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