Software timing calibration of the ARGO-YBJ detector

Details Software timing calibration of the ARGO-YBJ detector Software timing calibration of the ARGO-YBJ detector

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aph....30..287a&link_type=abstract

Astroparticle Physics, Volume 30, Issue 6, p. 287-292.

Physics

11

Extensive Air Showers, Time And Frequency

Scientific paper

The ARGO-YBJ experiment is mainly devoted to search for astronomical gamma sources. The arrival direction of air showers is reconstructed thanks to the times measured by the pixels of the detector. Therefore, the timing calibration of the detector pixels is crucial in order to get the best angular resolution and pointing accuracy. Because of the large number of pixels a hardware timing calibration is practically impossible. Therefore an off-line software calibration has been adopted. Here, the details of the procedure and the results are presented.

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