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Conferences
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ICN-UNAM
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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
572
false
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129 (7A)
1
Poster
Search for Pulsed VHE Gamma-Ray Emission from Pulsars with H.E.S.S.
Mr.
Humboldt University Berlin
7e8d1108d560d9aa791efb299614ae4e
Mr.
Humboldt University Berlin
7e8d1108d560d9aa791efb299614ae4e
Mr.
CERN
23fcbb9a9641637952b5609b385cec19
Mr.
Universite de Geneve
e0697301aff1c96dafe63b2f8c29cf2e
Mr.
Australia Telescope National Facility
88de9661ce3828ae2b9a270efcb41077
Mr.
University of Chicago
f7a6889034bfdf98bcfd31661c7c954d
Mr.
Humboldt University Berlin
d4a235cd11a425ba44c0fc3b48402ed5
Mr.
University of Erlangen-Nuremberg
dad1346926165d23a27428a4418b8601
Mr.
North-West University, Potchefstroom
663e5be255603ebb00ecd47d17afe730
Merida, Mexico
Regency (Hyatt)
2007-07-06T14:45:00
2007-07-06T14:45:00
We present recent results of a search for pulsed very-high-energy (VHE) gamma-ray
emission from pulsars using data taken with the High Energy Stereoscopic System
(H.E.S.S.), an array of imaging Cherenkov telescopes located in Namibia. The data
set, accumulated during four years of operation until 2006, comprises observations of
eleven young pulsars, selected according to their spin-down luminosity relative to
distance, and two millisecond pulsars. No evidence for pulsed emission was found in
any data set and differential upper limits on pulsed energy flux were derived, and
compared to a variety of model predictions on VHE gamma-ray emission from the
vicinity of pulsar magnetospheres.
paper
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link
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1
More information about the venue
http://www.icrc2007.unam.mx/
link
http://www.icrc2007.unam.mx/
doc
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word file
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