update

EiffL · Nov 8, 2024 · 00a732b · 00a732b
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Showing 1 changed file with 6 additions and 6 deletions.
diff --git a/Paris2024/index.html b/Paris2024/index.html
@@ -59,7 +59,7 @@ <h2>François Lanusse</h2>
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-			<section data-background-image="/talks/assets/WMAP_timeline_large.jpg">
+			<!-- <section data-background-image="/talks/assets/WMAP_timeline_large.jpg">
 				<h3 class="slide-title" style="position: absolute; top: 0">
 				  the $\Lambda$CDM view of the Universe
 				</h3>
@@ -99,7 +99,7 @@ <h3 class="slide-title" style="position: absolute; top: 0">
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 			<section>
 				<section data-background-video="/talks/assets/animation-day-to-night.mov" data-background-video-muted>
@@ -286,7 +286,7 @@ <h3 class='slide-title'>Cosmological Simulation-Based Inference</h3>
 		<!-- <div class="fragment">For this talk, let's <b class="alert">ignore the elephant in the room</b>:<br> <b>Do we have reliable enough models for the full complexity of the data?</b></div> -->
 	</section>
 
-	<section>
+	<!-- <section>
 		<h3 class="slide-title">...so why is this not completely mainstream?</h3>
 			<img class="plain" data-src="/talks/assets/lfi_sim.png" style="width:1000px;"/>
 	
@@ -305,7 +305,7 @@ <h3 class="slide-title">...so why is this not completely mainstream?</h3>
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+	</section> -->
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 	<section>
@@ -1407,8 +1407,8 @@ <h3 class="slide-title">Solution of the heat equation on SO(3)</h3>
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 						<li class="fragment"> Like the Gaussian distribution, it is <b class="alert">closed under convolution</b>, corresponds to the <b class="alert">solution of the heat diffusion</b> process on SO(3).
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-						<li class="fragment"> In the limit of small $\epsilon$, it is close to the Gaussian distribution. For large $\epsilon$ it tends to the uniform distribution on $\mathrm{SO}(3)$.
-						  </li>
+						<!-- <li class="fragment"> In the limit of small $\epsilon$, it is close to the Gaussian distribution. For large $\epsilon$ it tends to the uniform distribution on $\mathrm{SO}(3)$.
+						  </li> -->
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