• DocumentCode
    280513
  • Title

    XMM-X-ray multimirror mission

  • Author

    Cole, R.E.

  • Author_Institution
    Dept. of Phys., Leicester Univ., UK
  • fYear
    1990
  • fDate
    33190
  • Firstpage
    42491
  • Lastpage
    42493
  • Abstract
    The X-ray multimirror mission is the second cornerstone of the Horizon 2000 programme. The aim of the mission is to carry out high throughput X-ray spectroscopy of celestial objects in the energy range 0.1 to 10 keV. Three telescopes each contain a nest of grazing incidence mirrors focussing X-rays onto a CCD camera. Two of the telescopes also contain a reflection grating spectrometer each with a further, dedicated CCD camera. A 30 cm optical telescope is mounted parallel to the X-ray telescopes to monitor the X-ray sources in the visible and UV bands. The chief areas of technology development are in the X-ray mirror fabrication, the CCD detectors for the cameras and the intensifier tubes for the optical telescope. Currently in a technology development and science definition phase, XMM is due for launch in 1998
  • Keywords
    CCD image sensors; X-ray astronomy; X-ray spectrometers; X-ray spectroscopy; artificial satellites; astronomical telescopes; mirrors; television cameras; 0.1 to 10 keV; CCD camera; CCD detectors; Horizon 2000 programme; UV bands; X-ray astronomy; X-ray mirror fabrication; X-ray multimirror mission; X-ray sources; X-ray spectroscopy; X-ray telescopes; celestial objects; grazing incidence mirrors; intensifier tubes; optical telescope; reflection grating spectrometer; visible band;
  • fLanguage
    English
  • Publisher
    iet
  • Conference_Titel
    UK Interest in Horizon 2000 - The ESA Space Science Programme, IEE Colloquium on
  • Conference_Location
    London
  • Type

    conf

  • Filename
    190834