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The Yuan-Tseh Lee Array for Microwave Background property, conjointly referred to as the Array for Microwave Background property (AMiBA), may be a radio reflector designed to watch the cosmic microwave background and also the Sunyaev-Zel’dovich impact in clusters of galaxies. It’s situated on Mauna Loa in Hawaii, at 3,396 m on top of water level.
AMiBA is presently designed as a 7-element measuring instrument atop a hexapod mount. Observations at a wavelength of three millimeter (86–102 Ghz) started in Oct 2006, and also the detections of six clusters by the Sunyaev-Zel’dovich impact were declared in 2008. The telescope are going to be upgraded to thirteen components by early 2009 and is expandable up to nineteen components. AMiBA is that the results of a collaboration between the academe Sinica Institute of physics and uranology, the National Taiwan University and also the Australia Telescope National Facility, and conjointly involves researchers from different universities.
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