from ultraviolet to near-infrared with three-color simultaneous high-precision photometry and imaging, which meets the scientific requirements for various fields. The diverse scientific objectives of MCI require not only a robust airborne platform, advanced optical systems, and observing facilities but also comprehensive software support for scientific operations and research. To this end, it is essential to develop realistic observational simulation software to thoroughly evaluate the MCI data stream and provide calibration tools for future scientific investigations. The MCI instrument simulation software will serve as a foundation for the development of the MCI data processing pipeline and will facilitate improvements in both hardware and software, as well as in the observational operation strategy, in alignment with the mission's scientific goals. In conclusion, we present a comprehensive overview of the MCI instrument simulation and some corresponding performances of the MCI data processing pipeline.
title Mock Observations for the CSST Mission: Multi-Channel Imager--Instrument Simulation
topic Instrumentation and Methods for Astrophysics
Astrophysics of Galaxies
url https://arxiv.org/abs/2511.12481