1.0KMI - Nagoya Universityhttps://www.kmi.nagoya-u.ac.jp/engrich600338<blockquote class="wp-embedded-content" data-secret="Wl5dtYlfBQ"><a href="https://www.kmi.nagoya-u.ac.jp/eng/seminar/985/">Weak Lensing Study of Subhalos in very nearby Galaxy Cluster</a></blockquote><iframe sandbox="allow-scripts" security="restricted" src="https://www.kmi.nagoya-u.ac.jp/eng/seminar/985/embed/#?secret=Wl5dtYlfBQ" width="600" height="338" title="“Weak Lensing Study of Subhalos in very nearby Galaxy Cluster” — KMI - Nagoya University" data-secret="Wl5dtYlfBQ" 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> The structure we observe today is believed to be the result of hierarchical clustering of smaller CDM halos through the expansion of the universe. Although the scenario has been very successful in explaining the observed large scale structure of the universe, there is almost no observational evidence to test it on the Mpc scale where mass assembly history becomes important. This unclear situation will resolved by the direct observation of cluster subhalo properties such as mass function and spatial distribution …