Software timing calibration of the ARGO-YBJ detector

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59 Citazioni (Scopus)


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 calibratin of the detector pixels is crucial in ordere to get the best angular resolution abd pointing accuracy. Because of the large number of pixels a hardware timing calibration is practically impossible. Therefore, an off-line software calibration. Here, the details of the procedure and the results are presented.
Lingua originaleEnglish
pagine (da-a)287-292
Numero di pagine6
RivistaAstroparticle Physics
Stato di pubblicazionePublished - 2008

All Science Journal Classification (ASJC) codes

  • Astronomy and Astrophysics

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