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SUMMARY:Observations of extended VHE gamma-ray emission from MSH 15-52 wit
 h CANGAROO-III
DTSTART;VALUE=DATE-TIME:20070704T174100Z
DTEND;VALUE=DATE-TIME:20070704T175300Z
DTSTAMP;VALUE=DATE-TIME:20260810T110137Z
UID:indico-contribution-422@cern.ch
DESCRIPTION:Speakers: Mr. NAKAMORI\, Takeshi (Kyoto University)\nThe gamma
 -ray pulsar PSR B1509-58\, surrounded by the supernova remnant \nMSH15-\n5
 2\, was expected to be a Very High Energy gamma-ray source. CANGAROO-I 3.8
 \nm telescope reported a marginal detection of VHE gamma-rays above 1.9 Te
 V \nand\nrecently H.E.S.S. detected an extended signal along with the puls
 ar jets\, from\nsub-TeV to tens of TeV.\n\n We observed MSH15-52 using CAN
 GAROO-III imaging atmospheric Cherenkov\ntelescope array located in South 
 Australia\, from April to June in 2006. We\nalso detected gamma-rays above
  860GeV with more than 5 sigma level during \nan\neffective exposure of 48
 .4 hours. Obtained differential flux of VHE gamma-ray\nis consistent with 
 that of H.E.S.S.\, and its morphology shows an extended\nemission compared
  to our PSF.\n\nhttps://indico.nucleares.unam.mx/event/4/session/5/contrib
 ution/422
LOCATION:Merida\, Mexico Uxmal + Tulum (Holiday Inn)
URL:https://indico.nucleares.unam.mx/event/4/session/5/contribution/422
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