罗曼日冕仪社区参与计划：使用泽尼克波前传感器对罗曼空间望远镜及日冕仪进行全面表征
The Roman Coronagraph Community Participation Program: Using the Zernike wavefront sensor for a full characterisation of the Roman Space Telescope and the Coronagraph Instrument
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中文总结 AI 辅助
本研究主张启用罗曼空间望远镜日冕仪（CGI）搭载的双路泽尼克波前传感器（ZWFS），利用罗曼社区参与计划（CPP）的工具分析其灵敏度，以保障罗曼天文台稳定性并为HWO铺路。
中文摘要 AI 辅助
罗曼空间望远镜日冕仪（CGI）将展示一系列技术与方法，以实现空间天文台对反射光行星的直接探测。在CGI搭载的多种观测模式和日冕仪设备中，包含可直接测量系统光学像差的透射式双路泽尼克波前传感器（ZWFS）。目前该双路ZWFS尚未得到支持，本研究主张启用这一独特观测模式。我们利用罗曼社区参与计划（CPP）开发并支持的CGI模拟器及其他工具，研究ZWFS的灵敏度。此类分析对理解罗曼天文台的稳定性、为走向LUVOIR（HWO）铺平道路至关重要。
英文摘要
The Roman Space Telescope Coronagraph Instrument (CGI) will demonstrate a series of technologies and techniques to enable the direct detection of reflected-light planets with space-based observatories. Among the several available observing modes and coronagraphic devices embarked in CGI, there is the transmissive dual-path Zernike wavefront sensor (ZWFS) that could be used to directly measure optical aberrations in the system. The dual-path ZWFS is currently unsupported, but in this work we advocate for the commissioning of this unique observing mode. We investigate the sensitivity of the ZWFS using CGI simulator and other tools developed and supported by the Roman community participation program (CPP). This type of analysis is crucial for understanding the stability of the Roman observatory and to prepare the path towards HWO.
