1.0KMI - Nagoya Universityhttps://www.kmi.nagoya-u.ac.jp/engVery High Energy Gamma-Ray Astronomy and the Next Generation Observatory CTA - KMI - Nagoya Universityrich600338<blockquote class="wp-embedded-content" data-secret="ijqTovvhwL"><a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/845/">Very High Energy Gamma-Ray Astronomy and the Next Generation Observatory CTA</a></blockquote><iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/845/embed/#?secret=ijqTovvhwL" width="600" height="338" title="“Very High Energy Gamma-Ray Astronomy and the Next Generation Observatory CTA” — KMI - Nagoya University" data-secret="ijqTovvhwL" frameborder="0" marginwidth="0" marginheight="0" scrolling="no" class="wp-embedded-content"></iframe><script type="text/javascript">
/* <![CDATA[ */
/*! This file is auto-generated */
!function(d,l){"use strict";l.querySelector&&d.addEventListener&&"undefined"!=typeof URL&&(d.wp=d.wp||{},d.wp.receiveEmbedMessage||(d.wp.receiveEmbedMessage=function(e){var t=e.data;if((t||t.secret||t.message||t.value)&&!/[^a-zA-Z0-9]/.test(t.secret)){for(var s,r,n,a=l.querySelectorAll('iframe[data-secret="'+t.secret+'"]'),o=l.querySelectorAll('blockquote[data-secret="'+t.secret+'"]'),c=new RegExp("^https?:$","i"),i=0;i<o.length;i++)o[i].style.display="none";for(i=0;i<a.length;i++)s=a[i],e.source===s.contentWindow&&(s.removeAttribute("style"),"height"===t.message?(1e3<(r=parseInt(t.value,10))?r=1e3:~~r<200&&(r=200),s.height=r):"link"===t.message&&(r=new URL(s.getAttribute("src")),n=new URL(t.value),c.test(n.protocol))&&n.host===r.host&&l.activeElement===s&&(d.top.location.href=t.value))}},d.addEventListener("message",d.wp.receiveEmbedMessage,!1),l.addEventListener("DOMContentLoaded",function(){for(var e,t,s=l.querySelectorAll("iframe.wp-embedded-content"),r=0;r<s.length;r++)(t=(e=s[r]).getAttribute("data-secret"))||(t=Math.random().toString(36).substring(2,12),e.src+="#?secret="+t,e.setAttribute("data-secret",t)),e.contentWindow.postMessage({message:"ready",secret:t},"*")},!1)))}(window,document);
/* ]]> */
</script>
Very high energy gamma-ray astronomy explores the non-thermal Universe, probing via their gamma ray emission, the populations, acceleration mechanisms and propagation of high energy particles in our Galaxy and in external galaxies. Despite one century of research, many details of cosmic particle accelerators are poorly understood, as is their influence on the evolution of structures in the Universe. The current Imaging Atmospheric Cherenkov Telescope (IACT) instruments, such as the H.E.S.S., MAGIC and VERITAS telescope systems, together with the gamma ray …