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Author: CarrieFilion

index.html

@@ -107,7 +107,7 @@ <h2> <b> EXP </b>: applications to cosmology</h2>
 								</ul>
 						</article>
 						<article class="thumb">
-							<a href="images/fulls/5.png" class="image"><img src="images/thumbs/4.png" alt="" /></a>
+							<a href="images/fulls/4.png" class="image"><img src="images/thumbs/center-2.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 
@@ -142,7 +142,7 @@ <h2> <b> EXP</b>: applications to dynamical systems </h2>
 								<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 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 
-									<a href="https://ui.adsabs.harvard.edu/abs/2023MNRAS.521.1757J/abstract">Johnson, Petersen et al, 2023</a>;</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>
@@ -160,7 +160,7 @@ <h2> <b> EXP</b>: applications to observations</h2>
 								lopsidedness in galaxies 
 								(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 
+								 These expansions are also how we map an image of a galaxy 
 								 <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>