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  Upper limits to the SN1006 multi-TeV gamma-ray flux from H.E.S.S. observations

Aharonian, F., Akhperjanian, A. G., Aye, K.-M., Bazer-Bachi, A. R., Beilicke, M., Benbow, W., et al. (2005). Upper limits to the SN1006 multi-TeV gamma-ray flux from H.E.S.S. observations. Astronomy & Astrophysics, 437(1), 135-139. doi:10.1051/0004-6361:20042522.

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Aharonian, F.1, Author           
Akhperjanian, A. G.1, Author           
Aye, K.-M.2, Author
Bazer-Bachi, A. R.2, Author
Beilicke, M.1, Author           
Benbow, W.1, Author           
Berge, D.1, Author           
Berghaus, P.2, Author
Bernlöhr, K.1, Author           
Bolz, O.1, Author           
Boisson, C:2, Author
Borgmeier, C.2, Author
Breitling, F.2, Author
Brown, A. M.2, Author
Bussons Gordo, J.2, Author
Chadwick, P. M.2, Author
Chounet, L.-M.2, Author
Cornils, R.1, Author           
Costamante, L.1, Author           
Degrange, B.2, Author
Djannati-Atai, A.1, Author           Drury, L.O'C.2, AuthorErgin, T.2, AuthorEspigat, P.2, AuthorFeinstein, F.1, Author           Fleury, P.2, AuthorFontaine, G.2, AuthorFunk, S.1, Author           Gallant, Y. A.1, Author           Giebels, B.2, AuthorGillessen, S.1, Author           Goret, P.2, AuthorDubus, G.1, Author           Hadjichristidis, C.2, AuthorHauser, M.2, AuthorHeinzelmann, G.2, AuthorHenri, G.2, AuthorHermann, G.1, Author           Hinton, J. A.1, Author           Hofmann, W.1, Author           Holleran, M.2, AuthorHorns, D.1, Author           de Jager, O. C.2, AuthorJung, I.1, Author           Khélifi, B.1, Author           Komin, N.2, AuthorKonopelko, A.3, Author           Latham, I. J.2, AuthorLe Gallou, R.2, AuthorLemoine, M.2, AuthorLemière, A.2, AuthorLeroy, N.2, AuthorLohse, T.2, AuthorMarcowith, A.2, AuthorMasterson, C.1, Author           McComb, T. J. L.2, Authorde Naurois, M.1, Author           Nolan, S. J.2, AuthorNoutsos, A.2, AuthorOrford, K. J.1, Author           Osborne, J. L.1, Author           Ouchrif, M.2, AuthorPanter, M.1, Author           Pelletier, G.2, AuthorPita, S.2, AuthorFuchs, Y.2, AuthorPühlhofer, G.1, Author           Punch, M.2, AuthorRaubenheimer, B. C.2, AuthorRaue, M.1, Author           Raux, J.2, AuthorRayner, S. M.2, AuthorRedondo, I.2, AuthorReimer, A.2, AuthorReimer, O.2, AuthorRipken, J.2, Authorvan der Walt, D.J.2, AuthorRob, L.2, AuthorRolland, L.2, AuthorRowell, G.1, Author           Sahakian, V.2, AuthorSaugé, L.1, Author           Schlenker, S.2, AuthorSchlickeiser, R.2, AuthorSchuster, C.2, AuthorSchwanke, U.2, AuthorSiewert, M.2, AuthorSol, H.2, AuthorSteenkamp, R.2, AuthorStegmann, C.2, AuthorTavernet, J.-P.2, AuthorThéoret, C. G.2, AuthorTluczykont, M.2, AuthorVenter, C.2, AuthorVasileiadis, G.1, Author           Vincent, P.2, AuthorVisser, B.2, AuthorVölk, H. J.3, Author           Wagner, S. J.2, Author more..
Affiliations:
1Division Prof. Dr. Werner Hofmann, MPI for Nuclear Physics, Max Planck Society, ou_904550              
2Yerevan Physics Institute, Armenia University of Durham, Department of Physics, UK Centre d'Etudes Spatiales des Rayonnements, CNRS/UPS Toulouse, France Universität Hamburg, Institut für Experimentalphysik, Germany Physique Corpusculaire et Cosmologie, IN2P3/CNRS, Collège de France, Paris, France Institut für Physik, Humboldt-Universität zu Berlin, Germany LUTH, UMR 8102 du CNRS, Observatoire de Paris, Section de Meudon, France Groupe d'astroparticules de Montpellier, IN2P3/CNRS, Université Montpellier II, France Laboratoire de Physique Nucléaire et de Hautes Energies, IN2P3/CNRS, Universités Paris VI & VII, Jussieu, France European Associated Laboratory for Gamma-Ray Astronomy, jointly supported by CNRS and MPG Laboratoire Leprince-Ringuet, IN2P3/CNRS, Ecole Polytechnique, Palaiseau, France Dublin Institute for Advanced Studies, Ireland Service d'Astrophysique. DAPNIA/DSM/CEA, CE Saclay, Gif-sur-Yvette, France Landessternwarte, Königstuhl, Heidelberg, Germany Laboratoire d'Astrophysique de Grenoble, INSU/CNRS, Université Joseph Fourier, France Unit for Space Physics, North-West University, Potchefstroom, South Africa Institut für theoretische Physik, Lehrstuhl IV, Ruhr-Universität Bochum, Germany Institute of Particle and Nuclear Physics, Charles University, Prague, Czech Republic University of Namibia, Windhoek, Namibia, ou_persistent22              
3Prof. Heinrich J. Völk, Emeriti, MPI for Nuclear Physics, Max Planck Society, ou_907548              

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Free keywords: gamma rays: observations -- ISM: supernova remnants
 Abstract: Observations of the shell-type supernova remnant SN1006 have been carried out with the HESS system of Cherenkov telescopes during 2003 (18.2 h with two operating telescopes) and 2004 (6.3 h with all four telescopes). No evidence for TeV gamma-ray emission from any compact or extended region associated with the remnant is seen and resulting upper limits at the 99.9% confidence level are up to a factor 10 lower than previously-published fluxes from CANGAROO. For SN1006 at its current epoch of evolution we define limits for a number of important global parameters. Upper limits on the gamma-ray luminosity (for E = 0.26 to 10 TeV, distance d = 2 kpc) of Lγ < 1.7 x 1033 erg s-1, and the total energy in corresponding accelerated protons, Wp < 1.6 x 1050 erg are estimated (for proton energies Ep 1.5 to 60 TeV and assuming the lowest value n = 0.05 cm-3 of the ambient target density discussed in literature). Extending this estimate to cover the range of proton energies observed in the cosmic ray spectrum up to the knee (we take here Ep 1 GeV to 3 PeV, assuming a differential particle index -2) gives Wp < 6.3 x 1050 erg. A lower limit on the post-shock magnetic field of B > 25μG results when considering the synchrotron/inverse-Compton framework for the observed X-ray flux and γ -ray upper limits.

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Language(s): eng - English
 Dates: 2005-07-01
 Publication Status: Issued
 Pages: -
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 Table of Contents: -
 Rev. Type: -
 Identifiers: eDoc: 236923
DOI: 10.1051/0004-6361:20042522
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Title: Astronomy & Astrophysics
  Alternative Title : A&A
Source Genre: Journal
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Pages: - Volume / Issue: 437 (1) Sequence Number: - Start / End Page: 135 - 139 Identifier: -