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Atacama Submillimeter Telescope Experiment ASTE望遠鏡 阿塔卡马亚毫米望远镜实验 Atacama Submillimeter Telescope Experiment Atacama Submillimeter Telescope Experiment Atacama Submillimeter Telescope Experiment
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阿塔卡马亚毫米望远镜实验（英語：Atacama Submillimeter Telescope Experiment，ASTE）是由三菱电机制造的10米口径射电望远镜，它是阿塔卡馬大型毫米波/亞毫米波陣列（ALMA）的前原型。 ASTE部署在查南托峰（Cerro Chajnantor）附近的潘帕拉博拉（Pampa La Bola）和智利北部的。望远镜具有优异的性能，表面精度的方均根达到19μm。利用卫星连接和互联网可以从多个站点远程控制该望远镜。它由日本国家天文台、东京大学、名古屋大学、大阪府立大学与智利大学合作运营。 The Atacama Submillimeter Telescope Experiment (ASTE) is a 10-meter-diameter antenna built by Mitsubishi Electric as a preprototype for ALMA. The ASTE was deployed to its site on Pampa La Bola, near Cerro Chajnantor and the Llano de Chajnantor Observatory in northern Chile. The antenna shows excellent performance including a surface accuracy of 19 μm (0.00075 in) r.m.s. The telescope is remotely controllable from multiple sites through satellite connections and the Internet. It is operated by the National Astronomical Observatory of Japan and the University of Tokyo, Nagoya University, and Osaka Prefecture University, in cooperation with the Universidad de Chile. ASTE望遠鏡（アステぼうえんきょう）は日本の国立天文台が南米の標高4800mの高地に設置し運用を行う電波望遠鏡である。 チリ北部アントファガスタ州のアタカマ砂漠に位置する。ASTEという名称はアタカマサブミリ波望遠鏡実験（アタカマサブミリはぼうえんきょうじっけん、英: Atacama Submillimeter Telescope Experiment）の略。最後に実験が付くのは、後述のようにテスト機としての役割を担っているためである。 ASTEは、技術領域における「実験」という意味と研究補助「実験」の意味を重ねたものである。そのため、鏡面精度は、20μmという高い精度や実験運用段階にあるボロメータ受信機などを搭載している。また、「実験」プラットホームという意味がある。 L'Atacama Submillimeter Telescope Experiment (ASTE) est une antenne/télescope millimétrique de 10 mètres de diamètre, construite par Mitsubishi Electric, installée dans le désert d'Atacama, au Chili et qui sert comme prototype pour le projet Atacama Large Millimeter Array (ALMA). L’Atacama Submillimeter Telescope Experiment (ASTE) è un telescopio per frequenze sub-millimetriche costituito da un'antenna da 10 metri costruita da Mitsubishi Electric, gestito dall'Osservatorio astronomico nazionale del Giappone (NAOJ) in collaborazione con l'università del Cile ed altri atenei giapponesi. ASTE è stato precursore del complesso osservativo ALMA verso il quale sono confluiti i successivi sforzi del NAOJ concernenti l'astronomia osservativa ad onde corte. Das Atacama Submillimeter Telescope Experiment ASTE ist ein Radioteleskop für den Submillimeterbereich. Das ASTE-Teleskop mit 10 m Antennendurchmesser und hochgenauer Reflektorfläche wurde von Mitsubishi Electric als Vorentwurf einer Antenne für das Atacama Large Millimeter Array ALMA gebaut. Es ist seit 2004 als Einzelteleskop für Frequenzen bis zu 900 GHz in der Pampa La Bola in 4860 m Höhe in der Nähe des ALMA-Standorts in Chile in Betrieb. ASTE ist ein Projekt des National Astronomical Observatory of Japan, mehrerer japanischer Universitäten und der Universidad de Chile.
