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index.md

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 ## Results
 
-<figure style="width: 50%; float: left; margin: 0 18px 6px 0;">
+<figure style="width: 50%; float: left; margin: 0 15px 10px 0;">
   <img src="assets/css/profiles.png" alt="Elbow Method Graph" style="width: 100%;">
-  <figcaption style="text-align: justify; font-size: 0.8em; font-style: italic; margin: 6px 0 0 0;">
+  <figcaption style="text-align: justify; font-size: 0.8em; font-style: italic; font-weight: 300; color: #666; margin: 10px 0 0 0;">
     Figure: Median radial profiles for Gas density (first row), Dark matter density (second row), neutral fraction (third row),
     ionisation fraction (fourth row), temperature (fifth row), a magnified version of the same temperature profiles
     (sixth row), and metallicity of filaments in the simulations at redshifts 15, 9, 7 and 5. The radius represents the
@@ -88,6 +88,7 @@ properties over time.
   </figcaption>
 </figure>
 
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 The study revealed several important trends in the evolution of cosmic filaments. As the Universe transitioned from a neutral to an ionized state, the density distribution of the filamentary network changed significantly. Higher-density filaments became more prevalent over time, reflecting the effects of gravitational collapse and radiative feedback from ionizing sources. By contrast, lower-density regions of the network diminished, likely due to the combined effects of radiation pressure and the hierarchical growth of structure.
 
 Temperature profiles showed a clear increase as a function of decreasing redshift, highlighting the progressive heating of the IGM by ionizing sources. High-density filaments developed distinct thermal envelopes, with peak temperatures observed at increasing distances from their central axes over time. This outward expansion of the heated regions suggests a dynamic interplay between radiation and the gravitational potential of the filaments. Interestingly, while lower-density filaments also experienced heating, they lacked the pronounced temperature peaks seen in their higher-density counterparts.