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DTSTAMP:20251208T081320Z
SUMMARY:Astrophysical Sciences and Technology Colloquium: The JWST
 Revolution in High-Redshift Supernova Discovery
DTSTART:20251208T210000Z
DTEND:20251208T220000Z
LOCATION:Chester F. Carlson Center for Imaging Science: 1125 or via Zoom
DESCRIPTION:<p class="default-image-margins"><span
 style="font-size:12pt"><span style="background:white"><span
 style="font-family:&quot;Times New Roman&quot;,serif"><b><span
 style="border:none windowtext 1.0pt; font-size:11.0pt; padding:0in"><span
 style="font-family:&quot;Arial&quot;,sans-serif"><span
 style="color:#424242">AST
 Colloquium</span></span></span></b></span></span></span><br>
 <span style="font-size:11pt"><span
 style="font-variant-ligatures:normal"><span
 style="text-decoration-thickness:initial"><span
 style="text-decoration-style:initial"><span
 style="text-decoration-color:initial"><span
 style="font-family:Calibri,sans-serif"><b><span
 style="font-size:16.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif">The JWST Revolution in
 High-Redshift Supernova
 Discovery</span></span></b></span></span></span></span></span></span></p>
 <p class="default-image-margins"><span style="font-size:11pt"><span
 style="font-family:Calibri,sans-serif"><b><span
 style="font-size:12.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif"><a
 href="https://rit.zoom.us/meeting/register/VHuzh3muQ-aUAKrT2v1v8g"
 style="color:#467886; text-decoration:underline">Zoom Link
 here</a></span></span></b></span></span><br>
 <span style="font-size:11pt"><span
 style="font-family:Calibri,sans-serif"><b><span
 style="font-family:&quot;Arial&quot;,sans-serif"><span
 style="color:#ed7d31"><br>
 Dr. Justin Pierel</span></span></b></span></span><br>
 <span style="font-size:11pt"><span style="tab-stops:199.3pt"><span
 style="font-family:Calibri,sans-serif"><span
 style="font-family:&quot;Arial&quot;,sans-serif">Postdoctoral
 Researcher</span></span></span></span><br>
 <span style="font-size:11pt"><span style="tab-stops:199.3pt"><span
 style="font-family:Calibri,sans-serif"><span
 style="font-family:&quot;Arial&quot;,sans-serif">Space Telescope Science
 Institute</span></span></span></span><br>
 <span style="font-size:11pt"><span
 style="font-family:Calibri,sans-serif"><i><span
 style="font-size:12.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif"><br>
 Abstract</span></span></i><span style="font-size:12.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif">:</span></span></span></
 span><br>
 <span style="font-size:11pt"><span
 style="font-family:Calibri,sans-serif"> <span
 style="font-family:&quot;Arial&quot;,sans-serif">The high-redshift
 transient universe has been an unexplored field of astrophysics due to
 the vast amount of resources required to discover supernovae (SNe) at
 z&amp;gt;1. Even with the Hubble Space Telescope, discoveries of the most
 distant stellar explosions have been restricted to z~2, with critical
 spectroscopy limited to z~1.5. With the launch of the James Webb Space
 Telescope (JWST), we have entered a new era of high-redshift SN discovery
 and understanding. JWST has significantly expanded our view of the
 transient universe, including hundreds of SNe and dozens of rest-frame
 UV-IR spectra for SNe reaching z=5.13. The JWST SN sample with both
 imaging and spectroscopy now includes the most distant Type Ia SNe (used
 for cosmological measurements) yet discovered, multiple strongly lensed
 SNe, and a wide variety of core-collapse SN sub-types from a previously
 unexplored phase of the transient universe. I will summarize the range of
 discoveries made in the first few years of JWST observations, the
 constraints gleaned from these exciting new objects, and our ongoing
 efforts to build the first statistical samples of high-redshift SNe.
 Looking ahead, these SNe give us a glimpse at what we can expect from the
 upcoming Nancy Grace Roman Space Telescope, which will revolutionize the
 discovery of distant stellar explosions.</span></span></span></p>
 <p class="default-image-margins"><span style="font-size:11pt"><span
 style="font-family:Calibri,sans-serif"><i><span
 style="font-size:12.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif">Bio:
 </span></span></i><span style="font-size:12.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif"></span></span></span></s
 pan><br>
 <span style="font-size:12pt"><span style="background:white"><span
 style="font-family:&quot;Times New Roman&quot;,serif"><span
 style="font-family:&quot;Arial&quot;,sans-serif"><span
 style="color:black">Justin graduated from Bowdoin College with a
 bachelor’s degree in mathematics and spent two years at NASA Goddard
 Space Flight Center as a member of the Cassini team. He received his
 master’s and PhD in Physics from the University of South Carolina,
 where he was awarded South Carolina Space Grant Consortium and FINESST
 Fellowships. Justin moved to the Space Telescope Science Institute in
 2021 as a postdoc in the “Transient Science at Space Telescope”
 group, where he is now a NASA Einstein Fellow focused on time-domain
 science with the James Webb Space Telescope.</span></span><span
 style="font-family:&quot;Arial&quot;,sans-serif"></span></span></span></s
 pan></p>
 <p class="default-image-margins"><span style="font-size:12pt"><span
 style="background:white"><span style="font-family:&quot;Times New
 Roman&quot;,serif"><i><span style="border:none windowtext 1.0pt;
 font-size:11.0pt; padding:0in"><span
 style="font-family:&quot;Arial&quot;,sans-serif"><span
 style="color:black">Intended Audience:</span></span></span></i><span
 style="font-size:11.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif"></span></span></span></s
 pan></span><br>
 <span style="font-size:12pt"><span style="background:white"><span
 style="font-variant-ligatures:normal"><span
 style="text-decoration-thickness:initial"><span
 style="text-decoration-style:initial"><span
 style="text-decoration-color:initial"><span
 style="font-family:&quot;Times New Roman&quot;,serif"><span
 style="border:none windowtext 1.0pt; font-size:11.0pt; padding:0in"><span
 style="font-family:&quot;Arial&quot;,sans-serif"><span
 style="color:black">Beginners, undergraduates, graduates. Those with
 interest in the topic.</span></span></span><span
 style="font-size:11.0pt"><span
 style="font-family:&quot;Arial&quot;,sans-serif"></span></span></span></s
 pan></span></span></span></span></span></p>
 <p><span style="font-size:11pt"><span
 style="font-variant-ligatures:normal"><span
 style="text-decoration-thickness:initial"><span
 style="text-decoration-style:initial"><span
 style="text-decoration-color:initial"><span
 style="font-family:Calibri,sans-serif"><span
 style="font-family:&quot;Arial&quot;,sans-serif"></span></span></span></s
 pan></span></span></span></p>
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