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<div id="magicdomid345" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;">Dear all,</span></div>
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<div id="magicdomid347" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;">our next Extreme Object meeting will be </span><span class="b" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;"><b class="">next
Thursday, 27th of October, at 13:15 (CEST).</b></span><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;"> The speaker is </span><span class="b" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;"><b class="">Nora Valtonen-Mattila</b></span><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;"> a
PhD from Uppsala Unversity. She will talk about high energy neutrinos from supernova. </span></div>
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<div id="magicdomid349" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;">The meeting will be held in lecture room FC61 at the Astronomy department on the 6th floor in Albanova building.
Looking forward to see most of you there. </span></div>
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<div id="magicdomid351" class="ace-line" style="padding-right: 1px;"><span class="b" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;"><b class="">Title: </b></span></div>
<div id="magicdomid352" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;">Observing core-collapse supernovae through neutrinos: from MeV to TeV</span></div>
<div id="magicdomid353" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;"> </span></div>
<div id="magicdomid354" class="ace-line" style="padding-right: 1px;"><span class="b" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;"><b class="">Abstract:</b></span></div>
<div id="magicdomid355" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;">Core-collapse supernovae are one of the most energetic events in the cosmos, releasing a tremendous amount of energy
in the form of low-energy O(10 MeV) neutrinos before the shock breakout. Some models have also predicted post-explosion emission of high-energy neutrinos O(>TeV) through particle acceleration processes. In this talk, I will explore how we can use both energy
ranges to observe supernovae and, in particular, how we can extend the detection horizon of IceCube by using high-energy neutrinos.</span></div>
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<div id="magicdomid358" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;">Kind regards,</span></div>
<div id="magicdomid359" class="ace-line" style="padding-right: 1px;"><span class="" style="cursor: auto; padding-top: 0px; padding-bottom: 1px;">Ana Sagués Carracedo & Haakon Andresen</span></div>
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