欧空局研究用于超新星调查和暗能量表征的宽视场成像仪

P. Gondoin, V. Kirschner, A. Santovincenzo, A. Lyngvi
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引用次数: 0

摘要

本文总结了欧空局利用广角光学红外成像仪(WFI)寻找低红移Ia型超新星以测量宇宙膨胀变化率的可行性研究结果。WFI深宇宙的多光谱图像也可以使天体物理学的许多其他研究领域受益。WFI有效载荷包括一个2米级望远镜,一个1平方度视场成像相机和一个低分辨率积分场光谱仪。确定了一个任务概念,其中包括
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ESA study of a wide field imager for supernovae surveys and dark energy characterization
This paper summarizes the results of an ESA feasibility study of a Wide-Field Optical Infrared Imager (WFI) that would search for Type Ia supernovae at low redshift with the aim to measure the changing rate of expansion of the universe. WFI multi-spectral images of the deep universe could also benefit to many other research area in astrophysics. The WFI payload includes a 2 m class telescope, a 1 square degree field of view imaging camera and a low-resolution integral field spectrometer. A mission concept was identified that consists of
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ESA study of a wide field imager for supernovae surveys and dark energy characterization Drag-free deep-space laser ranging missions for fundamental physics
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