About: South Pole Telescope

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The South Pole Telescope (SPT) is a 10-metre (390 in) diameter telescope located at the Amundsen–Scott South Pole Station, Antarctica. The telescope is designed for observations in the microwave, millimeter-wave, and submillimeter-wave regions of the electromagnetic spectrum, with the particular design goal of measuring the faint, diffuse emission from the cosmic microwave background (CMB). The first major survey with the SPT—designed to find distant, massive, clusters of galaxies through their interaction with the CMB, with the goal of constraining the dark energy equation of state—was completed in October 2011. In early 2012, a new camera (SPTpol) was installed on the SPT with even greater sensitivity and the capability to measure the polarization of incoming light. This camera operated

Attributes	Values
rdf:type	yago:WikicatTelescopes yago:WikicatSubmillimetreTelescopes yago:Artifact100021939 yago:AstronomicalTelescope102751295 yago:Device103183080 yago:Instrument103574816 yago:Instrumentality103575240 yago:Magnifier103709206 yago:Object100002684 yago:PhysicalEntity100001930 yago:RadioTelescope104044716 yago:ScientificInstrument104147495 yago:Telescope104403638 yago:Whole100003553 yago:WikicatRadioTelescopes ArtificialSatellite
rdfs:label	مرصد القطب الجنوبي (ar) South Pole Telescope (de) Suda Polusa Teleskopo (eo) Telescopio Polo Sur (es) Teleskop South Pole (in) South Pole Telescope (it) South Pole Telescope (fr) 南極点望遠鏡 (ja) South Pole Telescope (pl) Telescópio do Polo Sul (pt) South Pole Telescope (en) Южный полярный телескоп (ru) Південний полярний телескоп (uk) 南极望远镜 (zh)
rdfs:comment	Suda Polusa Teleskopo (SPT) — estas la radioteleskopo de tipo de parabola reflektoro kun diametro de la ĉefa spegulo D = 10 m. Ĝi estas situanta sur la teritorio de Polusa stacio Amundsen-Scott en Antarktio. (eo) El Telescopio Polo Sur es un nuevo telescopio desplegado en el Polo Sur que está diseñado para estudiar el fondo cósmico de microondas. Construido entre noviembre de 2006 y febrero de 2007, el SPT es el telescopio más grande jamás desplegado en el Polo Sur. Este telescopio proporciona una nueva y poderosa herramienta para estudiar la energía oscura. (es) 南極点望遠鏡（なんきょくてんぼうえんきょう、South Pole Telescope, SPT）は、南極点に建設された口径10メートルの電波望遠鏡である。北アメリカの9つの大学及び研究機関が参加するSPT Collaborationが運用を行う。 (ja) O Telescópio do Polo Sul é um telescópio de 10 metros de diâmetro localizado na estação Amundsen–Scott, na Antártida. O telescópio é projetado para observações de vários tipos de ondas, no espectro eletromagnético, com o objetivo de medir a emissão difusa da radiação cósmica de fundo (CMB). A primeira grande pesquisa com o SPT – projetado para localizar aglomerados de galáxias distantes – foi concluída em outubro de 2011. No início de 2012, uma nova câmara foi instalada no SPT com maior sensibilidade e capacidade de medir a polarização da luz incidente. Esta câmera é projetada para medir o chamado "modo-B" ou componente "rotacional", levando a restrições sobre a massa do neutrino e a escala de energia de inflação. (pt) Южный полярный телескоп (SPT, англ. South Pole Telescope) — 10-метровый радиотелескоп в обсерватории в Антарктиде на станции Амундсен-Скотт на географическом южном полюсе Земли.Телескоп предназначен для наблюдений в микроволновых, миллиметровых и субмиллиметровых длинах волн.Основная цель — измерение слабого диффузного излучения от космического микроволнового фона (CMB). (ru) Південнополюсний телескоп, The South Pole Telescope (SPT) — це 10-ти метровий телескоп на полярній станції Амудсена-Скотта в Антарктиді. Цей високочастотний телескоп оглядає небо в частотах 70-300 ГГц. Головна наукова мета — знайти тисячі кластерів галактик, а також темну матерію (uk) 南极望远镜（英語：The South Pole Telescope，简称：SPT）是一个位于南极洲南极点阿蒙森-史考特南极站的10米（394英寸）直径的射电望远镜。它是一个微波/毫米波望远镜，观测的频率范围在70－300千兆赫兹（GHz）之间。南极望远镜的主要科学任务是调查南天球数千个星系团之间的联系，这些星系团可能约束暗能量的作用而处于平衡状态。这个望远镜由芝加哥大学、柏克莱加州大学、凯斯西储大学、伊利诺伊大学厄巴纳-香槟分校、史密松天体物理台、科罗拉多大学博尔德分校、麦吉尔大学和戴维斯加利福尼亚大学等八所大学或机构组成的工作小组共同运行，由美国国家科学基金会提供资金支持。 (zh) مرصد القطب الجنوبي أو تلسكوب القطب الجنوبي (بالإنجليزية:(South Pole Telescope (SPT) هو تلسكوب راديوي له طاسة (هوائي) في شكل قطع مكافيء يبلغ قطرها 10 متر، وهو يقع في . يقيس التلسكوب في حيز الموجات الكهرومغناطيسية تحت المليمتر، أي يقيس الترددات 95، و150 و220 ميجا هرتز. (ar) Das South Pole Telescope (SPT) ist ein Radioteleskop mit 10 m Reflektordurchmesser mit Standort an der Amundsen-Scott-Südpolstation. Das SPT arbeitet im Millimeterwellenbereich bei Frequenzen von 95, 150 und 220 GHz. Durch die hervorragenden Eigenschaften des kalten und trockenen Beobachtungsstandorts am Südpol und durch Verwendung großer Bolometerkameras mit zurzeit 960 Elementen können rasch große Himmelsgebiete kartiert werden. Die Genauigkeit des Reflektors erlaubt auch zukünftige Beobachtungen im Submillimeterbereich. (de) Le South Pole Telescope (SPT) est un radiotélescope de 10 mètres de diamètre situé à la station polaire Amundsen-Scott sur l'Antarctique. Le télescope est conçu pour observer les régions micro-ondes, d'ondes millimétriques et d'ondes sub-millimétriques du spectre électromagnétique, avec le dessein particulier de mesurer les émissions en provenance du fond diffus cosmologique.Son premier arpentage (achevé en octobre 2010) cherchait à repérer les gros amas de galaxies lointains par leur interaction avec le fond diffus cosmologique, en vue de contraindre l'équation d'état de l'énergie noire. Au début de 2012, un nouvel appareil capteur fut installé sur le SPT ayant la vocation d'étudier le fond diffus cosmologique. Encore plus sensible et capable d'évaluer la polarisation de la lumière entran (fr) Teleskop South Pole atau The South Pole Telescope (SPT) adalah sebuah teleskop diameter 10 meter (394 in) terletak di Amundsen-Scott Station South Pole, Antartika. Teleskop ini dirancang untuk pengamatan di microwave, gelombang milimeter, dan wilayah gelombang submillimeter dari spektrum elektromagnetik, dengan desain tujuan tertentu untuk pengukuran samar, emisi menyebar dari Cosmic Microwave Background (CMB). (in) The South Pole Telescope (SPT) is a 10-metre (390 in) diameter telescope located at the Amundsen–Scott South Pole Station, Antarctica. The telescope is designed for observations in the microwave, millimeter-wave, and submillimeter-wave regions of the electromagnetic spectrum, with the particular design goal of measuring the faint, diffuse emission from the cosmic microwave background (CMB). The first major survey with the SPT—designed to find distant, massive, clusters of galaxies through their interaction with the CMB, with the goal of constraining the dark energy equation of state—was completed in October 2011. In early 2012, a new camera (SPTpol) was installed on the SPT with even greater sensitivity and the capability to measure the polarization of incoming light. This camera operated (en) Il South Pole Telescope (SPT) è un radiotelescopio di 10 metri situato presso la base Amundsen-Scott, al Polo Sud, Antartide. Il telescopio osserva nelle microonde e nelle onde millimetriche tra i 70 e i 300 GHz. Lo scopo principale del SPT è di esplorare il cielo al fine di mappare le anisotropie primarie e secondarie della radiazione cosmica di fondo (CMB). (it) South Pole Telescope (SPT) – radioteleskop zbudowany w stacji Amundsena-Scotta na biegunie południowym przez konsorcjum amerykańskich uczelni. Rozpoczął pracę w lutym 2007. Pracuje w paśmie częstotliwości 70-300 GHz (mikrofale) i jest przeznaczony do poszukiwania odległych gromad galaktyk metodą wykorzystującą efekt Suniajewa-Zeldowicza. (pl)
foaf:homepage	http://pole.uchicago.edu/
foaf:depiction
dcterms:subject	Astronomical telescopes and observatories in the Antarctic Submillimetre telescopes 2007 establishments in Antarctica Radio telescopes Cosmic microwave background experiments
Wikipage page ID	2260546 (xsd:integer)
Wikipage revision ID	1093291402 (xsd:integer)
Link from a Wikipage to another Wikipage	Case Western Reserve University Electromagnetic spectrum List of astronomical observatories Astronomical telescopes and observatories in the Antarctic Submillimetre telescopes United States Department of Energy University of California, Berkeley University of California, Davis University of Chicago University of Colorado Boulder University of Illinois at Urbana–Champaign 2007 establishments in Antarctica Intracluster medium Cosmic microwave background radiation Cosmological constant McGill University Gordon and Betty Moore Foundation Cosmic microwave background Equatorial mount Ludwig Maximilian University of Munich Smithsonian Astrophysical Observatory Polar night Thou Amundsen–Scott South Pole Station Radio telescopes Dark Energy Dark energy Altazimuth mount Extremely high frequency Fermilab Harvard University Terahertz radiation Argonne National Laboratory Atacama Cosmology Telescope Cosmic microwave background experiments Kavli Foundation (United States) BICEP and Keck Array Bolometer Square degree Gregorian telescope Inch Michigan State University Microwave National Science Foundation Redshift Lists of telescopes

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