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stephenpardystephenpardy
committedMar 23, 2018
major reorg
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‎CV/index.html

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<h2 id="teaching-experience">TEACHING EXPERIENCE</h2>
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<div class="col-xs-6 col-md-9">
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<p><span><em>Teaching Assistant</em></span> Spring 2014, Fall 2016<br />University of Wisconsin - Madison</p>
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<p><span><em>Teaching Assistant</em></span> Spring 2014, Fall 2016, Fall 2017<br />University of Wisconsin - Madison</p>
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<ul>
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<li><p>Designed course material and taught discussion sections</p></li>
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</ul>
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<div class="col-xs-12 col-md-3">
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<h2 id="publications">PUBLICATIONS</h2>
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</div>
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<a href='https://scholar.google.com/citations?user=LbZ6-RcAAAAJ'>Google Scholar</a>
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<a href='https://ui.adsabs.harvard.edu/#search/q=%5EPardy%2C%20S.&sort=date%20desc%2C%20bibcode%20desc'>ADS</a>
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<div class="col-xs-6 col-md-9">
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<p>
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<b>Pardy, S. A.</b>; D'Onghia, E.; Fox, A. accepted -- <small><a href="http://adsabs.harvard.edu/cgi-bin/bib_query?arXiv:1802.01600">Models of Tidally Induced Gas Filaments in the Magellanic Stream</a></small>
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<br>
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</p>
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<p>
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<span class="expanded">Bridge, J.~S.; Hayes, M.; Melinder, J.; Östlin, G.; Gronwall, C.; Ciardullo, R.; Atek, H.; Cannon, J. M.; Gronke, M.; Guaita, L.; Hagen, A.; Herenz, E. C.; Kunth, D.; Laursen, P.; Mas-Hesse, J. M.; <b>Pardy, S. A.</b>;</span>
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</div>
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<h2 id="Outreach">Outreach</h2>
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<h2 id="Outreach">Service and Outreach</h2>
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</div>
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<div class="col-xs-6 col-md-9">
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<p><h3><em>Outreach:</em></h3></p>
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<ul>
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<li><p> Referee - Monthly Notices of the Royal Astronomical Society</p></li>
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<li><p> Webmaster and LOC member for `The Role of Gas in Galaxies' - international conference with 130+ attendees.</p></li>
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<li><p> Televised lecture at UW-Madison Space Place </p></li>
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<li><p> Webmaster and LOC member for <a href='http://gasingalaxiesconference.com/'>The Role of Gas in Galaxies</a> - international conference with 130+ attendees.</p></li>
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<li><p> <a href="https://wpt.org/University-Place/how-build-galaxy-three-easy-steps">Televised lecture</a> at UW-Madison Space Place </p></li>
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<li><p> Department service: Graduate student Chair - 2016, Prospective graduate student organizer - 2014, 2015, 2017</p></li>
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<li><p> Public talks and observing at state parks through the `Universe in the Park' program </p></li>
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<li><p> Telescope operator for public observing at Washburn Observatory and Macalester College</p></li>
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<li><p> Public talks and observing at state parks through the <a href="http://www.astro.wisc.edu/the-public/universe-in-the-park/">Universe in the Park</a> program </p></li>
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<li><p> Telescope operator for public observing at <a href="http://www.astro.wisc.edu/the-public/public-observing-at-washburn/?Washburn/">Washburn Observatory</a> and Macalester College</p></li>
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</ul>
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<p><h3><em>Mentor:</em></h3></p>
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<p><h3><em>Students Mentored:</em></h3></p>
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<li><p>Stellar evolution workshop at Wisconsin state Science Olympiad competition winter 2014.</p></li>
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<li><p>Ramsey Junior High School Science Fair 2013.</p></li>
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<li><p> William Tyndall - 2014 - 2016</p></li>
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<li><p> Boquan Chen - 2014 - present </p></li>
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<li><p>William Tyndall - 2014 - 2016</p></li>
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<li><p>Boquan Chen - 2014 - present</p></li>
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</ul>
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<p>Hosted public observing nights and was a founding member of Physics Club at Macalester College.</p>
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‎_config.yml

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name: Stephen Pardy
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markdown: kramdown
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collections:
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visualizations:
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output: true
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permalink: /visualizations/:path/

