<html><head><meta http-equiv="Content-Type" content="text/html charset=us-ascii"></head><body style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space;" class=""><div class="">TODAY!!!</div><br class=""><div><blockquote type="cite" class=""><div class="">On 22 Oct 2018, at 17:12, Francesco Taddia <<a href="mailto:ftadd@astro.su.se" class="">ftadd@astro.su.se</a>> wrote:</div><br class="Apple-interchange-newline"><div class="">
<meta http-equiv="Content-Type" content="text/html; charset=us-ascii" class=""><div style="word-wrap: break-word; -webkit-nbsp-mode: space; -webkit-line-break: after-white-space;" class="">Dear all,<div class=""><br class=""></div><div class="">on Thursday (Oct 25, 13:00-14:00, KTH meeting room on the 5th floor) we will have our next EO meeting,</div><div class="">where Francesca Capel will give the following talk:</div><div class=""><br class=""></div><div class=""><i class="">Title: A hierarchical model for the sources of ultra-high energy cosmic rays (UHECR)<br class=""><br class="">Abstract:<br class="">The study of UHECR is challenged by both the rarity of events and the difficulty in modelling their production, propagation and detection. I will present a Bayesian hierarchical model which enables a joint fit of the UHECR energy spectrum and arrival directions with a physical model of UHECR phenomenology. In this way, possible associations with candidate source catalogs can be assessed in a physically and statistically principled manner. Results from the application of the model to data from the Pierre Auger Observatory will also be shown.</i></div><div class=""><i class=""><br class=""></i></div><div class=""><i class=""><br class=""></i></div><div class="">cheers</div><div class=""><br class=""></div><div class="">/Francesco</div></div><br class="">-------------------------------------------------<br class=""><a href="mailto:okc-wp4@albanova.se" class="">okc-wp4@albanova.se</a> mailing list</div></blockquote></div><br class=""></body></html>