Commissioning the scientific instruments of the James Webb Space Telescope

R. Kimble, S. Friedman, C. Oliveira, S. Birkmann, T. Boeker, M. Boyer, R. Doyon, A. Glasse, S. Kendrew, A. Martel, E. Nelan, A. Noriega-Crespo, C. Proffitt, Corbett T. Smith, J. Stansberry, B. Vila, C. Willott
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Abstract

The James Webb Space Telescope features a powerful complement of focal-plane instruments: the Mid-Infrared Instrument (MIRI), the Near-Infrared Camera (NIRCam), the Near-Infrared Imager and Slitless Spectrograph (NIRISS), the Near-Infrared Spectrograph (NIRSpec), and the Fine Guidance Sensor (FGS). These instruments offer an exciting suite of scientific capabilities for imaging, high-contrast imaging, and spectroscopy. To bring these capabilities on-line after launch, a carefully scoped and sequenced set of commissioning activities has been developed. These activities will confirm the functionality of the instruments, characterize their performance (optimizing where possible), obtain initial calibrations at a level required to properly plan observations, and demonstrate essential operational sequences such as target acquisition. We present a high-level overview of these activities and the planned commissioning timeline to execute them.
调试詹姆斯·韦伯太空望远镜的科学仪器
詹姆斯·韦伯太空望远镜拥有强大的焦平面仪器:中红外仪器(MIRI)、近红外相机(NIRCam)、近红外成像仪和无缝光谱仪(NIRISS)、近红外光谱仪(NIRSpec)和精细制导传感器(FGS)。这些仪器为成像、高对比度成像和光谱学提供了一套令人兴奋的科学能力。为了使这些功能在发射后上线,已经开发了一套精心设计和排序的调试活动。这些活动将确认仪器的功能,表征其性能(在可能的情况下进行优化),获得适当计划观测所需水平的初始校准,并演示基本的操作顺序,如目标获取。我们提供了这些活动的高级概述以及执行它们的计划调试时间表。
本文章由计算机程序翻译,如有差异,请以英文原文为准。
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