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
{"title":"Commissioning the scientific instruments of the James Webb Space Telescope","authors":"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","doi":"10.1117/12.2561819","DOIUrl":null,"url":null,"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.","PeriodicalId":185935,"journal":{"name":"Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave","volume":"36 1","pages":"0"},"PeriodicalIF":0.0000,"publicationDate":"2020-12-13","publicationTypes":"Journal Article","fieldsOfStudy":null,"isOpenAccess":false,"openAccessPdf":"","citationCount":"0","resultStr":null,"platform":"Semanticscholar","paperid":null,"PeriodicalName":"Space Telescopes and Instrumentation 2020: Optical, Infrared, and Millimeter Wave","FirstCategoryId":"1085","ListUrlMain":"https://doi.org/10.1117/12.2561819","RegionNum":0,"RegionCategory":null,"ArticlePicture":[],"TitleCN":null,"AbstractTextCN":null,"PMCID":null,"EPubDate":"","PubModel":"","JCR":"","JCRName":"","Score":null,"Total":0}
引用次数: 0
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.