Paper
28 July 2008 Recent progress at the MIRA: development of fringe tracking system
Naoko Ohishi, Masanori Yoshizawa, Jun Nishikawa, Naoshi Murakami, Yasuo Torii, Syunsaku Suzuki, Koichi Kubo, Hikaru Iwashita, Yoshinobu Kondo
Author Affiliations +
Abstract
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.
© (2008) COPYRIGHT Society of Photo-Optical Instrumentation Engineers (SPIE). Downloading of the abstract is permitted for personal use only.
Naoko Ohishi, Masanori Yoshizawa, Jun Nishikawa, Naoshi Murakami, Yasuo Torii, Syunsaku Suzuki, Koichi Kubo, Hikaru Iwashita, and Yoshinobu Kondo "Recent progress at the MIRA: development of fringe tracking system", Proc. SPIE 7013, Optical and Infrared Interferometry, 701305 (28 July 2008); https://doi.org/10.1117/12.788985
Lens.org Logo
CITATIONS
Cited by 1 scholarly publication.
Advertisement
Advertisement
RIGHTS & PERMISSIONS
Get copyright permission  Get copyright permission on Copyright Marketplace
KEYWORDS
Interferometers

Polarimetry

Ferroelectric materials

Mirrors

Control systems

Sensors

Interferometry

Back to Top