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The Neutron star Interior Composition Explorer (NICER): design and development

机译:中子星内部组合探测器(NICER):设计和开发

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摘要

During 2014 and 2015, NASA's Neutron star Interior Composition Explorer (NICER) mission proceeded successfully through Phase C, Design and Development. An X-ray (0.2-12 keV) astrophysics payload destined for the International Space Station, NICER is manifested for launch in early 2017 on the Commercial Resupply Services SpaceX-11 flight. Its scientific objectives are to investigate the internal structure, dynamics, and energetics of neutron stars, the densest objects in the universe. During Phase C, flight components including optics, detectors, the optical bench, pointing actuators, electronics, and others were subjected to environmental testing and integrated to form the flight payload. A custom-built facility was used to co-align and integrate the X-ray "concentrator" optics and silicon-drift detectors. Ground calibration provided robust performance measures of the optical (at NASA's Goddard Space Flight Center) and detector (at the Massachusetts Institute of Technology) subsystems, while comprehensive functional tests prior to payload-level environmental testing met all instrument performance requirements. We describe here the implementation of NICER's major subsystems, summarize their performance and calibration, and outline the component-level testing that was successfully applied.
机译:在2014年和2015年期间,NASA的中子星内部成分探索器(NICER)任务成功完成了C阶段的设计和开发。 NICER的X射线(0.2-12 keV)天体物理学有效载荷发往国际空间站,已于2017年初在商业补给服务SpaceX-11航班上发射。其科学目的是研究中子星的内部结构,动力学和高能学。中子星是宇宙中最密集的物体。在阶段C中,对飞行组件(包括光学器件,检测器,光学平台,指向致动器,电子设备等)进行了环境测试,并进行了集成,以形成飞行有效载荷。使用定制的设备将X射线“聚光器”光学器件和硅漂移检测器进行对准和集成。地面校准为光学子系统(在NASA的戈达德太空飞行中心)和探测器(在麻省理工学院)提供了可靠的性能指标,而有效载荷级环境测试之前的全面功能测试满足了所有仪器性能要求。我们在这里描述NICER主要子系统的实现,总结其性能和校准,并概述成功应用的组件级测试。

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