‎_includes/foot.html

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<footer>
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<div class="container">
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<div class="row">
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<p>email: spardy [at] astro.wisc.edu</p>
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</div>
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<div class="col-sm-1">
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<p><a href="https://github.com/stephenpardy"><img src="/images/GitHub-Mark-64px.png" alt="Github"></a>
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</div>
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<div class="col-sm-1">
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<a href="http://www.researchgate.net/profile/Stephen_Pardy"><img src="/images/researchgate2.svg" height=64px width=64px alt="Research Gate"></img></a></p>
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<div class="col-sm-1">
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<a href="https://www.linkedin.com/in/stephen-pardy-599b7b98"><img src="/images/In-Black-66px-TM.png" height=66px width=78px alt='linkedin'></img></a></p>
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</div>
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</footer>
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<script src="https://ajax.googleapis.com/ajax/libs/jquery/1.11.1/jquery.min.js"></script>
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<script src="/bootstrap-3.2.0-dist/js/bootstrap.min.js"></script>
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<script>
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$(document).ready(function() {
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</body>
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</html>

‎_includes/head.html

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<head>
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<title>{{ page.title }}</title>
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<link rel="icon" type="image/png" href="/resources/favicon2.ico">
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<link href="/bootstrap-3.2.0-dist/css/bootstrap.min.css" rel="stylesheet">
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<link rel="stylesheet" type="text/css" href="/css/main.css">
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</head>
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<body>
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<div class="navbar navbar-default navbar-fixed-top" role="navigation">
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<div class="container">
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<button type="button" class="navbar-toggle collapsed" data-toggle="collapse" data-target=".navbar-collapse">
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<span class="sr-only">Toggle navigation</span>
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<span class="icon-bar"></span>
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<span class="icon-bar"></span>
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<span class="icon-bar"></span>
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</button>
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<a class="navbar-brand" href="/">Home</a>
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</div>
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<div class="collapse navbar-collapse">
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<ul class="nav navbar-nav">
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<li><a href="/research">Research</a></li>
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<li><a href="/CV">CV</a></li>
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<li><a href="/blog">Blog</a></li>
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<li class="dropdown">
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<a href="#" class="dropdown-toggle" data-toggle="dropdown" role="button" aria-haspopup="true" aria-expanded="false">Projects <span class="caret"></span></a>
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<ul class="dropdown-menu">
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<li><a href="/projects/horoscope.html">Horoscope</a></li>
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<li><a href="/projects/boxplot.html">Boxplot</a></li>
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<li><a href="/projects/HST_Mast_ngrams.html">HSTgrams</a></li>
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‎_layouts/default.html

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<!DOCTYPE html>
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<html>
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<head>
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<title>{{ page.title }}</title>
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<link rel="icon" type="image/png" href="/resources/favicon2.ico">
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<link href="/bootstrap-3.2.0-dist/css/bootstrap.min.css" rel="stylesheet">
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<link rel="stylesheet" type="text/css" href="/css/main.css">
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<div class="navbar navbar-default navbar-fixed-top" role="navigation">
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<a class="navbar-brand" href="/">Home</a>
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<ul class="nav navbar-nav">
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<li><a href="/research">Research</a></li>
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<li><a href="/CV">CV</a></li>
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<li><a href="/visualization">Scientific Visualizations</a></li>
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<li><a href="/blog">Blog</a></li>
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<li class="dropdown">
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<a href="#" class="dropdown-toggle" data-toggle="dropdown" role="button" aria-haspopup="true" aria-expanded="false">Projects <span class="caret"></span></a>
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<ul class="dropdown-menu">
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<li><a href="/projects/horoscope.html">Horoscope</a></li>
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<li><a href="/projects/boxplot.html">Boxplot</a></li>
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<li><a href="/projects/HST_Mast_ngrams.html">HSTgrams</a></li>
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</ul>
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</ul>
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</div><!--/.nav-collapse -->
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</div>
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</div>
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{% include head.html %}
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<div class="row bottom-buffer"></div>
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</div><!-- /.container -->
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<p>email: spardy [at] astro.wisc.edu</p>
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</div>
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<div class="col-sm-1">
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<p><a href="https://github.com/stephenpardy"><img src="/images/GitHub-Mark-64px.png" alt="Github"></a>
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</div>
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<div class="col-sm-1">
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<a href="http://www.researchgate.net/profile/Stephen_Pardy"><img src="/images/researchgate2.svg" height=64px width=64px></img></a></p>
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<script src="https://ajax.googleapis.com/ajax/libs/jquery/1.11.1/jquery.min.js"></script>
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<script src="/bootstrap-3.2.0-dist/js/bootstrap.min.js"></script>
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<script>
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$(document).ready(function() {
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$(".expanded").hide();
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</body>
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</html>
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{% include foot.html %}

