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<!doctype html>
<html lang="en">
<head>
<!--====== Required meta tags ======-->
<meta charset="utf-8">
<meta http-equiv="x-ua-compatible" content="ie=edge">
<meta name="description" content="">
<meta name="viewport" content="width=device-width, initial-scale=1, shrink-to-fit=no">
<!--====== Title ======-->
<title>TARDIS-Con 2023</title>
<!--====== Favicon Icon ======-->
<link rel="shortcut icon" href="assets/images/tardis-logo-2.svg" type="image/png">
<!--====== Bootstrap css ======-->
<link rel="stylesheet" href="assets/css/bootstrap.min.css">
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<div data-countdown="2023-07-10 00:00:00"></div>
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<h2 class="header-title">TARDIS-Con 2023</h2>
<h4 class="text-white">
10July
- 21July
2023
</h4>
<h4 class="text-white">at Michigan State University, East Lansing, USA</h4>
<div class="col-xs-12" style="height:50px;"></div>
<h3 class="text-white">TARDIS-Con 2023 is an unconference-style conference
focused on open science code and astrophysics. We believe that collaboration and
open-source development are key to advancing the field of astrophysics and we are
excited to bring together researchers and students from many disciplines such as
astrophysics, software engineering, machine learning, and natural language processing.
</h3>
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<div class="section-title text-center pb-20">
<h2 class="title">Why You Should Join?</h2>
<p class="text">We will be providing a platform for participants to come together and share
their knowledge, expertise, and ideas. Our aim is to create an open and inclusive space
where attendees can work collaboratively on scientific code, tools, and techniques.</p>
</div> <!-- section title -->
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data-wow-delay="0s">
<div class="features-icon">
<i class="lni-microphone"></i>
<span>01</span>
</div>
<div class="features-content">
<h4 class="features-title"><a href="#">TARDIS</a></h4>
<p class="text">One of the major projects we will be working on is improving the TARDIS code
for simulating supernovae. This will involve developing new visualization tools to help
researchers better understand the complex radiative transfer processes involved in
supernovae. Additionally, we will be exploring new microphysics models to improve the
accuracy of simulations, and working to optimize the code's performance, including the
possibility of adding GPU acceleration.</p>
</div>
</div> <!-- single features -->
</div>
<div class="col-lg-4 col-md-6 col-sm-8">
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data-wow-delay="0.5s">
<div class="features-icon">
<i class="lni-users"></i>
<span>02</span>
</div>
<div class="features-content">
<h4 class="features-title"><a href="#">STARDIS</a></h4>
<p class="text">We will also be focusing on the STARDIS code, a radiative transfer code used
for modeling stars. Our goal is to improve its capabilities by adding non-local
thermodynamic equilibrium (NLTE) modeling, which will allow for more accurate
simulations of a wider range of stars. We will also be exploring new microphysics models
to improve the accuracy of STARDIS simulations and working to optimize the code's
performance.</p>
</div>
</div> <!-- single features -->
</div>
<div class="col-lg-4 col-md-6 col-sm-8">
<div class="single-features text-center mt-30 wow fadeIn" data-wow-duration="1s"
data-wow-delay="1s">
<div class="features-icon">
<i class="lni-bullhorn"></i>
<span>03</span>
</div>
<div class="features-content">
<h4 class="features-title"><a href="#">Carsus</a></h4>
<p class="text">At TARDIS-Con 2023, we will also be focusing on the Carsus
project, an atomic structure database that provides input to radiative transfer codes.
Our goals include expanding its capabilities by including additional databases, such as
the Vienna Atomic Line Database (VALD), and exploring how different databases impact the
spectra generated. We will also be working on visualizations, such as Grotrian diagrams,
to better understand the complex atomic processes involved in astrophysical simulations.
By improving the accuracy and reliability of radiative transfer simulations through the
Carsus project, we hope to advance our understanding of the universe.</p>
</div>
</div> <!-- single features -->
</div>
<div class="col-lg-4 col-md-6 col-sm-8">
<div class="single-features text-center mt-30 wow fadeIn" data-wow-duration="1s"
data-wow-delay="0.5s">
<div class="features-icon">
<i class="lni-heart"></i>
<span>04</span>
</div>
<div class="features-content">
<h4 class="features-title"><a href="#">Machine-learning emulators</a></h4>
<p class="text">We will also be focusing on our surrogate models and emulators, which are
critical to our work on radiative transfer simulations. Our research will center around
finding new combinations with uncertainty quantification techniques, and exploring how
nested sampling can leverage the gradients provided by emulators. We will also be
developing active learning techniques and working to build high-dimensional emulators
for our radiative transfer codes, which will allow us to generate accurate simulations
more efficiently. By advancing our understanding of surrogate models and emulators, we
hope to improve the accuracy and efficiency of radiative transfer simulations, and
ultimately gain new insights into the universe.</p>
</div>
</div> <!-- single features -->
</div>
<div class="col-lg-4 col-md-6 col-sm-8">
<div class="single-features text-center mt-30 wow fadeIn" data-wow-duration="1s"
data-wow-delay="1s">
<div class="features-icon">
<i class="lni-cup"></i>
<span>05</span>
</div>
<div class="features-content">
<h4 class="features-title"><a href="#">Computational Metascience</a></h4>
<p class="text">Collect data and build a prototype model to analyze the overall climate of
the current academic research system. Utilize data from various sources to examine key
metrics such as peer review rates, publishing rates, funding rates, and growth of the
global research community. Explore how these metrics have evolved over time and identify
any trends or patterns that may indicate systemic issues or opportunities for
improvement. Analyze the impact of factors such as funding models, publication
standards, and work culture (e.g. tension between work-life balance and ever growing
list of requirements for “success” of a researcher) on the climate of the academic
research system. </p>
</div>
</div> <!-- single features -->
</div>
<div class="col-lg-4 col-md-6 col-sm-8">
<div class="single-features text-center mt-30 wow fadeIn" data-wow-duration="1s"
data-wow-delay="1.5s">
<div class="features-icon">
<i class="lni-gallery"></i>
<span>06</span>
</div>
<div class="features-content">
<h4 class="features-title"><a href="#">A global census of astronomers</a></h4>
<p class="text">Validate state-of-the-art author name disambiguation algorithms using
scientific publication metadata and a validation set of uniquely identified researchers
from ORCiD. Explore and evaluate various author name disambiguation algorithms and
extend beyond these approaches by leveraging computational tools such as natural
language processing to create unique author profiles based on their abstracts. Develop a
validation framework that incorporates both quantitative and qualitative metrics to
assess the accuracy of the disambiguation algorithms. </p>
</div>
</div> <!-- single features -->
</div>
</div> <!-- row -->
</div> <!-- container -->
<div class="section-title text-center pb-20">
<p class="text">In addition to these projects, we will have many other opportunities for participants to
work collaboratively on open science code in astrophysics. These include projects focused on machine
learning, natural language processing, and other cutting-edge techniques. By working together and
sharing our knowledge and expertise, we hope to drive forward the development of open science code and
advance our understanding of the universe.</p>
</div> <!-- section title -->
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