CPI-C: Cool Planet Imaging Coronagraph on Chinese Space Station Survey Telescope
Jiangpei Dou, Xi Zhang, Gang Zhao, Mingming Xu, Zhen Wu, Gang Wang, Baoning Yuan, Lingyi Kong, Yiming Zhu, Bingli Niu, Zhonghua Lv, Yongjun Qi, Shu Jiang, Bo Chen, Wei Guo, Di Wang, Yinglu Lin, Liping Zheng, Jing Guo, Ruokun Li, Liyan Xu, Huihai Wu, Cheng Wen, Shuwei Miao

TL;DR
CPI-C on the Chinese Space Station Survey Telescope aims to directly image and analyze cool exoplanets around nearby stars using high-contrast imaging techniques in visible light.
Contribution
First space-based instrument capable of directly imaging reflection light from cool exoplanets in visible wavelengths, enabling detailed physical characterization.
Findings
Achieves contrast better than 10^-8 at 3-4λ/D IWA
Employs step-transmission apodization and phase correction techniques
Enables systematic spectroscopic analysis of exoplanets
Abstract
Cool Planet Imaging Coronagraph (CPI-C) on Chinese Space Station Survey Telescope (CSST) is proposed to direct image the cool planets around nearby solar-type stars (within 40 pc). The core scientific objective of CPI-C is to conduct high-contrast directly imaging surveys of exoplanets ranging in size from Neptune-like to Jupiter-like, located at separations of 0.5 to 5 AU from their host stars, and to perform systematic spectroscopic analysis of the detected planets through high-precision multi-band photometry. CPI-C employs a step-transmission apodization technique to suppress the diffraction noises from the telescope pupil and a precise phase correction technique to eliminate the speckle noises due to imperfections of the optical surfaces. The contrast requirement is better than at an inner working angle (IWA) of , in the visible wavelength from 600 nm to 900…
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