‎_layouts/front.html

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<!DOCTYPE html>
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<html>
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{% include head.html %}
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<div class="container">
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<div class="row">
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<div class="col-10">
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{{ content }}
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</div>
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</div>
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<div class="row bottom-buffer"></div>
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</div><!-- /.container -->
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<script src="https://ajax.googleapis.com/ajax/libs/jquery/1.11.1/jquery.min.js"></script>
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<script src="/bootstrap-3.2.0-dist/js/bootstrap.min.js"></script>
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<script>
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$(document).ready(function() {
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</script>
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</body>
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</html>

‎css/main.css

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}
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div .aboutcontainer {
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margin-top: 20px;
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div .aboutcol {
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outline: 1px solid #999;
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body {
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font: 16px sans-serif;

‎images/In-Black-66px-TM.png

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‎images/In-Black-89px-TM.png

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‎images/Magellanic_Stream_3_1.jpeg

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‎images/Magellanic_Stream_5_1.jpeg

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‎images/Magellanic_Stream_7_1.jpeg

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‎images/Magellanic_Stream_9_1.jpeg

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‎images/researchthumbnails/ChemTagging.png

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‎index.html

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---
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layout: default
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layout: front
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title: Stephen Pardy
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---
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<h2>Stephen Pardy</h2>
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<div class="container">
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<div class="container aboutcontainer">
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<div class="row">
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<div class="col-md-8">
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<h2>About me</h2>
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<p>I am a fifth year graduate student working with <a href="http://www.elenadonghia.com/">Elena D'Onghia</a> at the University of Wisconsin - Madison.</p>
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<p>I run computational models of galaxies to understand how small galaxies grow, interact, and ultimately build larger systems like the Milky Way.</p>
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<p>My work focuses Magellanic spirals - galaxies that, like the Large Magellanic Cloud, have misplaced bars, single spiral arms, or irregular features. Much of my current work is focused on how these galaxies can contribute gas to our own galaxy in the form of cold gas streams, and how the satellite population may be different around these galaxies.</p>
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<div class="col-md-4">
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<img src="/images/HeadShot.jpeg" alt="HeadShot" height=300>
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<p> You can also check out our group's <a href="https://donghiagroup.github.io/">Github page</a> to see publicly-available code.</p>
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<img src="/images/HeadShot.jpeg" alt="HeadShot" height=300>
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<div class='col-md-6'>
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<div class="container">
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<h1>Stephen Pardy</h1>
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<h2>PhD Student - Astronomy</h2>
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</div>
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</div>
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<div class="row">
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<p>email: stephenpardy [at] gmail.com</p>
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</div>
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<div class="col-sm-1">
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<p><a href="https://github.com/stephenpardy"><img src="/images/GitHub-Mark-64px.png" alt="Github"></a>
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</div>
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<div class="col-sm-1">
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<a href="http://www.researchgate.net/profile/Stephen_Pardy"><img src="/images/researchgate2.svg" height=64px width=64px alt="Research Gate"></img></a></p>
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</div>
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<div class="col-sm-1">
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<a href="https://www.linkedin.com/in/stephen-pardy-599b7b98"><img src="/images/In-Black-66px-TM.png" height=66px width=78px alt='linkedin'></img></a></p>
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‎research/index.html

