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JEM-X: The X-ray monitor on INTEGRAL

    Research output: Chapter in Book/Report/Conference proceeding › Article in proceedings › Research › peer-review

    Abstract

    The INTEGRAL X-ray monitor, JEM-X, (together with the two gamma ray instruments, SPI and IBIS) provides simultaneous imaging with arcminute angular resolution in the 3-35 keV band. The good angular resolution and low energy response of JEM-X plays an important role in the detection and identification of gamma ray sources as well as in the analysis and scientific interpretation of the combined X-ray and gamma ray data. JEM-X is a coded aperture X-ray telescope consisting of two identical detectors. Each detector has a sensitive area of 500 cm(2), and views the sky through its own coded aperture mask. The coded masks are located 3.4 m above the detector windows. The detector field of view is constrained by X-ray collimators (6.6degrees FOV, FWHM).
    Original languageEnglish
    Title of host publicationX-ray and Gamma-ray Instumentation for Astronomy XIII
    EditorsKathryn A Flanagan, Oswald H. W Siegmund
    Publication date2004
    Pages139-150
    ISBN (Print)0-8194-5038-3
    DOIs
    Publication statusPublished - 2004
    EventX-ray and Gamma-ray Instrumentation for Astronomy XIII - San Diego, CA, United States
    Duration: 3 Aug 2003 → 5 Aug 2003

    Conference

    ConferenceX-ray and Gamma-ray Instrumentation for Astronomy XIII
    Country/TerritoryUnited States
    CitySan Diego, CA
    Period03/08/2003 → 05/08/2003
    SeriesProceedings of SPIE - The International Society for Optical Engineering
    ISSN0277-786X

    Keywords

    • JEM-X
    • INTEGRAL
    • X-ray astronomy
    • micro strip detector

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