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schedule.html
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<!DOCTYPE html>
<html>
<head>
<title>Schedule | Future by the Future</title>
<link rel="stylesheet" type="text/css" href="main.css">
<link rel="icon" href="https://markalab.github.io/future/images/icon.png">
</head>
<body>
<center>
<nav>
<ul>
<li><a href="index.html">WELCOME</a></li>
<li><a href="schedule.html">SCHEDULE</a></li>
<li><a href="location.html">LOCATION</a></li>
<li><a href="code.html">CODE OF CONDUCT</a></li>
</ul>
</nav>
</center>
<p style="font-size:0.5em">Image credit: NSF, LIGO, Sonoma State University, A. Simmonet</p>
<img src="images/GW170817_crop.jpeg" width="100%">
<h2>SCHEDULE</h2>
<br>
<h3>Friday</h3>
<style type="text/css">
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<table class="tg">
<tr>
<th class="tg-11ys">8:50-9:00</th>
<th class="tg-b6pr">Szabi and Zsuzsa Marka</th>
<th class="tg-ohiz">Opening statement</th>
</tr>
<tr>
<td class="tg-11ys">9:00-9:20</td>
<td class="tg-b6pr">Brian Greene</td>
<td class="tg-ohiz">Welcome remark</td>
</tr>
<tr>
<td class="tg-11ys">9:20-9:50</td>
<td class="tg-b6pr">Azadeh Keivani</td>
<td class="tg-11ys">Is multi-messenger astrophysics the best approach to study sources of high-energy neutrinos and ultra-high energy cosmic rays? (<a href="https://drive.google.com/open?id=1DkFC_zJBpIC-DEQcTzl6ZhBlx5G11idq">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">9:50-10:20</td>
<td class="tg-b6pr">Josh Dillon</td>
<td class="tg-11ys">Opening the 21 cm Window on Our Cosmic Dawn (<a href="https://drive.google.com/file/d/1aL6sz6sn_wk8ZE7JVfn6mQIph2oUjI32/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">10:20-10:50</td>
<td class="tg-b6pr">Jasmine Gill</td>
<td class="tg-11ys">From Dreams to Future Discoveries: Advancing Multi-Messenger Core-Collapse Supernova Science (<a href="https://drive.google.com/open?id=127Ha9ezCEi13gMEYgNg-Y_tiXSiQvDrO">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">10:50-11:00</td>
<td class="tg-b6pr"></td>
<td class="tg-ohiz">Coffee break</td>
</tr>
<tr>
<td class="tg-11ys">11:00-11:30</td>
<td class="tg-b6pr">Dario Carbone</td>
<td class="tg-11ys">Identifying EM counterparts to NS-NS mergers: an Optimized Radio Follow-up Strategy (<a href="https://drive.google.com/file/d/1KaEvWbWeoaPKm5FoWLIEascpKaWTPxpy/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">11:30-12:00</td>
<td class="tg-b6pr">Ashley Villar</td>
<td class="tg-11ys">Analyzing Cosmic Messengers with More Data, New Tools & Unified Modeling (<a href="https://drive.google.com/file/d/1GG8u4ebxpAOI0KGJjX6hd92epq4wqae5/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">12:00-12:50</td>
<td class="tg-b6pr">Panel Discussion: Reshmi Mukherjee</td>
<td class="tg-11ys">What is needed? Community for multimessenger science</td>
</tr>
<tr>
<td class="tg-11ys">12:50-1:50</td>
<td class="tg-b6pr"></td>
<td class="tg-ohiz">Lunch provided</td>
</tr>
<tr>
<td class="tg-11ys">1:50-2:20</td>
<td class="tg-b6pr">Katelyn Breivik</td>
<td class="tg-11ys">The stellar graveyard: a multi-messenger, multi-band puzzle (<a href="https://drive.google.com/file/d/1RiMwcSXNj3p5gkJE2gesH2VY1N5X71FI/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">2:20-2:50</td>
<td class="tg-b6pr">Katerina Chatziioannou</td>
<td class="tg-11ys">Studying the neutron star equation of state with multi messenger observations (<a href="https://drive.google.com/file/d/18G2VctYXiFtj_TjRGsbyXdxYG1tcAhcH/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">2:50-3:20</td>
<td class="tg-b6pr">Imre Bartos</td>
<td class="tg-11ys">The Age of Abundance: How Frequent Discoveries will Transform Multimessenger Astrophysics (<a href="https://drive.google.com/file/d/1x4kEbL1HId3YJ5mHy_9YGFH_1Z6czbRi/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">3:20-3:30</td>
<td class="tg-b6pr"></td>
<td class="tg-ohiz">Coffee break</td>
</tr>
<tr>
<td class="tg-11ys">3:30-4:00</td>
<td class="tg-b6pr">Leo Singer</td>
<td class="tg-11ys">Black and Gold: The Future of Gravitational Wave Mulit-Messenger Astronomy (<a href="https://drive.google.com/file/d/1BJRlIbUG1Tbzn2EtQAlHWuhHWHpOva_H/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">4:00-4:30</td>
<td class="tg-b6pr">Michael Coughlin</td>
<td class="tg-11ys">Using EMCCDs for high-cadence observations of objects variable on short time-scales (<a href="https://drive.google.com/file/d/1ed3Q6crbZrkDUvU72IuHSOB5WODhFo2T/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">4:30-5:30</td>
<td class="tg-b6pr">Evan Goetz</td>
