Update Research Topics authored by Thomas Bretz's avatar Thomas Bretz
...@@ -9,7 +9,9 @@ ...@@ -9,7 +9,9 @@
<li> Astroparticle physics <li> Astroparticle physics
<li> Quest for the still unknown origin and acceleration of cosmic rays <li> Quest for the still unknown origin and acceleration of cosmic rays
<li> Measurement of the spectrum and composition of cosmic-rays <li> Measurement of the spectrum and composition of cosmic-rays
<li> Upgrade on-going for a better determination of the primary particle type <li> Upgrade ongoing for a better determination of the primary particle type
<li> Where do Ultra-High Energy cosmic-rays come from?
<li> Which process is responsible for their acceleration?
</ul> </ul>
</blockquote> </blockquote>
</details> </details>
...@@ -31,9 +33,8 @@ ...@@ -31,9 +33,8 @@
<summary>Possible topics for Bachelor- and Master-theses</summary> <summary>Possible topics for Bachelor- and Master-theses</summary>
<blockquote> <blockquote>
<ul> <ul>
<li>Chemical composition using AugerPrime and Deep Learning <li>Is the GZK effect responsible for the cut-off at the highest energies? Chemical composition using AugerPrime and Deep Learning
<li>Anylsis of the performance of a novel prototype array using SiPMs <li>Is the galactic center responsible for cosmic-rays on Earth? Search for UHE Photons with machine learning
<li>Search for ultra-high energetic photons using AugerPrime
</ul> </ul>
</blockquote> </blockquote>
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...@@ -54,6 +55,8 @@ ...@@ -54,6 +55,8 @@
<li> Astronomy at TeV energies <li> Astronomy at TeV energies
<li> Possible origin of cosmic-rays: Active Galactic Nuclei <li> Possible origin of cosmic-rays: Active Galactic Nuclei
<li> Time evolution of their spectrum (monitoring) <li> Time evolution of their spectrum (monitoring)
<li> What drives the violent behavior of these objects?
<li> What process is responsible for the energy transfer?
</ul> </ul>
</blockquote> </blockquote>
</details> </details>
...@@ -74,12 +77,9 @@ ...@@ -74,12 +77,9 @@
<summary>Possible topics for Bachelor- and Master-theses</summary> <summary>Possible topics for Bachelor- and Master-theses</summary>
<blockquote> <blockquote>
<ul> <ul>
<li>Improved background suppression using Deep Learning <li>Search for triggered transient events: Improved background suppression using Deep Learning
<li>Improved energy resolution using Deep Learning <li>How does the spectrum change with flux? Improved energy resolution using Deep Learning
<li>Search for periodicity in Active Galactic Nuclei <li>Never seen before: Search for periodicity in Active Galactic Nuclei
<li>Programming of an online database for flux-data of Active Galactic Nuclei
<li>Analytical description of the zenith-angle dependent trigger-rate
<li>Implementation of a database-driven data analysis
</ul> </ul>
</blockquote> </blockquote>
</details> </details>
...@@ -121,10 +121,8 @@ ...@@ -121,10 +121,8 @@
<summary>Possible topics for Bachelor- and Master-theses</summary> <summary>Possible topics for Bachelor- and Master-theses</summary>
<blockquote> <blockquote>
<ul> <ul>
<li>Improvement of Background suppression and Energy resolultion using Deep Learning <li>What is the performance we get from the hybrid system? Improvement of Background suppression and Energy resolution using Deep Learning
<li>Simulation of the performance of the first Hybrid Detector <li>First detection of a source in the hybrid setup: First hybrid measurement of the Crab Nebula
<li>First hybrid measurement of the Crab Nebula using an array of three telescope
<li>Calibration measurements of the water tanks using a scintillator detector
</ul> </ul>
</blockquote> </blockquote>
</details> </details>
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