4
Conferences
false
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ICN-UNAM
1482bc95ee34f0461176da21871284c8
3
icrc2007@icrc2007.unam.mx
30th International Cosmic Ray Conference
The 30th International Cosmic Ray Conference will be held from July 3, 2007 to July 11, 2007 in Merida, Yucatan, Mexico.
True
Merida, Mexico
2007-07-03T08:00:00
2007-07-11T19:00:00
2005-09-26T05:04:53
2024-04-12T17:46:55
Mexico/General
Dr.
IGeof-UNAM
40af9343b8bb9d18708b4f0252d5f53c
286
false
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0
Oral
Localising the H.E.S.S. Galactic Centre point source
MPI for Nuclear Physics
71253470a03cf83e752f0c81f80a3ed5
MPI for Nuclear Physics
71253470a03cf83e752f0c81f80a3ed5
MPI for Nuclear Physics
d41d8cd98f00b204e9800998ecf8427e
MPI for Nuclear Physics
d41d8cd98f00b204e9800998ecf8427e
MPI for Nuclear Physics
d41d8cd98f00b204e9800998ecf8427e
University of Leeds
d41d8cd98f00b204e9800998ecf8427e
MPI for Nuclear Physics
d41d8cd98f00b204e9800998ecf8427e
Merida, Mexico
Uxmal + Tulum (Holiday Inn)
2007-07-04T08:54:00
2007-07-04T09:06:00
00:12
The detection of TeV gamma-rays from the direction of the Galactic Centre is one of
the most exciting discoveries in recent years. Observations by the H.E.S.S. system of
imaging atmospheric Cherenkov telescopes provide the most precise available data on
this source in the energy range 150 GeV - 30 TeV. The vicinity of the kinetic centre
of our galaxy harbours numerous objects which could potentially accelerate particles
to very high energies and thus produce the gamma-ray flux observed. The
centre-of-gravity of the point-like emission measured by H.E.S.S. is in good
agreement with the position of the supermassive black hole Sgr A* and the recently
discovered PWN G359.95-0.04. Given a systematic pointing error of about 30'', a
possible association with the SNR Sgr A East could not be ruled out with data
available from 2004. In this contribution an update is given on the position of the
H.E.S.S. Galactic Centre source using 2005/2006 data. The systematic pointing error
is significantly reduced using guiding telescopes for pointing corrections, making it
possible to exclude with high significance Sgr A East as the source of the TeV
gamma-rays.
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1
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http://www.icrc2007.unam.mx/
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