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    Development of bolometric astronomical interferometer in mm and submm bands

    Development of bolometric astronomical interferometer in mm and submm bands


    We are developing a bolometric astronomical interferometer in mm and submm wave bands by applying Martin-Puplett type Fourier transform spectrometer to aperture synthesis technique. Since the spectroscopically resolved intensity distribution of four Stokes parameters are measurable by this instrument, we refer this to multi-components Fourier transform interferometer abbreviated as MuFT. Fundamentals of the MuFT with results of laboratory experiments and current status of astronomical observations with MuFT are summarized.

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    Titel :

    Development of bolometric astronomical interferometer in mm and submm bands

    Beteiligte:
    Hattori, M. (Autor:in) / Ohta, S. (Autor:in) / Matsuo, H. (Autor:in) / Takahashi, J. (Autor:in)
    Erschienen in:

    2005 Joint 30th International Conference on Infrared and Millimeter Waves and 13th International Conference on Terahertz Electronics ; 2 ; 531-532 vol. 2

    Erscheinungsdatum :

    2005-01-01

    Format / Umfang :

    1705835 byte

    ISBN :

    0-7803-9348-1

    DOI :

    https://doi.org/10.1109/ICIMW.2005.1572649

    Medientyp :

    Aufsatz (Konferenz)

    Format :

    Elektronische Ressource

    Sprache :

    Englisch

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