<td class="tg-11ys">Searching for continuous gravitational waves with advanced detectors and beyond (<a href="https://drive.google.com/open?id=1MHpMqcJNxnlXVZf2UsXFClqLGuU4Xou3">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">5:00-5:40</td>
<td class="tg-b6pr">Panel Discussion: Yuri Levin</td>
<td class="tg-11ys">What is needed? Instruments</td>
</tr>
<tr>
<td class="tg-11ys">5:40-7:00</td>
<td class="tg-b6pr"></td>
<td class="tg-ohiz">Wine and cheese</td>
</tr>
</table>
<br><br>
<h3>Saturday</h3>
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<table class="tg">
<tr>
<td class="tg-11ys">8:30-9:00</td>
<td class="tg-b6pr">Evan Hall</td>
<td class="tg-11ys">Cosmic Explorer and the Future of Ground-Based Gravitational-Wave Detection (<a href="https://drive.google.com/open?id=1720OxBDTQxsXOILYkyBBnnV8oXlr99jA">slides</a>)</td>
</tr>
<tr>
<th class="tg-11ys">9:00-9:30</th>
<th class="tg-b6pr">Shuo Zhang</th>
<th class="tg-11ys">High-energy X-ray View of the Central 10 pc of the Galaxy (<a href="https://drive.google.com/open?id=1hqdmE2NI7eP8Ao49yy9-r-uyQ3NyeCrJ">slides</a>)</th>
</tr>
<tr>
<td class="tg-11ys">9:30-10:00</td>
<td class="tg-b6pr">Marcos Santander</td>
<td class="tg-11ys">The future of high-energy neutrino astrophysics (<a href="https://drive.google.com/file/d/1FBLG-7p8YPA1A6Ic0nZRXU05mYiJv6xV/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">10:00-10:30</td>
<td class="tg-b6pr">Hsin-Yu Chen</td>
<td class="tg-11ys">The bright and loud future of gravitational-wave multi-messenger astrophysics and cosmology (<a href="https://drive.google.com/open?id=15ts7Hb1D4U7OKbN-SdGwOI3S9FqgPQqR">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">10:30-10:50</td>
<td class="tg-b6pr"></td>
<td class="tg-ohiz">Coffee break</td>
</tr>
<tr>
<td class="tg-11ys">10:50-11:20</td>
<td class="tg-b6pr">Carl Johan Haster</td>
<td class="tg-11ys">The future of Gravitational Wave inference - problems to solve over the next few years (<a href="https://drive.google.com/file/d/1Sw5pxBkCw5qg3mxP0gWqQ3wl9gW1lZ_F/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">11:20-11:50</td>
<td class="tg-b6pr">Marcelle Soares Santos</td>
<td class="tg-11ys">Precision cosmology with standard sirens and traditional probes in DES and LSST DESC (<a href="https://drive.google.com/open?id=1A6qKOobeDrLloxJ9MYtbYn3UBWOFmFTd">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">11:50-12:20</td>
<td class="tg-b6pr">Ali Kheirandish</td>
<td class="tg-11ys">Multimessenger observations and the path to uncovering cosmic ray sources: strategies for identifying flaring, obscured, and efficient sources (<a href="https://drive.google.com/file/d/1JH9EdZKqRAuA9Cv9_ug6yKDaw7XHCJGC/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">12:20-12:35</td>
<td class="tg-b6pr">Jamie Rollins</td>
<td class="tg-11ys">Binary Black Holes from LIGO/Virgo's First and Second Observing Runs (<a href="https://drive.google.com/file/d/1iOSUaYa3hQu5ho4qbHz5p6v6KaouJSoS/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">12:35-1:00</td>
<td class="tg-b6pr">Panel Discussion: Brian Metzger</td>
<td class="tg-11ys">What is needed? Theory and Modelling</td>
</tr>
<tr>
<td class="tg-11ys">1:00-1:40</td>
<td class="tg-b6pr"></td>
<td class="tg-ohiz">Lunch</td>
</tr>
<tr>
<td class="tg-11ys">1:40-2:10</td>
<td class="tg-b6pr">Phil Cowperthwaite</td>
<td class="tg-11ys">Chasing EM Counterparts with Next-Generation Facilities (<a href="https://drive.google.com/file/d/1Y-VGBSwo4a85dmwJd-uGqvfNqVOQ4_2b/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">2:10-2:40</td>
<td class="tg-b6pr">Anamaria Effler</td>
<td class="tg-11ys">Some LIGO Instrumental Lessons for the Future (<a href="https://drive.google.com/file/d/1IcJAbWEbirZyP19YnDUvNZFO2eri6lZB/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">2:40-3:10</td>
<td class="tg-b6pr">Ke Fang</td>
<td class="tg-11ys">High-energy Astroparticle Counterparts to Neutron Star Mergers (<a href="https://drive.google.com/file/d/1_5asG8Q3adCVa6NWvB8v8xD-7H7cFJCa/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">3:10-3:40</td>
<td class="tg-b6pr">Peter Veres</td>
<td class="tg-11ys">Role of Gamma-ray Bursts in the Future of Multimessenger Astrophysics (<a href="https://drive.google.com/file/d/16Fqo6cRrT-iS_27FE10CQvm4cH7K7jTm/view?usp=sharing">slides</a>)</td>
</tr>
<tr>
<td class="tg-11ys">3:40-4:20</td>
<td class="tg-b6pr">Panel Discussion: Szabi Marka</td>
<td class="tg-11ys">Predictions for the Future</td>
</tr>
<tr>
<td class="tg-11ys">4:20-4:30</td>
<td class="tg-b6pr">Zsuzsa Marka</td>
<td class="tg-ohiz">Closing remarks</td>
</tr>
</table>