UCR High Energy Astrophysics

Thank you for visiting the UCR High Energy Astrophysics Research page. We are in the process of building a comprehensive page describing the our current research, so please visit this site again for more detailed info. The following gives a brief summary.

One major project is the Tracking and Imaging Gamma Ray Experiment (TIGRE), an advanced telescope for detecting and imaging celestial gamma rays from 0.3 MeV to 100 MeV. TIGRE employs solid-state detector technology, allowing dramatic improvements in spatial and energy resolutions over what is available using standard scintillation detectors. Over a several year mission, TIGRE would map the medium-energy gamma-ray sky with unprecendented detail, exploring sources of positron annihilation, nuclear line, and continuum emission.

The group at UCR is also active in the analysis and interpretation of data from various satellites, including the Compton Gamma Ray Observatory. The the CGRO Guest Investigator Program, we have explored the application of novel techniques for extracting scientifically interesting information from CGRO data. Two major results from these investigations, performed with collaborators at other institutions, have been the discovery of the "antimatter cloud" and the gamma-ray halo which appears to surround the Milky Way galaxy.

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Questions or problems: Contact Dave Dixon