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---
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<link href="{{ site.baseurl }}/css/research.css" rel="stylesheet">
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<div class="container">
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<h2>Research Projects</h2>
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<div class="row">
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<ul class="img-list">
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<li>
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<a href="#Stream">
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<img src="{{ site.baseurl }}/images/researchthumbnails/MagellanicStream.png" width="150" height="150" />
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<span class="text-content"><span>Magellanic Stream</span></span>
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</a>
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</li>
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<a href="#Magellanics">
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<img src="{{ site.baseurl }}/images/researchthumbnails/Magellanic.png" width="150" height="150" />
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<span class="text-content"><span>Magellanic Galaxies</span></span>
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</a>
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</li>
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<a href="#ISIMA">
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<img src="{{ site.baseurl }}/images/researchthumbnails/isima_tail.png" width="150" height="150" />
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<span class="text-content"><span>Tidal Streams</span></span>
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</a>
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</li>
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<a href="#LARS">
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<img src="{{ site.baseurl }}/images/researchthumbnails/lars.png" width="150" height="150" />
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<span class="text-content"><span>Lyman Alpha Reference Sample</span></span>
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</a>
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</li>
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</ul>
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</div>
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<h2>Overview:</h2>
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<p>I work in Professor <a href="http://www.elenadonghia.com/">Elena D'Onghia's group</a>. Her work focuses on dynamics of disks like our Milky Way. One of the issues is how spiral arms form. You can play with am interactive version of her results <a href="{{ site.baseurl }}/research_visualizations/num_arms.html">here</a>.</p>
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<p> You can also check out our group's <a href="https://donghiagroup.github.io/">Github page</a> to see publicly-available code.</p>
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<p>My thesis work focuses on small galaxies. I use computation models to understand how these small systems grow, interact, and ultimately build larger systems like the Milky Way.
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In particular, I focus on Magellanic spirals - galaxies that, like the Large Magellanic Cloud, have misplaced bars, single spiral arms, or irregular features. I have written papers on how these galaxies interact, how they can contribute gas to our own galaxy in the form of cold gas streams, and how the satellite population may be different around them.</p>
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<h2>Research Projects</h2>
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<div class="row">
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<ul class="img-list">
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<li>
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<a href="#Stream">
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<img src="{{ site.baseurl }}/images/researchthumbnails/MagellanicStream.png" width="150" height="150" />
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<span class="text-content"><span>Magellanic Stream</span></span>
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</a>
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</li>
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<li>
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<a href="#Magellanics">
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<img src="{{ site.baseurl }}/images/researchthumbnails/Magellanic.png" width="150" height="150" />
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<span class="text-content"><span>Magellanic Galaxies</span></span>
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</a>
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</li>
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<li>
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<a href="#ChemTagging">
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<img src="{{ site.baseurl }}/images/researchthumbnails/ChemTagging.png" width="150" height="150" />
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<span class="text-content"><span>Chemical Tagging</span></span>
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</a>
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</li>
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<li>
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<a href="#ISIMA">
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<img src="{{ site.baseurl }}/images/researchthumbnails/isima_tail.png" width="150" height="150" />
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<span class="text-content"><span>Tidal Streams</span></span>
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</a>
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</li>
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<li>
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<a href="#LARS">
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<img src="{{ site.baseurl }}/images/researchthumbnails/lars.png" width="150" height="150" />
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<span class="text-content"><span>Lyman Alpha Reference Sample</span></span>
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</a>
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</li>
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</ul>
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</div>
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<h2>Multiple Filaments in the Magellanic Stream</h2>
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<p>My current work focuses on the interaction between the Large and Small Magellanic Clouds. My simulations explore how this interaction formed the complex and extensive stream of HI gas seen around the Clouds. Stay tuned for details.</p>
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<h4>Paper: <a href="https://arxiv.org/abs/1802.01600">arxiv/1802.01600</a></h4>
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<p>Some of my current work focuses on the interaction between the Large and Small Magellanic Clouds. My simulations explore how this interaction formed the complex and extensive stream of HI gas seen around the Clouds.</p>
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<p>You can explore some of our results <a href="{{ site.baseurl }}/research_visualizations/stream_stripping.html">here</a>.</p>
