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assets/css/main.css

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-webkit-transition-delay: 2.075s;
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-ms-transition-delay: 2.075s;
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transition-delay: 2.075s;
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height: 20%;
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height: calc(40vh - 2em);
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min-height: 20em;
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width: 33.333333%;
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}

assets/js/main.js

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usePopupForceClose: true,
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usePopupLoader: true,
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usePopupNav: true,
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windowMargin: 50
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windowMargin: 20
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});
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// Hack: Set margins to 0 when 'xsmall' activates.

index.html

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@@ -61,7 +61,7 @@ <h2>Why should I use basis function expansions?</h2>
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Analysis (mSSA), and examples of using mSSA + BFE for dynamical discovery can be seen in
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<a href="https://ui.adsabs.harvard.edu/abs/2021MNRAS.501.5408W/abstract">here</a> and
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<a href="https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.1757J/abstract">here</a> (see also the
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<a href = "https://exp-docs.readthedocs.io/en/latest/topics/ssa.html">EXP readme</a>).
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<a href = "https://exp-docs.readthedocs.io/en/latest/topics/ssa.html">EXP readthedocs</a>).
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A particularly powerful use of BFE is as a universal language to succinctly summarize the relevant
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dynamical information in galaxies for comparison across and between different simulations.</p>
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</article>
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how we map an image of a galaxy to a sound via sonification. We are currently developing a framework for
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expansions of integral field spectrograph data, which will allow for analyses of both velocity and chemical
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information.</p>
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<p>Quantifying <a href="https://ui.adsabs.harvard.edu/abs/2024arXiv241111972G/abstract"disk></a> asymmetry plus blurb</p>
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<p>Quantifying <a href="https://ui.adsabs.harvard.edu/abs/2024arXiv241111972G/abstract"disk></a> asymmetry</p>
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</article>
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<article class="thumb">
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<a href="images/fulls/plain.png" class="image"><img src="images/thumbs/9.png" alt="" /></a>

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