Development of bolometric astronomical interferometer in mm and submm bands

Makoto Hattori, I. S. Ohta, H. Matsuo, J. Takahashi

Research output: Chapter in Book/Report/Conference proceedingConference contribution

Abstract

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.

Original languageEnglish
Title of host publicationThe Joint 30th International Conference on Infrared and Millimeter Waves and 13th International Conference on Terahertz Electronics, 2005. IRMMW-THz 2005
Pages531-532
Number of pages2
Publication statusPublished - 2005 Dec 1
Event30th International Conference on Infrared and Millimeter Waves and 13th International Conference on Terahertz Electronics, 2005. IRMMW-THz 2005 - Williamsburg, VA, United States
Duration: 2005 Sep 192005 Sep 23

Publication series

NameThe Joint 30th International Conference on Infrared and Millimeter Waves and 13th International Conference on Terahertz Electronics, 2005. IRMMW-THz 2005
Volume2

Other

Other30th International Conference on Infrared and Millimeter Waves and 13th International Conference on Terahertz Electronics, 2005. IRMMW-THz 2005
CountryUnited States
CityWilliamsburg, VA
Period05/9/1905/9/23

ASJC Scopus subject areas

  • Engineering(all)

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