I'm working at the
IAAT on a PhD thesis in Very High Energy Astronomy.
The thesis will contain two parts, one deals with the development of the Mirror Alignment Control System for phase II of the
HESS experiment. The other part is a morphology study of HESS I data from the source HESSJ1837-069.
The HESS telescopes
The
HESS experiment currently operates 4 telescopes in Namibia. A new extension,
HESS phase II, is under construction. I'm developing a semi-automatic system for aligning the ~900 mirrors of the new telescope.
The morphology study
One problem with most Very High Energy data at the moment is that the observational background is very high compared to the source signal, and that both are very low. This means that we have to deal with data that follows a Poisson distribution rather then a Gaussian distribution.
This causes all kinds of problems. Luckily there are other people around the world facing the same problem and some of them might have found
good solutions to deal with this.
General analysis results of the source can be found
here, if you are part of the HESS collaboration