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<p>Picture: The present day distribution of gas in the Magellanic Stream from one of our simulations and in the HI gas of Nidever et al. 2010.</p>
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<h2>Asymmetries in Magellanic Galaxies</h2>
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<p>As part of my thesis project, I examined the role of interactions in causing the asymmetries in Magellanic Galaxies. See my <a href="http://arxiv.org/abs/1602.07689">paper</a> about tidally induced asymmetric-disks and how they masquerade as offset bars in Magellanic Galaxies. If you are interested, you can check out an <a href="{{ site.baseurl }}/visualization/">interactive visualization</a> of the results.</p>
59-
<p>We use a custom version of the <a href="http://www.h-its.org/english/research/tap/galic/">GalIC</a> code to
60-
simulate isolated galaxies and evolve encounters with Gadget 3.
76+
<h4>Paper: <a href="http://arxiv.org/abs/1602.07689">arxiv/1602.07689</a></h4>
77+
<p>As part of my thesis project, I examined the role of interactions in causing the asymmetries in Magellanic Galaxies. We discovered that tidally induced asymmetric-disks can masquerade as offset bars in Magellanic Galaxies. If you are interested, you can check out an <a href="{{ site.baseurl }}/research_visualizations/mag_irregulars.html">interactive visualization</a> of the results.</p>
78+
<p>We use a custom version of the <a href="http://www.h-its.org/english/research/tap/galic/">GalIC</a> code to simulate isolated galaxies and evolve encounters with Gadget 3.
6179
</p>
6280
<p>Picture: A simulation of a recently disrupted galaxy modeled after the LMC. The colors represent surface density of stars.</p>
6381
</div>
6482
</div>
65-
<div class="row proj_content A-section" id="ISIMA">
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<div class="col-xs-12 col-md-8">
67-
<h2>Tidal Streams as a Probe of Dark Matter</h2>
68-
<p>As a 2014 fellow at the <a href="http://isima.ucsc.edu/">International Summer Institute for Modeling in Astrophysics</a>, I worked with Andreas Küpper on modeling the tidal stream of NGC 5466. Tidal streams act as unique probes of the dark matter halo of their environments. This work, along with new data from Jay Strader, will place strong contraints on the shape and total mass of the Milky Way. We use a Markov chain Monte Carlo to probe parameter space, where the likelihood function is drawn in real time from very efficient restricted N-Body simulations of the globular cluster in our test potential.</p>
69-
<p>Picture: A model of the Milky Way with our best fit stream model for NGC 5466 in red.</p>
83+
<div class="row proj_content A-section" id="ChemTagging">
84+
<div class="col-xs-12 col-md-8" id="ChemTagging">
85+
<h2>Chemical Tagging</h2>
86+
<h4>Paper: <a href="https://arxiv.org/abs/1709.03987">arxiv/1709.03987</a></h4>
87+
<p> Understanding where stars are born is a fundamental problem for astrophysics. This project used detailed chemical data from the APOGEE survey of more than 100,000 stars in the Milky Way to determine if there were statistically significant groups of stars that may have been born together. You can explore an interactive visualization that shows why this problem can be so challenging <a href="{{ site.baseurl }}/research_visualizations/chemical_tagging.html">here</a>.
88+
</p>
89+
<p>Picture: Stars from known globular clusters in chemical space.</p>
7090
</div>
7191
<div class="col-xs-0 col-md-4">
72-
<p><img id="projpix" src="{{ site.baseurl }}/images/researchthumbnails/isima_tail.png" border="0" alt="" class="img-responsive"></p>
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<p><img id="projpix" src="{{ site.baseurl }}/images/researchthumbnails/ChemTagging.png" border="0" alt="" class="img-responsive"></p>
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</div>
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</div>
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<div class="row proj_content B-section" id="LARS">
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<div class="row proj_content B-section" id="ISIMA">
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<div class="col-xs-0 col-md-4">
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<p><img id="projpix" src="{{ site.baseurl }}/images/researchthumbnails/lars.png" border="0" alt="" class="img-responsive"></p>
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<p><img id="projpix" src="{{ site.baseurl }}/images/researchthumbnails/isima_tail.png" border="0" alt="" class="img-responsive"></p>
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</div>
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<div class="col-xs-12 col-md-8">
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<h2>Tidal Streams as a Probe of Dark Matter</h2>
101+
<p>As a 2014 fellow at the <a href="http://isima.ucsc.edu/">International Summer Institute for Modeling in Astrophysics</a>, I worked with Andreas Küpper on modeling the tidal stream of NGC 5466. Tidal streams act as unique probes of the dark matter halo of their environments. This work, along with new data from Jay Strader, will place strong contraints on the shape and total mass of the Milky Way. We use a Markov chain Monte Carlo to probe parameter space, where the likelihood function is drawn in real time from very efficient restricted N-Body simulations of the globular cluster in our test potential.</p>
102+
<p>Picture: A model of the Milky Way with our best fit stream model for NGC 5466 in red.</p>
103+
</div>
104+
</div>
105+
<div class="row proj_content A-section" id="LARS">
79106
<div class="col-xs-12 col-md-8">
80107
<h2>LARS and eLARS</h2>
108+
<h4>Papers: <a href="http://arxiv.org/abs/1408.6275">arxiv/1408.6275</a> and <a href="https://arxiv.org/abs/1609.04020">arxiv/1609.04020</a></h4>
81109
<p>The Lyman Alpha Reference Sample (LARS) is a large Hubble project and international collaboration testing the escape of Lyman Alpha photons from distant galaxies.</p>
82110
<p>LARS utilizes almost the entire electromagnetic spectrum: from UV and optical spectra that reveal intense star formation, to radio observations that probe the neutral hydrogen and molecular gas content. The survey started with 14 galaxies and 28 more have now been added through e(xtended)LARS. We have conducted HI observations using the GBT, VLA, and GMRT of all 14 LARS galaxies and many of the 28 eLARS.</p>
83-
<p>I recently published a <a href="http://arxiv.org/abs/1408.6275">paper</a> detailing the reduction and analysis of these first 14 galaxies.</p>
111+
<p>In 2014, we released the results for the first 14 galaxies. A few years later we added to this by carrying out similar measurements on a strange galaxy (Haro 11) that emits lots of Lyman Alpha and Lyman Continuum emission.</p>
84112
<p>Picture: HI contours on DSS image of interacting galaxies Arp 238 (LARS 03).</p>
85113
<p></p>
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</div>
115+
<div class="col-xs-0 col-md-4">
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<p><img id="projpix" src="{{ site.baseurl }}/images/researchthumbnails/lars.png" border="0" alt="" class="img-responsive"></p>
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</div>
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</div>
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</div>
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‎_visualizations/num_arms.html ‎research_visualizations/num_arms.html

