Description
The discovery of a new radiation component at TeV energies in the Vela pulsar, beating at the same frequency that the rotational period of the pulsar, has opened the door for new, exciting interpretations of acceleration of particles in extreme environments. The H.E.S.S. archival dataset with more than 15 years of observations offers a fantastic opportunity to search for more of these objects. Within this project, we will develop analysis tools (using python/GammaPy) to perform timing analysis, and search for high energy pulsation for the best pulsar candidates, using H.E.S.S. and LAT data.
Special Qualifications:
Programming Languages: python
| Field | C1: Astroparticle physics analysis and observations |
|---|---|
| DESY Place | Zeuthen |
| DESY Division | AP |
| DESY Group | HESS |
Primary authors
Emma Maria de Ona Wilhelmi
(Z_GA (Gammaastronomie))
Stefan Ohm
(Z_HESS (High Energy Steroscopic System))
