Mock Observations for the CSST Mission: Main Surveys-the Slitless Spectroscopy Simulation
Xin Zhang, Yue-dong Fang, Cheng-liang Wei, Guo-liang Li, Feng-shan Liu, Hang-xin Ji, Hao Tian, Nan Li, Xian-min Meng, Jian-jun Chen, Xia Wang, Rui Wang, Chao Liu, Zhong-wen Hu, Ran Li, Peng Wei, Jing Tang

TL;DR
This paper presents a simulation framework for the CSST's slitless spectroscopic system, analyzing its properties and detection performance to aid in data processing development before real observations begin.
Contribution
It introduces a novel simulation framework for the CSST slitless spectroscopic system, enabling performance assessment and aiding in pipeline development.
Findings
Nearly all 1st order spectra have corresponding 0th order images.
GI spectral band shows higher detection efficiency than GV and GU bands.
Simulation results support the primary use of the GI band for stellar and galactic observations.
Abstract
The China Space Station Telescope (CSST), slated to become China's largest space-based optical telescope in the coming decade, is designed to conduct wide-field sky surveys with high spatial resolution. Among its key observational modes, slitless spectral observation allows simultaneous imaging and spectral data acquisition over a wide field of view, offering significant advantages for astrophysical studies. Currently, the CSST is in the development phase and lacks real observational data. As a result, the development of its data processing pipeline and scientific pre-research must rely on the mock data generated through simulations. This work focuses on developing a simulation framework for the CSST slitless spectral imaging system, analyzing its spectral dispersing properties and structural design. Additionally, the detection performance of the slitless spectral system is assessed for…
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Taxonomy
TopicsOptical Polarization and Ellipsometry · Adaptive optics and wavefront sensing · Astronomy and Astrophysical Research