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‎research_visualizations/stream_stripping.html

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---
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layout: default
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title: "Magellanic Stream Gas Stripping"
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thumbnail: /images/vizthumbnails/stream_stripping_thumbnail.png
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abstract: Explore the Magellanic Stream Gas.
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---
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<div class="container">
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<h4>Explore the removal of gas from the Magellanic Stream</h4>
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<iframe src="{{ site.baseurl }}/resources/astro/streamstripping_interactive.html" marginwidth="0" marginheight="0" scrolling="no" width="1400" height="1000" frameborder="0"></iframe>
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</div>

‎resources/astro/Magellanic_Stream_3_1.jpeg

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‎resources/astro/streamstripping_interactive.html

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---
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<!DOCTYPE html>
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<link href="https://maxcdn.bootstrapcdn.com/bootstrap/3.3.7/css/bootstrap.min.css" rel="stylesheet">
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color: #FFFFFF;
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</style>
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<body>
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<div class='container'>
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<div class="row">
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<div class="col-sm-3">
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<form name="input1" onSubmit="return handleClick()">
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<input name="Submit" type="submit" value="Set observed value." >
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<p>LMC HI Mass=4x10^8</p>
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<p>SMC HI Mass=2x10^8</p>
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<p>LMC Ionized fraction=<input type="text" id="inputLmcIonized" placeholder="0.4"></p>
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<p>SMC Ionized fraction=<input type="text" id="inputSmcIonized" placeholder="0.4"></p>
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<p>Stream HI Mass=4x10^8 Msun</p>
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<p>Stream Ionized Mass=2x10^9 Msun</p>
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<div class="row">
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<div class="col-sm-9">
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<p><div class="topfrac">
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4x10^8 + 2x10^9
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</div>
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<div class="bottomfrac">
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4x10^8 + 2x10^9 + 4x10^8 + 2x10^8 + <span id='spanLMCIonized'>1.6</span>x10^8
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+ <span id='spanSMCIonized'>0.8</span>x10^8
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</div>
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</p></div>
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<div class='col-sm-3'>
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<p>
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=<span id='spanPerc'>20</span>%
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</p>
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</div>
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</div>
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</form>
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</div>
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<div class="col-sm-6">
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<p><span id="info"></span></p>
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<table class="blueTable">
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<thead>
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<tr>
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<th>Galaxy</th>
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<th>Mtot</th>
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<th>Mstream</th>
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<th>Mgal</th>
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<th>Fstripped</th>
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</tr>
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</thead>
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<tbody>
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<tr>
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<td>LMC</td>
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<td><span id='LMCmtot'></span></td>
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<td><span id='LMCmstream'></span></td>
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<td><span id='LMCmgalaxy'></span></td>
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<td><span id='LMCf'></span></td>
