wee edits

Author: CarrieFilion

assets/css/main.css

@@ -1270,13 +1270,14 @@ input, select, textarea {
 			cursor: default;
 			left: 0;
 			position: absolute;
-			text-align: center;
+			text-align: left;
 			width: 100%;
 			height: 100%;
 			z-index: 2;
 			overflow-y: auto;
 			box-sizing: border-box;
 			background: none;
+			color: #000000;
 		}
 
 			.poptrox-popup .caption h2, .poptrox-popup .caption h3, .poptrox-popup .caption h4, .poptrox-popup .caption h5, .poptrox-popup .caption h6 {
@@ -1288,6 +1289,19 @@ input, select, textarea {
 				color: #000000;
 			}
 
+			.poptrox-popup .caption ul,
+			.poptrox-popup .caption ol {
+				text-align: left;
+				padding-left: 1.5em;
+				margin: 0.5em 0 1em 0;
+			}
+
+			.poptrox-popup .caption ul li,
+			.poptrox-popup .caption ol li {
+				padding-left: 0.25em;
+				margin-bottom: 0.4em;
+			}
+
 		.poptrox-popup .loader {
 			-moz-animation: spinner 1s infinite linear !important;
 			-webkit-animation: spinner 1s infinite linear !important;

assets/sass/components/_poptrox-popup.scss

@@ -91,14 +91,26 @@
 			overflow-y: auto;
 			box-sizing: border-box;
 			background: none;
+			color: #000000;
 
 			h2, h3, h4, h5, h6 {
 				margin: 0 0 (_size(element-margin) * 0.25) 0;
 				color: #000000;
 			}
 
 			p {
-				color: _palette(fg-bold);
+				color: #000000;
+			}
+
+			ul, ol {
+				text-align: left;
+				padding-left: 1.5em;
+				margin: 0.5em 0 1em 0;
+			}
+
+			ul li, ol li {
+				padding-left: 0.25em;
+				margin-bottom: 0.4em;
 			}
 		}
 

index.html

@@ -55,7 +55,7 @@ <h2> What is a basis function expansion? </h2>
 								have been used to derive potential fields at each timestep from particle data at computational effort 
 								proportional to the number of particles – drastically less computationally intense than other 
 								techniques to determine potentials 
-								<a href="https://ui.adsabs.harvard.edu/abs/1992ApJ...386..375H/abstract">Hernquist (1992)</a>. </p>
+								<a href="https://ui.adsabs.harvard.edu/abs/1992ApJ...386..375H/abstract">(Hernquist, 1992)</a>. </p>
 							<p> More generally: in theoretical analyses, BFE have been partnered with mathematical tools of 
 								perturbation theory and linear algebra to solve equations, to describe interactions and identify 
 								physical mechanisms such as in the interaction of the Milky Way and Large Magellanic Cloud 
@@ -96,18 +96,18 @@ <h2> <b> EXP </b>: applications to cosmology</h2>
 								these tools to snapshots from simulations of galaxy formation to: </p>
 								<ul>
 									<li> Compare and contrast the signatures of filamentary accretion from halo deformation in the FIRE simulation suite 
-										(<a “https://ui.adsabs.harvard.edu/abs/2025ApJ...988..190A/abstract” Arora et al, 2025 </a>); </li>
+										(<a href="https://ui.adsabs.harvard.edu/abs/2025ApJ...988..190A/abstract">Arora et al, 2025</a>); </li>
 									<li> Describe the deformation of dark matter halos as they respond to infalling satellites in the MWest simulation suite 
 										(Darragh-Ford et al 2025, in prep)</li>
 									<li> Characterise the effect of deforming dark matter halos on the structural properties of disks  in the Auriga simulation 
 										suite (Lavin et al 2025, in prep); </li>
 									<li> Investigate the interplay between dynamical structure formation, dark matter physics, and feedback mechanisms in the 
-										<a “https://dreams-project.readthedocs.io/en/latest/index.html” DREAMS<a/> suite of cosmological simulations 
+										<a href="https://dreams-project.readthedocs.io/en/latest/index.html" target="_blank">DREAMS</a> suite of cosmological simulations 
 										(Filion et al 2025, in prep) </li>
 								</ul>
 						</article>
 						<article class="thumb">
-							<a href="images/fulls/5.png" class="image"><img src="images/thumbs/center-2.png" alt="" /></a>
+							<a href="images/fulls/5.png" class="image"><img src="images/thumbs/4.png" alt="" /></a>
 							<h2> <b> Exp </b>: the code and the collaboration </h2>
 							<p><b> Exp </b> is designed to connect: (1) theoretical descriptions of dynamics, (2) N-body simulations, and (3) data-efficient descriptions of 
 								their natural consequences.  <b> Exp </b> provides recent developments from applied mathematics and numerical computation to represent time 
@@ -140,9 +140,9 @@ <h2> <b> EXP</b>: applications to dynamical systems </h2>
 							<p> The collaboration has applied <b> EXP </b> to various simulations to: </p>
 							<ul>
 								<li> Follow the evolution of galactic bars (<a”https://ui.adsabs.harvard.edu/abs/2021MNRAS.501.5408W/abstract” Weinberg & Petersen 2020</a>), 
-									as well as its interaction with a dark matter halo (<a “https://ui.adsabs.harvard.edu/abs/2025arXiv251009751H/abstract” Hunt et al, 2025></a>)</li>
+									as well as its interaction with a dark matter halo (<a href="https://ui.adsabs.harvard.edu/abs/2025arXiv251009751H/abstract">Hunt et al, 2025</a>)</li>
 								<li> Distinguish intrinsic halo instabilities from evolution driven by disk/halo coupling in the simulation of an isolated galaxy 
-									(https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.1757J/abstract Johnson, Petersen et al 2023);</li>
+									<a href="https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.1757J/abstract">Johnson, Petersen et al, 2023</a>;</li>
 								<li> Isolate the signatures of multiple interacting satellites in a simulated galactic disk (Petersen et al 2025, in prep);</li>
 								<li> Connect features found in phase-space local patches of a simulated disk into global structures (Tavangar et al 2025, in prep);</li>
 								<li> Characterize the morphological transformation of the SMC and LMC as they orbit our Milky Way (Rathore et al 2025, in prep)</li>
@@ -161,7 +161,7 @@ <h2> <b> EXP</b>: applications to observations</h2>
 								(e.g. <a href=”https://ui.adsabs.harvard.edu/abs/2025MNRAS.539..661G/abstract”>Ganapathy et al 2025</a>),
 								 measure galaxy inclination (e.g. Martinez et al, in prep), and identify morphological features like bars. 
 								 These expansions are also how we map an image of a 
-								 (<a href=”https://carriefilion.github.io/#Sonification”>into a sound </a>) via sonification. Similarly, 
+								 <a href=”https://carriefilion.github.io/#Sonification”>into a sound </a> via sonification. Similarly, 
 								 we can perform expansions of integral field spectrograph data, which allow for analyses of both velocity 
 								 and chemical information. </p>
 						</article>