HAL : in2p3-00023668, version 1
 arXiv : astro-ph/0501512
 Astronomy and Astrophysics 432 (2005) L9-L12
 Search for TeV emission from the region around PSR B1706-44 with the H.E.S.S. experiment
 HESS Collaboration(s)
 (2005)
 The region around PSR B1706-44 has been observed with the H.E.S.S. imaging atmospheric Cherenkov telescopes in 2003. No evidence for gamma-ray emission in the TeV range was found at the pulsar position or at the radio arc which corresponds to the supernova remnant G 343.1-2.3. The 99% confidence level flux upper limit at the pulsar position is Ful(E > 350GeV) = 1.4e-12 /cm^2/s assuming a power law with photon index of 2.5 and Ful(E > 500GeV) = 1.3e-12 /cm^2/s without an assumption on the spectral shape. The reported upper limits correspond to 8% of the flux from an earlier detection by the CANGAROO experiment.
 Thème(s) : Physique/Astrophysique/Cosmologie et astrophysique extra-galactiquePlanète et Univers/Astrophysique
 Mot(s)-clé(s) : Gamma rays: observations – ISM: individual objects: PSR B1706-44 – ISM: supernova remnants – ISM: individual objects: G 343.1-2.3
 Lien vers le texte intégral : http://fr.arXiv.org/abs/astro-ph/0501512
 in2p3-00023668, version 1 http://hal.in2p3.fr/in2p3-00023668 oai:hal.in2p3.fr:in2p3-00023668 Contributeur : Simone Lantz <> Soumis le : Jeudi 9 Novembre 2006, 10:25:19 Dernière modification le : Jeudi 9 Novembre 2006, 10:31:34