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X-WR-CALNAME;VALUE=TEXT:ITC Luncheon
PRODID:-//Harvard events data//EN
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UID:event_1441049_0
SUMMARY:ITC Luncheon
DESCRIPTION:<p style="margin-bottom:9.4pt">	<span style="background:white"><span style="line-height:normal"><span><span style='NewRoman",serif'><span style="color:#444444">Sean Ressler (CITA), “</span></span></span><span><span style="background:white"><span style='NewRoman",serif'><span style="color:black">Kelvin-Helmholtz Interactions in the Galactic Center's Circumnuclear Disk.</span></span></span></span>”</span></span></p><p style="margin-bottom:9.4pt">	<span style="background:white"><span style="line-height:normal"><span><span style="background:white"><span style='NewRoman",serif'><span style="color:#222222">Jonathan Morag (</span></span></span></span><span><span style='NewRoman",serif'>Weizmann Institute of Science<span style="background:white"><span style="color:#222222">), “An analytic Model for Shock Cooling Emission in Core-Collapse Supernovae Calibrated to Numeric Calculations”</span></span></span></span></span></span></p><p style="margin-bottom:9.4pt">	<span style="background:white"><span style="line-height:normal"><span><span style='NewRoman",serif'><span style="color:#444444">Zach Murray (Harvard), </span></span></span><span><span style="background:white"><span style='NewRoman",serif'><span style="color:black">"Using Machine Learning to Predict Main-Belt Asteroid Albedos"</span></span></span></span></span></span></p><p style="margin-bottom:9.4pt">	<span style="background:white"><span style="line-height:normal"><span><span style='NewRoman",serif'><span style="color:#444444">Fabio Pacucci (CfA), “</span></span></span><span><span style="background:white"><span style='NewRoman",serif'><span style="color:black">‘Tis the Season to Detect a SgrA*-like SMBH in a Milky Way Satellite”</span></span></span></span></span></span></p>
LOCATION:Phillips
STATUS:CONFIRMED
DTSTART:20221201T173000Z
DTEND:20221201T183000Z
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