2007/08/26 by The Tibet As Gamma Collaboration, The Tibet AS Gamma Collaboration, M. Amenomori +1
Physics and Astronomy · #Astrophysics (astro-ph) #Astrophysics and Cosmic Phenomena #FOS: Physical sciences #Neutrino Physics Research #Radiation Detection and Scintillator Technologies #astro-ph
paper · pdf · doi:10.48550/arxiv.0708.3462
4 pages, 3 figures, proceedings of 30th ICRC, International Cosmic Ray Conference 2007, Merida, Yucatan, Mexico, 3-11 July 2007
arxiv created 2007/08/26 · openalex publication_date 2007/08/26 · arxiv updated 2009/12/01 · openalex created_date 2025/10/10 · openalex updated_date 2026/07/28
We searched for pulsed gamma-ray emissions from the Crab pulsar using data of the Tibet-III air shower array from November 1999 through November 2005. No evidence for the pulsed emissions was found in our analysis. Upper limits at different energies were calculated for a 3 σ confidence level in the energy range of multi-TeV to several hundred TeV.