The Mid-Infrared Instrument for theJames Webb Space Telescope, VI: The Medium Resolution Spectrometer

Authors:
  • MWMartyn Wells
    Martyn Wells
  • JPJ.-W. Pel
    J.-W. Pel
  • AGAlistair Glasse
    Alistair Glasse
  • GWG. S. Wright
    G. S. Wright
  • GAGabby Aitink-Kroes
    Gabby Aitink-Kroes
  • SBSteven Beard
    Steven Beard
  • BBB. R. Brandl
    B. R. Brandl
  • AGAngus Gallie
    Angus Gallie
  • VGV. C. Geers
    V. C. Geers
  • AGA. M. Glauser
    A. M. Glauser
  • PHPeter Hastings
    Peter Hastings
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Abstract
We describe the design and performance of the Medium Resolution Spectrometer (MRS) for the JWST-MIRI instrument. The MRS incorporates four coaxial spectral channels in a compact opto-mechanical layout that generates spectral images over fields of view up to 7.7 X 7.7 arcseconds in extent and at spectral resolving powers ranging from 1,300 to 3,700. Each channel includes an all-reflective integral field unit (IFU): an 'image slicer' that reformats the input field for presentation to a grating spectrometer. Two 1024 X 1024 focal plane arrays record the output spectral images with an instantaneous spectral coverage of approximately one third of the full wavelength range of each channel. The full 5 to 28.5 micron spectrum is then obtained by making three exposures using gratings and pass-band-determining filters that are selected using just two three-position mechanisms. The expected on-orbit optical performance is presented, based on testing of the MIRI Flight Model and including spectral and spatial coverage and resolution. The point spread function of the reconstructed images is shown to be diffraction limited and the optical transmission is shown to be consistent with the design expectations
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