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- AMiBA abstract "The Yuan-Tseh Lee Array for Microwave Background Anisotropy, also known as the Array for Microwave Background Anisotropy (AMiBA), is a radio telescope designed to observe the cosmic microwave background and the Sunyaev-Zel'dovich effect in clusters of galaxies. It is located on Mauna Loa in Hawaii, at 3,396 metres (11,142 ft) above sea level.AMiBA was originally configured as a 7-element interferometer atop a hexapod mount. Observations at a wavelength of 3 mm (86–102 GHz) started in October 2006, and the detections of six clusters by the Sunyaev-Zel'dovich effect were announced in 2008. In 2009 the telescope was upgraded to 13 elements, and it is capable of further expansion to 19 elements. AMiBA is the result of a collaboration between the Academia Sinica Institute of Astronomy and Astrophysics, the National Taiwan University and the Australia Telescope National Facility, and also involves researchers from other universities.".
- AMiBA thumbnail AMiBA_1.jpg?width=300.
- AMiBA wikiPageExternalLink amiba.asiaa.sinica.edu.tw.
- AMiBA wikiPageID "19876261".
- AMiBA wikiPageRevisionID "601658029".
- AMiBA altitude "3,396 m".
- AMiBA angularResolution "2".
- AMiBA angularResolution "6".
- AMiBA built "2000".
- AMiBA caption "AMiBA during construction in 2006".
- AMiBA diameter "0.576 m".
- AMiBA dome "Retractable shelter".
- AMiBA firstLight "September 2006".
- AMiBA hasPhotoCollection AMiBA.
- AMiBA location "Mauna Loa, Hawaii".
- AMiBA mounting "Hexapod platform".
- AMiBA name "Array for Microwave Background Anisotropy".
- AMiBA style Interferometry.
- AMiBA wavelength "3.0".
- AMiBA website amiba.asiaa.sinica.edu.tw.
- AMiBA subject Category:Cosmic_microwave_background_experiments.
- AMiBA point "19.536194444444444 -155.57527777777779".
- AMiBA type Artifact100021939.
- AMiBA type Device103183080.
- AMiBA type Instrument103574816.
- AMiBA type Instrumentality103575240.
- AMiBA type Magnifier103709206.
- AMiBA type Object100002684.
- AMiBA type PhysicalEntity100001930.
- AMiBA type ScientificInstrument104147495.
- AMiBA type Telescope104403638.
- AMiBA type Whole100003553.
- AMiBA type SpatialThing.
- AMiBA comment "The Yuan-Tseh Lee Array for Microwave Background Anisotropy, also known as the Array for Microwave Background Anisotropy (AMiBA), is a radio telescope designed to observe the cosmic microwave background and the Sunyaev-Zel'dovich effect in clusters of galaxies. It is located on Mauna Loa in Hawaii, at 3,396 metres (11,142 ft) above sea level.AMiBA was originally configured as a 7-element interferometer atop a hexapod mount.".
- AMiBA label "AMiBA".
- AMiBA label "AMiBA".
- AMiBA label "宇宙微波背景輻射陣列".
- AMiBA sameAs AMiBA.
- AMiBA sameAs m.04q7vcw.
- AMiBA sameAs Q1094807.
- AMiBA sameAs Q1094807.
- AMiBA sameAs AMiBA.
- AMiBA lat "19.536194444444444".
- AMiBA long "-155.57527777777779".
- AMiBA wasDerivedFrom AMiBA?oldid=601658029.
- AMiBA depiction AMiBA_1.jpg.
- AMiBA homepage amiba.asiaa.sinica.edu.tw.
- AMiBA isPrimaryTopicOf AMiBA.