Mock Observations for the CSST Mission: CPI-C -- Instrument Simulation

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Hauptverfasser: Zhao, Gang, Zhu, Yiming, Dou, Jiangpei, Chen, Yili, Lv, Zhonghua, Niu, Bingli, Yan, Zhaojun, Ma, Bo, Li, Ran
Format: Preprint
Veröffentlicht: 2025
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author Zhao, Gang
Zhu, Yiming
Dou, Jiangpei
Chen, Yili
Lv, Zhonghua
Niu, Bingli
Yan, Zhaojun
Ma, Bo
Li, Ran
author_facet Zhao, Gang
Zhu, Yiming
Dou, Jiangpei
Chen, Yili
Lv, Zhonghua
Niu, Bingli
Yan, Zhaojun
Ma, Bo
Li, Ran
contents To support the development of the data processing pipeline and the scientific performance assessment for the Cool Planet Imaging Coronagraph (CPI-C) on the Chinese Space Station Survey Telescope (CSST), we have developed the end-to-end instrument simulation program, CPISM. This paper details the core modules of CPISM that simulate the CPI-C instrument, focusing on the simulation of the high-contrast imaging optical system and the visible-band science camera. We modeled key optical components, such as the transmission apodizing filter, the wavefront corrector, and the focal plane mask using the HCIPy package. A $10^{-8}$ contrast dark hole region, consistent with design specifications, was simulated using the Electric Field Conjugation (EFC) optimization method, and broadband observation effects were considered. For the science camera, which is an electron multiplying charge-coupled device (EMCCD), we established a detailed model encompassing photon collection, charge transfer, electron multiplication (EM), and readout processes, based on test data. This model simulates complex instrumental features including dark current, charge transfer efficiency, clock-induced charge, multiplication noise factor, and various readout effects like striping and drift. We also proposed and validated an improved statistical model for the EM process to enhance simulation efficiency. CPISM can generate simulated images containing rich instrumental details, closely similar to the expected real observational data, thus laying the foundation for the development and verification of CPI-C data processing algorithms and preparations for future scientific research.
format Preprint
id arxiv_https___arxiv_org_abs_2511_08886
institution arXiv
publishDate 2025
record_format arxiv
spellingShingle Mock Observations for the CSST Mission: CPI-C -- Instrument Simulation
Zhao, Gang
Zhu, Yiming
Dou, Jiangpei
Chen, Yili
Lv, Zhonghua
Niu, Bingli
Yan, Zhaojun
Ma, Bo
Li, Ran
Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
To support the development of the data processing pipeline and the scientific performance assessment for the Cool Planet Imaging Coronagraph (CPI-C) on the Chinese Space Station Survey Telescope (CSST), we have developed the end-to-end instrument simulation program, CPISM. This paper details the core modules of CPISM that simulate the CPI-C instrument, focusing on the simulation of the high-contrast imaging optical system and the visible-band science camera. We modeled key optical components, such as the transmission apodizing filter, the wavefront corrector, and the focal plane mask using the HCIPy package. A $10^{-8}$ contrast dark hole region, consistent with design specifications, was simulated using the Electric Field Conjugation (EFC) optimization method, and broadband observation effects were considered. For the science camera, which is an electron multiplying charge-coupled device (EMCCD), we established a detailed model encompassing photon collection, charge transfer, electron multiplication (EM), and readout processes, based on test data. This model simulates complex instrumental features including dark current, charge transfer efficiency, clock-induced charge, multiplication noise factor, and various readout effects like striping and drift. We also proposed and validated an improved statistical model for the EM process to enhance simulation efficiency. CPISM can generate simulated images containing rich instrumental details, closely similar to the expected real observational data, thus laying the foundation for the development and verification of CPI-C data processing algorithms and preparations for future scientific research.
title Mock Observations for the CSST Mission: CPI-C -- Instrument Simulation
topic Instrumentation and Methods for Astrophysics
Earth and Planetary Astrophysics
url https://arxiv.org/abs/2511.08886