{"id":2120,"date":"2020-06-18T13:06:19","date_gmt":"2020-06-18T04:06:19","guid":{"rendered":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/?post_type=seminar&p=2120"},"modified":"2021-07-13T14:46:30","modified_gmt":"2021-07-13T05:46:30","slug":"prototype-telescopes-of-the-cherenkov-telescope-array","status":"publish","type":"seminar","link":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/","title":{"rendered":"Prototype Telescopes of the Cherenkov Telescope Array"},"content":{"rendered":"

The Cherenkov Telescope Array (CTA) is the next-generation gamma-ray observatory to be completed in 2020s. CTA will be comprised of about 100 Cherenkov telescopes with three different mirror diameters to achieve a wide energy coverage of 20 GeV\u2013300 TeV, which will be deployed in the northern and southern CTA sites. The CTA Nagoya group has been actively involved in the development of three CTA prototype telescopes, all of them achieved gamma-ray detection or air-shower first light in last one year. I will briefly summarize some of physics motivations, prototype status, and future prospects of CTA.<\/span><\/p>\n

Slides<\/a><\/span><\/p>\n","protected":false},"featured_media":0,"template":"","tags":[],"seminar_category":[58],"acf":{"s_now_accepting":true,"s_date_order":"2020-06-24 17:30:00","s_date_end":null,"s_date_text":"","s_text":"Akira Okumura (KMI, Nagoya Univ.)","s_place":"","s_place_other":"","s_categoryother":"","s_poster":"","s_poster2":"","s_slide":""},"yoast_head":"\nPrototype Telescopes of the Cherenkov Telescope Array - KMI - Nagoya University<\/title>\n<meta name=\"robots\" content=\"index, follow, max-snippet:-1, max-image-preview:large, max-video-preview:-1\" \/>\n<link rel=\"canonical\" href=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/\" \/>\n<meta property=\"og:locale\" content=\"en_US\" \/>\n<meta property=\"og:type\" content=\"article\" \/>\n<meta property=\"og:title\" content=\"Prototype Telescopes of the Cherenkov Telescope Array - KMI - Nagoya University\" \/>\n<meta property=\"og:description\" content=\"The Cherenkov Telescope Array (CTA) is the next-generation gamma-ray observatory to be completed in 2020s. CTA will be comprised of about 100 Cherenkov telescopes with three different mirror diameters to achieve a wide energy coverage of 20 GeV\u2013300 TeV, which will be deployed in the northern and southern CTA sites. The CTA Nagoya group has been actively involved in the development of three CTA prototype telescopes, all of them achieved gamma-ray detection or air-shower first light in last one year. …\" \/>\n<meta property=\"og:url\" content=\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/\" \/>\n<meta property=\"og:site_name\" content=\"KMI - Nagoya University\" \/>\n<meta property=\"article:modified_time\" content=\"2021-07-13T05:46:30+00:00\" \/>\n<meta name=\"twitter:card\" content=\"summary_large_image\" \/>\n<script type=\"application\/ld+json\" class=\"yoast-schema-graph\">{\"@context\":\"https:\/\/schema.org\",\"@graph\":[{\"@type\":\"WebPage\",\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/\",\"url\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/\",\"name\":\"Prototype Telescopes of the Cherenkov Telescope Array - KMI - Nagoya University\",\"isPartOf\":{\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/#website\"},\"datePublished\":\"2020-06-18T04:06:19+00:00\",\"dateModified\":\"2021-07-13T05:46:30+00:00\",\"breadcrumb\":{\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/#breadcrumb\"},\"inLanguage\":\"en-US\",\"potentialAction\":[{\"@type\":\"ReadAction\",\"target\":[\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/\"]}]},{\"@type\":\"BreadcrumbList\",\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/#breadcrumb\",\"itemListElement\":[{\"@type\":\"ListItem\",\"position\":1,\"name\":\"Home\",\"item\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/\"},{\"@type\":\"ListItem\",\"position\":2,\"name\":\"Seminars\",\"item\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/\"},{\"@type\":\"ListItem\",\"position\":3,\"name\":\"Prototype Telescopes of the Cherenkov Telescope Array\"}]},{\"@type\":\"WebSite\",\"@id\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/#website\",\"url\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/\",\"name\":\"KMI - Nagoya University\",\"description\":\"Nagoya University: Kobayashi-Maskawa Institute for the Origin of Particles and the Universe (KMI)\",\"potentialAction\":[{\"@type\":\"SearchAction\",\"target\":{\"@type\":\"EntryPoint\",\"urlTemplate\":\"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/?s={search_term_string}\"},\"query-input\":{\"@type\":\"PropertyValueSpecification\",\"valueRequired\":true,\"valueName\":\"search_term_string\"}}],\"inLanguage\":\"en-US\"}]}<\/script>\n<!-- \/ Yoast SEO plugin. -->","yoast_head_json":{"title":"Prototype Telescopes of the Cherenkov Telescope Array - KMI - Nagoya University","robots":{"index":"index","follow":"follow","max-snippet":"max-snippet:-1","max-image-preview":"max-image-preview:large","max-video-preview":"max-video-preview:-1"},"canonical":"https:\/\/www.kmi.nagoya-u.ac.jp\/eng\/seminar\/2120\/","og_locale":"en_US","og_type":"article","og_title":"Prototype Telescopes of the Cherenkov Telescope Array - KMI - Nagoya University","og_description":"The Cherenkov Telescope Array (CTA) is the next-generation gamma-ray observatory to be completed in 2020s. 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