MAGIC - Roadmap to a standard analysis

Details MAGIC - Roadmap to a standard analysis MAGIC - Roadmap to a standard analysis

Feb 2005

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005aipc..745..730b&link_type=abstract

HIGH ENERGY GAMMA-RAY ASTRONOMY: 2nd International Symposium on High Energy Gamma-Ray Astronomy. AIP Conference Proceedings, Vo

Astronomy and Astrophysics

Astronomy

13

Gamma-Ray Sources, Gamma-Ray Bursts, X- And Gamma-Ray Telescopes And Instrumentation

Scientific paper

The current generation of Imaging Air Cerenkov Telescopes takes data at a rate of up to 1 kHz requiring a maximum storage rate of 30 MB/s or 1.8 GB/h. Processing these data necessarily involves a lot of automatisation and optimisation of the software. This enforces the development of a stand-alone standard analysis. The final goal is having highly compressed output which can be provided as the full-physics input to a more dedicated analysis by collaborators or guest observers.

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