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AMiBA PROJECT OVERVIEW- The Array for Microwave Background Anisotropy (AMiBA) , alsoknown as the Yuan-Tseh Lee Array for Microwave BackgroundAnisotropy
- This project:
- led, designed, constructed, and operated by the Academic SinicaInstitute of Astronomy and Astrophysics (ASIAA)
- major collaborations with National Taiwan University, PhysicsDepartment (NTUP), Electrical Engineering Department (NTUEE)and the Australian Telescope National Facility (ATNF).
- Contributions also came from the Carnegie Mellon University(CMU), and the National Radio Astronomy Observatory (NRAO).
- AMiBA is a radio telescope designed to observe the cosmicmicrowave background and the Sunyaev-Zel''dovich effect in clustersof galaxies.
- AMiBA is currently configured as a 7-element interferometer,using 0.576 m Cassegrain dishes mounted on a 6 m carbonfibre hexapod mount. It is located on Mauna Loa in Hawaii, at 3,396m above sea, and observes at 3 mm (86102 GHz) to minimizeforegrounds.The telescope has a retractable shelter, made fromseven steel trusses and PVC fabric.
AMiBA 1.2M Carbon Antenna ofRadio Telescope


