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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. After completion of the SZE campaigns, the telescope has been repurposed to study the evolution of molecular gas throughout the history of the Universe. It is now referred to as the Yuan-Tseh Lee Array (YTLA). It is located on Mauna Loa in Hawaii, at 3,396 metres (11,142 ft) above sea level.

Attributes	Values
rdf:type	yago:WikicatAstronomicalObservatoriesInHawaii yago:Artifact100021939 yago:Building102913152 yago:Object100002684 yago:Observatory103839671 yago:PhysicalEntity100001930 yago:YagoGeoEntity yago:YagoPermanentlyLocatedEntity yago:Structure104341686 yago:Whole100003553 ArtificialSatellite
rdfs:label	مصفوفة أميبا (ar) AMiBA (en) AMiBA (fr) AMiBA (sv) 宇宙微波背景輻射陣列 (zh)
rdfs:comment	مصفوفة أميبا مصفوفة يوان-تسيه لي لخلفية الميكروويف المتباين الخواص المعروفة أيضا باسم مصفوفة خلفية الميكروويف المتباين الخواص (AMiBA)، هو مقراب راديوي مصمم لمراقبة إشعاع الخلفية الكونية الميكروي وتأثير سونيايف-زيلدوفيتش في مجموعات المجرات. يقع المرصد في مونا لوا في هاواي، على ارتفاع 3,396 متر (11,142 قدم) فوق مستوى سطح البحر. (ar) L'AMiBA, acronyme de Array for Microwave Background Anisotropy, aussi appelé Yuan-Tseh Lee Array for Microwave Background Anisotropy, est un radiotélescope des États-Unis situé à Hawaï, sur le site de l'observatoire solaire du Mauna Loa, à 3 396 mètres d'altitude. Il a pour but l'observation du fond diffus cosmologique et de l'effet Sunyaev-Zel'dovich dans les amas de galaxies. Il est construit à partir de 2000 et est mis en service en septembre 2006. (fr) 宇宙微波背景輻射陣列（Array for Microwave Background Anisotropy, AMiBA），又稱為李遠哲陣列（Yuan-Tseh Lee Array for Microwave Background Anisotropy, YTLA），是用來觀測宇宙微波背景辐射和星系團苏尼亚耶夫-泽尔多维奇效应的電波望遠鏡。位於夏威夷冒纳罗亚火山，海拔3396公尺。 AMiBA 目前有 13 個干涉儀安裝在其六角型平台上。觀測波長是 3 mm (86–102 GHz)，於2006年10月建設完成。7 個偵測苏尼亚耶夫-泽尔多维奇效应的組件於2007年開始進行觀測，2010年組件增加至 13 個。AMiBA 計畫由中央研究院天文及天文物理研究所、國立臺灣大學、澳洲天文台以及其他大學合作進行。 (zh) 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. After completion of the SZE campaigns, the telescope has been repurposed to study the evolution of molecular gas throughout the history of the Universe. It is now referred to as the Yuan-Tseh Lee Array (YTLA). It is located on Mauna Loa in Hawaii, at 3,396 metres (11,142 ft) above sea level. (en) Yuan-Tseh Lee Array for Microwave Background Anisotropy, även känt som Array for Microwave Background Anisotropy (AMiBA), är ett radioteleskop som är utformat för att följa den kosmiska bakgrundsstrålningen och Sunyaev-Zeldovich-effekten i galaxhopar. Det ligger på Mauna Loas sluttning på ön Hawaii, på 3 396 meters höjd över havet. (sv)
foaf:depiction
dcterms:subject	Mauna Loa Astronomical observatories in Hawaii Cosmic microwave background experiments
Wikipage page ID	19876261 (xsd:integer)
Wikipage revision ID	1068545182 (xsd:integer)
Link from a Wikipage to another Wikipage	Canadian Institute for Theoretical Astrophysics List of astronomical observatories Monolithic microwave integrated circuit Decibel University of Bristol University of Hawaii Anisotropies Mauna Loa Radio telescope Cosmic microwave background Mauna Loa Subaru (telescope) Galaxy cluster Local oscillator Abell 1689 Abell 2142 Abell 2163 Abell 2261 Abell 2390 Academia Sinica Astronomical observatories in Hawaii Baryon Nottingham Trent University PVC Harvard-Smithsonian Center for Astrophysics Hawaii Atacama Large Millimeter Array Arcminute Cosmic microwave background experiments Jupiter Australia Telescope National Facility National Taiwan University Cassegrain reflector Redshift Interferometer Very Large Array Low noise amplifier Multipole First light (astronomy) National Radio Astronomy Observatory National Science Council Sunyaev-Zel'dovich effect Carbon fibre Taiwan Ministry of Education GHz System temperature Carnegie-Mellon University Yuan-Tseh Lee Weak lensing dbr:Abell_1995
sameAs	AMiBA AMiBA AMiBA AMiBA AMiBA AMiBA AMiBA AMiBA AMiBA
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thumbnail	wiki-commons:Special:FilePath/AMiBA_2.jpg?width=300
has abstract	مصفوفة أميبا مصفوفة يوان-تسيه لي لخلفية الميكروويف المتباين الخواص المعروفة أيضا باسم مصفوفة خلفية الميكروويف المتباين الخواص (AMiBA)، هو مقراب راديوي مصمم لمراقبة إشعاع الخلفية الكونية الميكروي وتأثير سونيايف-زيلدوفيتش في مجموعات المجرات. يقع المرصد في مونا لوا في هاواي، على ارتفاع 3,396 متر (11,142 قدم) فوق مستوى سطح البحر. (ar) 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. After completion of the SZE campaigns, the telescope has been repurposed to study the evolution of molecular gas throughout the history of the Universe. It is now referred to as the Yuan-Tseh Lee Array (YTLA). 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. (en)

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