minor changes

_config.yml

@@ -33,11 +33,11 @@ navbar-links:
 
 # Image to show in the navigation bar - image must be a square (width = height)
 # Remove this parameter if you don't want an image in the navbar
-# avatar: "/img/profile0.jpg"
+avatar: "/img/profile0.jpg"
 
 # If you want to have an image logo in the top-left corner instead of the title text,
 # then specify the following parameter
-title-img: "/img/profile0.jpg"
+# title-img: "/img/profile0.jpg"
 
 # --- Footer options --- #
 

research.md

@@ -5,27 +5,27 @@ title: Research
 
 
 <h3>
-    <a name='IceCube'></a> IceCube
+    <a name='IceCube'></a> IceCube<br/> 
     <span class="badge badge-primary">Analysis</span>
     <span class="badge badge-primary">Software</span>
     <span class="badge badge-primary">Hardware</span>
 </h3>
 
 <p> 
-The IceCube Neutrino Observatory, located at the South Pole, represents a groundbreaking advancement in astrophysical research. Comprising over 5,000 optical sensors embedded in a cubic kilometer of ice, IceCube is designed to detect high-energy neutrinos originating from cosmic sources such as supernovae, gamma-ray bursts, and active galactic nuclei. By capturing these elusive particles, IceCube provides crucial insights into the universe's most energetic phenomena, aiding our understanding of fundamental physics and the cosmos.
+     The IceCube Neutrino Observatory, located at the South Pole, represents a groundbreaking advancement in astrophysical research. Comprising over 5,000 optical sensors embedded in a cubic kilometer of ice, IceCube is designed to detect high-energy neutrinos originating from cosmic sources such as supernovae, gamma-ray bursts, and active galactic nuclei. By capturing these elusive particles, IceCube provides crucial insights into the universe's most energetic phenomena, aiding our understanding of fundamental physics and the cosmos.
 <br/> 
-In recent years, researchers have increasingly focused on the potential connections between neutrinos and dark matter, one of the most enigmatic components of the universe. Dark matter, which constitutes about 27% of the universe's mass-energy content, interacts gravitationally but remains largely undetectable through conventional means. The search for dark matter candidates, including Weakly Interacting Massive Particles (WIMPs) and other exotic particles, often hinges on their potential interactions with neutrinos.
+     In recent years, researchers have increasingly focused on the potential connections between neutrinos and dark matter, one of the most enigmatic components of the universe. Dark matter, which constitutes about 27% of the universe's mass-energy content, interacts gravitationally but remains largely undetectable through conventional means. The search for dark matter candidates, including Weakly Interacting Massive Particles (WIMPs) and other exotic particles, often hinges on their potential interactions with neutrinos.
 <br/> 
-IceCube plays a pivotal role in these searches by investigating how dark matter might produce neutrinos through annihilation or decay processes in regions of high dark matter density, such as the center of galaxies or the Sun. By analyzing the resulting neutrino flux, scientists aim to uncover signatures of dark matter interactions, shedding light on its nature and properties.
+     IceCube plays a pivotal role in these searches by investigating how dark matter might produce neutrinos through annihilation or decay processes in regions of high dark matter density, such as the center of galaxies or the Sun. By analyzing the resulting neutrino flux, scientists aim to uncover signatures of dark matter interactions, shedding light on its nature and properties.
 <br/> 
-This dual focus on high-energy neutrinos and dark matter interactions not only enriches our understanding of particle physics but also enhances our comprehension of the universe's structure and evolution. As research progresses, the IceCube Neutrino Observatory continues to be at the forefront of these exciting inquiries, pushing the boundaries of knowledge in both astrophysics and cosmology.
+     This dual focus on high-energy neutrinos and dark matter interactions not only enriches our understanding of particle physics but also enhances our comprehension of the universe's structure and evolution. As research progresses, the IceCube Neutrino Observatory continues to be at the forefront of these exciting inquiries, pushing the boundaries of knowledge in both astrophysics and cosmology.
 </p> 
 
 
 <div class="media">
     <div class="media-body">
        <p class="media-heading">
-           <a><img src="https://www.google.com/url?sa=i&url=https%3A%2F%2Ficecube.wisc.edu%2Fscience%2Ficecube%2F&psig=AOvVaw0vDK8AzLSUAg_9S6a9Dufy&ust=1729097394147000&source=images&cd=vfe&opi=89978449&ved=0CBQQjRxqFwoTCLDri_PrkIkDFQAAAAAdAAAAABAE" alt="IceCube" style="width:300px;height:800px;"></a>
+           <img src="https://www.google.com/url?sa=i&url=https%3A%2F%2Ficecube.wisc.edu%2Fscience%2Ficecube%2F&psig=AOvVaw0vDK8AzLSUAg_9S6a9Dufy&ust=1729097394147000&source=images&cd=vfe&opi=89978449&ved=0CBQQjRxqFwoTCLDri_PrkIkDFQAAAAAdAAAAABAE" alt="IceCube" style="width:300px;height:800px;">
        </p>
     </div>
 </div>
@@ -34,18 +34,18 @@ This dual focus on high-energy neutrinos and dark matter interactions not only e
 
 
 <h3>
-    <a name='TAMBO'></a> TAMBO
+    <a name='TAMBO'></a> TAMBO<br/> 
     <span class="badge badge-primary">Hardware</span>
 </h3>
 
 <p> 
-TAMBO (Tau Air-Shower Mountain-Based Observatory) is a proposed water-Cherenkov detector set on a cliff-edge in the high Peruvian Andes. Utilizing the unique geometry of the Colca valley, TAMBO is situated to produce a high-purity sample of 1–100 PeV astrophysical tau neutrino events, providing a novel aperture into the under-explored component of the existing high-energy neutrino spectrum.
+     TAMBO (Tau Air-Shower Mountain-Based Observatory) is a proposed water-Cherenkov detector set on a cliff-edge in the high Peruvian Andes. Utilizing the unique geometry of the Colca valley, TAMBO is situated to produce a high-purity sample of 1–100 PeV astrophysical tau neutrino events, providing a novel aperture into the under-explored component of the existing high-energy neutrino spectrum.
 </p> 
 
 <div class="media">
     <div class="media-body">
        <p class="media-heading">
-           <a><img src="https://www.google.com/url?sa=i&url=https%3A%2F%2Findico.fnal.gov%2Fevent%2F63406%2Fcontributions%2F297967%2Fattachments%2F181754%2F249338%2FTAMBOTalk_RobertMihaiAmarinei.pdf&psig=AOvVaw3_fwBb4JIrOuTgyqtS8Z-m&ust=1729097268613000&source=images&cd=vfe&opi=89978449&ved=0CBQQjRxqFwoTCLCPvbXrkIkDFQAAAAAdAAAAABAS" alt="TAMBO" style="width:800px;height:300px;"></a>
+           <img src="https://www.google.com/url?sa=i&url=https%3A%2F%2Findico.fnal.gov%2Fevent%2F63406%2Fcontributions%2F297967%2Fattachments%2F181754%2F249338%2FTAMBOTalk_RobertMihaiAmarinei.pdf&psig=AOvVaw3_fwBb4JIrOuTgyqtS8Z-m&ust=1729097268613000&source=images&cd=vfe&opi=89978449&ved=0CBQQjRxqFwoTCLCPvbXrkIkDFQAAAAAdAAAAABAS" alt="TAMBO" style="width:800px;height:300px;">
        </p>
     </div>
 </div>