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<oembed><version>1.0</version><provider_name>KMI - Nagoya University</provider_name><provider_url>https://www.kmi.nagoya-u.ac.jp/eng</provider_url><title>The Future of Very High Energy Astrophysics - KMI - Nagoya University</title><type>rich</type><width>600</width><height>338</height><html>&lt;blockquote class="wp-embedded-content" data-secret="NwO3tzRjGn"&gt;&lt;a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/996/"&gt;The Future of Very High Energy Astrophysics&lt;/a&gt;&lt;/blockquote&gt;&lt;iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/996/embed/#?secret=NwO3tzRjGn" width="600" height="338" title="&#x201C;The Future of Very High Energy Astrophysics&#x201D; &#x2014; KMI - Nagoya University" data-secret="NwO3tzRjGn" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"&gt;&lt;/iframe&gt;&lt;script type="text/javascript"&gt;
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</html><description>The field of very high energy (VHE) astrophysics had been revolutionized by the results from ground-based gamma-ray telescopes, including the current imaging atmospheric Cherenkov telescope (IACT) arrays: HESS, MAGIC and VERITAS. A worldwide consortium of scientists from 32 countries has formed to develop the Cherenkov Telescope Array (CTA) that will capitalize on the power of this technique to greatly expand the scientific reach of ground-based gamma-ray telescopes. CTA science topics will include the origin of cosmic rays and cosmic particle &hellip;</description></oembed>
