论文标题
詹姆斯·韦伯太空望远镜孔掩模干涉仪
The James Webb Space Telescope Aperture Masking Interferometer
论文作者
论文摘要
在不到一年的时间里，詹姆斯·韦伯（James Webb）太空望远镜（JWST）将继承成为世界上杰出的红外天文台的地幔。 JWST将携带Aperture屏蔽干涉仪（AMI），作为近红外成像仪和无slitless spectragraph（NIRISS）仪器的受支持的操作模式之一。在如此强大的平台上，AMI模式将传递有史以来最先进，功能最高的干涉仪，超过了通过敏感性数量级的任何事物。在这里，我们介绍了该设施的设计和调试的关键方面：数据模拟（$ \ texttt {ami_sim} $），使用两种不同方法（$ \ texttt {implaneia} $ and $ \ \ \ \ \ \ \ \ \ \ texttttt {amical} $）提取干涉测量值可观察结果，对AMI的预期效果的更新view view view view and commition commition commition torge torge tocement torge profection tocement torge profection torge prosport及我们的sart vet vet vet vet。
In less than a year, the James Webb Space Telescope (JWST) will inherit the mantle of being the world's pre-eminent infrared observatory. JWST will carry with it an Aperture Masking Interferometer (AMI) as one of the supported operational modes of the Near-InfraRed Imager and Slitless Spectrograph (NIRISS) instrument. Aboard such a powerful platform, the AMI mode will deliver the most advanced and scientifically capable interferometer ever launched into space, exceeding anything that has gone before it by orders of magnitude in sensitivity. Here we present key aspects of the design and commissioning of this facility: data simulations ($\texttt{ami_sim}$), the extraction of interferometeric observables using two different approaches ($\texttt{IMPLANEIA}$ and $\texttt{AMICAL}$), an updated view of AMI's expected performance, and our reference star vetting programs.
