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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    Title :

    Development of bolometric astronomical interferometer in mm and submm bands


    Contributors:
    Hattori, M. (author) / Ohta, S. (author) / Matsuo, H. (author) / Takahashi, J. (author)


    Publication date :

    2005-01-01


    Size :

    1705835 byte




    Type of media :

    Conference paper


    Type of material :

    Electronic Resource


    Language :

    English



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