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阿塔卡马亚毫米望远镜实验（英語：Atacama Submillimeter Telescope Experiment，ASTE）是由三菱电机制造的10米口径射电望远镜，它是阿塔卡馬大型毫米波/亞毫米波陣列（ALMA）的前原型。 ASTE部署在查南托峰（Cerro Chajnantor）附近的潘帕拉博拉（Pampa La Bola）和智利北部的。望远镜具有优异的性能，表面精度的方均根达到19μm。利用卫星连接和互联网可以从多个站点远程控制该望远镜。它由日本国家天文台、东京大学、名古屋大学、大阪府立大学与智利大学合作运营。 ASTE望遠鏡（アステぼうえんきょう）は日本の国立天文台が南米の標高4800mの高地に設置し運用を行う電波望遠鏡である。 チリ北部アントファガスタ州のアタカマ砂漠に位置する。ASTEという名称はアタカマサブミリ波望遠鏡実験（アタカマサブミリはぼうえんきょうじっけん、英: Atacama Submillimeter Telescope Experiment）の略。最後に実験が付くのは、後述のようにテスト機としての役割を担っているためである。 ASTEは、技術領域における「実験」という意味と研究補助「実験」の意味を重ねたものである。そのため、鏡面精度は、20μmという高い精度や実験運用段階にあるボロメータ受信機などを搭載している。また、「実験」プラットホームという意味がある。 Das Atacama Submillimeter Telescope Experiment ASTE ist ein Radioteleskop für den Submillimeterbereich. Das ASTE-Teleskop mit 10 m Antennendurchmesser und hochgenauer Reflektorfläche wurde von Mitsubishi Electric als Vorentwurf einer Antenne für das Atacama Large Millimeter Array ALMA gebaut. Es ist seit 2004 als Einzelteleskop für Frequenzen bis zu 900 GHz in der Pampa La Bola in 4860 m Höhe in der Nähe des ALMA-Standorts in Chile in Betrieb. ASTE ist ein Projekt des National Astronomical Observatory of Japan, mehrerer japanischer Universitäten und der Universidad de Chile. L'Atacama Submillimeter Telescope Experiment (ASTE) est une antenne/télescope millimétrique de 10 mètres de diamètre, construite par Mitsubishi Electric, installée dans le désert d'Atacama, au Chili et qui sert comme prototype pour le projet Atacama Large Millimeter Array (ALMA). L'ASTE a été installée sur le site de Pampa La Bola, près du Cerro Chajnantor et de l'Observatoire du Llano de Chajnantor dans le nord du Chili. Depuis son installation, l'antenne a fait preuve d'excellentes performances, et en particulier a une surface d'une précision de 19 μm (0.00075 in) r.m.s. Le télescope est contrôlé à distance grâce à des connexions satellitaires et Internet. Il est exploité par l'Observatoire astronomique national du Japon et l'Université de Tokyo, l'Université de Nagoya et l'Université d'Osaka, en coopération avec l'Université du Chili. The Atacama Submillimeter Telescope Experiment (ASTE) is a 10-meter-diameter antenna built by Mitsubishi Electric as a preprototype for ALMA. The ASTE was deployed to its site on Pampa La Bola, near Cerro Chajnantor and the Llano de Chajnantor Observatory in northern Chile. The antenna shows excellent performance including a surface accuracy of 19 μm (0.00075 in) r.m.s. The telescope is remotely controllable from multiple sites through satellite connections and the Internet. It is operated by the National Astronomical Observatory of Japan and the University of Tokyo, Nagoya University, and Osaka Prefecture University, in cooperation with the Universidad de Chile. Initially operating at 240 GHz using a focal-plane bolometer array, the telescope was upgraded in 2018 with a heterodyne receiver system operating at 345 GHz and 460 GHz. L’Atacama Submillimeter Telescope Experiment (ASTE) è un telescopio per frequenze sub-millimetriche costituito da un'antenna da 10 metri costruita da Mitsubishi Electric, gestito dall'Osservatorio astronomico nazionale del Giappone (NAOJ) in collaborazione con l'università del Cile ed altri atenei giapponesi. ASTE è stato precursore del complesso osservativo ALMA verso il quale sono confluiti i successivi sforzi del NAOJ concernenti l'astronomia osservativa ad onde corte. ASTE è collocato a Pampa La Bola nel deserto di Atacama, Cile, vicino all'osservatorio di Llano de Chajnantor presso il cerro omonimo nel nord del paese. Il telescopio è controllabile da remoto da più siti tramite connessioni satellitari e Internet, ovviando alle difficoltà causate dall'altitudine elevata e dall'accessibilità limitata. Inizialmente operante per campionare frequenze intorno ai 240 GHz utilizzando una matrice di bolometri collocati sul piano focale, il telescopio è stato aggiornato nel 2018 con un sistema di ricevitori per frequenze maggiori, a 345 GHz ed a 460 GHz.
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