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</tr>
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<tr>
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<td>SMC</td>
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<td><span id='SMCmtot'></span></td>
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<td><span id='SMCmstream'></span></td>
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<td><span id='SMCmgalaxy'></span></td>
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<td><span id='SMCf'></span></td>
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</tr>
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<tr>
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<td>Total</td>
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<td><span id='Totalmtot'></span></td>
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<td><span id='Totalmstream'></span></td>
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<td><span id='Totalmgalaxy'></span></td>
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<td><span id='Totalf'></span></td>
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</tr>
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</tbody>
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</table>
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</div>
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</div>
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<div class='row'>
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<div class="col-sm-4">
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<div id="chart"></div>
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</div>
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<div class="col-md-6">
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<div id='img'></div>
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</div>
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</div>
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</div>
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<script src="https://d3js.org/d3.v4.min.js"></script>
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<script src="https://ajax.googleapis.com/ajax/libs/jquery/1.11.1/jquery.min.js"></script>
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<script>
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function handleClick(event){
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valLMCIonized = +document.getElementById("inputLmcIonized").value;
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valSMCIonized = +document.getElementById("inputSmcIonized").value;
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LMCIonizedMass = valLMCIonized/(1-valLMCIonized)*4;
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document.getElementById("spanLMCIonized").textContent = LMCIonizedMass;
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SMCIonizedMass = valSMCIonized/(1-valSMCIonized)*2;
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document.getElementById("spanSMCIonized").textContent = SMCIonizedMass;
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assumedPerc = 100*(4+20)/(4+20+4+2+LMCIonizedMass+SMCIonizedMass);
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console.log(assumedPerc);
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document.getElementById("spanPerc").textContent = assumedPerc;
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svg.selectAll('.line')
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.attr("y1", y(assumedPerc))
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.attr("y2", y(assumedPerc));
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return false;
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var assumedPerc = 50;
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var data = [{perc: 21.6, ratio: 9, details: "This is the fiducial case.",
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imgURL: "Magellanic_Stream_9_1.jpeg", table: {'LMC': {'mtot': 12.6, 'mstream': 2.3, 'mgalaxy': 10.3, 'f': 18.0}, 'SMC': {'mtot': 5.4, 'mstream': 1.6, 'mgalaxy': 3.8, 'f': 29.8}, 'Total': {'mtot': 17.9, 'mstream': 3.9, 'mgalaxy': 14.0, 'f': 21.6}}},
230+
{perc: 17.8, ratio: 7, details: "These are some details about 7:1",
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imgURL: "Magellanic_Stream_7_1.jpeg", table: {'LMC': {'mtot': 6.7, 'mstream': 0.2, 'mgalaxy': 6.5, 'f': 2.7}, 'SMC': {'mtot': 3.5, 'mstream': 1.6, 'mgalaxy': 1.9, 'f': 46.8}, 'Total': {'mtot': 10.1, 'mstream': 1.8, 'mgalaxy': 8.3, 'f': 17.8}}},
232+
{perc: 10.0, ratio: 5, details: "These are some details about 5:1",
233+
imgURL: "Magellanic_Stream_5_1.jpeg", table: {'LMC': {'mtot': 5.7, 'mstream': 0.3, 'mgalaxy': 5.4, 'f': 5.7}, 'SMC': {'mtot': 4.9, 'mstream': 0.7, 'mgalaxy': 4.1, 'f': 15.1}, 'Total': {'mtot': 10.6, 'mstream': 1.1, 'mgalaxy': 9.5, 'f': 10.0}}},
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{perc: 20.9, ratio: 3, details: "These are some details about 3:1",
235+
imgURL: "Magellanic_Stream_3_1.jpeg", table: {'LMC': {'mtot': 5.4, 'mstream': 0.2, 'mgalaxy': 5.1, 'f': 4.2}, 'SMC': {'mtot': 9.9, 'mstream': 3.0, 'mgalaxy': 6.9, 'f': 29.9}, 'Total': {'mtot': 15.3, 'mstream': 3.2, 'mgalaxy': 12.1, 'f': 20.9}}}
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</body>

‎visualization/index.html

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