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  <organization>ICN-UNAM</organization>
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<supportEmail caption="Support">icrc2007@icrc2007.unam.mx</supportEmail>
<title>30th International Cosmic Ray Conference</title>
<description>The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.</description>
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 <name>Merida, Mexico</name>
 <address></address>
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<startDate>2007-07-03T08:00:00</startDate>
<endDate>2007-07-11T19:00:00</endDate>
<creationDate>2005-09-26T05:04:53</creationDate>
<modificationDate>2024-04-12T17:46:55</modificationDate>
<timezone>Mexico/General</timezone>
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  <organization>IGeof-UNAM</organization>
  <emailHash>40af9343b8bb9d18708b4f0252d5f53c</emailHash>
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 <title>Seven-year observation of multi-TeV gamma rays from the Crab Nebula with the Tibet air shower array</title>
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   <title>Dr.</title>
   <name first="Masato" middle="" last="Takita"></name>
   <organization>Institute for Cosmic Ray Research, University of Tokyo</organization>
   <emailHash>ae6f048c38d706fb9ac09a9affcec3b4</emailHash>
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   <title>Dr.</title>
   <name first="Munehiro" middle="" last="Ohnishi"></name>
   <organization>Institute for Cosmic Ray Research, University of Tokyo</organization>
   <emailHash>59c4ab92e8fbf631c4670d29fcce4257</emailHash>
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  <user>
   <title>Dr.</title>
   <name first="Masato" middle="" last="Takita"></name>
   <organization>Institute for Cosmic Ray Research, University of Tokyo</organization>
   <emailHash>ae6f048c38d706fb9ac09a9affcec3b4</emailHash>
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  <name>Merida, Mexico</name>
  <address></address>
  <room>Regency (Hyatt)</room>
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 <startDate>2007-07-06T14:45:00</startDate>
 <endDate>2007-07-06T14:45:00</endDate>
 <abstract>The Tibet air shower array, consisting of 533 scintillation counters
which are placed in a lattice with 7.5 m spacing, has been in
operation since 1999 at Yangbajing in Tibet, China at an altitude of
4,300 m above sea level.  In this conference, we will report on the
continuous observation of multi-TeV gamma rays from the Crab Nebula
with the Tibet air shower array.  We found no evidence for time
variability of flux intensity from the Crab Nebula at multi-TeV
energies.  Also the gamma-ray energy spectrum of the Crab Nebula is
consistent with our previous results and other observations by the
atmospheric imaging Cherenkov telescopes.  In addition, we will discuss
our systematic errors, such as the stability in pointing accuracy,
angular resolution and the absolute energy scale error, which have
been checked by monitoring the Moon's shadow in the cosmic-ray flux.</abstract>
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