Recent progress at the MIRA: development of fringe tracking system
2008
The MIRA-I.2 is a 30m baseline optical interferometer located at the Mitaka campus of the National Astronomical
Observatory of Japan. After the detection of the first fringes with Vega in 2002, we have continued
improvement of system performance and have demonstrated stellar diameter measurement in wide band
(600nm-1000nm). Recently, we begin on development of two scientific detectors: spectrometer with separate
fringe tracking system and interfeometric polarimetry. Recent progress and performance of our two system is
reported.
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