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Reminded of our EO meeting today at 13:00.
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<div id="divRplyFwdMsg" dir="ltr"><font face="Calibri, sans-serif" color="#000000" style="font-size:11pt"><b>From:</b> Okc-wp4-at-fysik.su.se <okc-wp4-at-fysik.su.se-bounces@lists.su.se> on behalf of Andre Schneider <andre.schneider@astro.su.se><br>
<b>Sent:</b> Tuesday, December 4, 2018 10:15 AM<br>
<b>To:</b> okc-wp4-at-fysik.su.se@lists.su.se<br>
<b>Subject:</b> [Okc-wp4] EO meeting on Dec 6</font>
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<font size="2" style="font-family:"Helvetica Neue",serif,EmojiFont"><span style="font-size:14px"><span style="color:rgb(33,33,33); font-family:wf_segoe-ui_normal,"Segoe UI","Segoe WP",Tahoma,Arial,sans-serif,serif,EmojiFont">Dear all,</span>
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our next speaker at the EO meeting (Dec 6, 13:00, @KTH meeting room on the 5th floor), will be <b>Ragnhild Lunnan</b>. Below is the info on her talk.</div>
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<font size="2" style="font-family:"Helvetica Neue",serif,EmojiFont"><span style="font-size:14px">Rapidly Evolving Transients in the ZTF Era</span></font></div>
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<font size="2" style="font-family:"Helvetica Neue",serif,EmojiFont"><span style="font-size:14px">Large-scale untargeted optical surveys are discovering many new types of transient phenomena beyond the standard Type Ia and core-collapse supernova paradigm. One
relatively unexplored part of parameter space is transients with shorter timescales (~days rather than ~weeks), as traditional supernova searches were not particularly sensitive to such events. Analysis from the Pan-STARRS Medium Deep Survey suggests such
transients constitute as much as 4-7% of the core-collapse supernova rate, however. In this talk, I will review previous work on rapidly evolving transients as well as discuss some recent, interesting events from iPTF and ZTF. </span></font></div>
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