Passer à la navigation principale Passer à la recherche Passer au contenu principal

A search for very high energy γ-ray emission from the starburst galaxy NGC253 with HESS

  • F. Aharonian
  • , A. G. Akhperjanian
  • , A. R. Bazer-Bachi
  • , M. Beilicke
  • , W. Benbow
  • , D. Berge
  • , K. Bernlöhr
  • , C. Boisson
  • , O. Bolz
  • , V. Borrel
  • , I. Braun
  • , F. Breitling
  • , A. M. Brown
  • , P. M. Chadwick
  • , L. M. Chounet
  • , R. Cornils
  • , L. Costamante
  • , B. Degrange
  • , H. J. Dickinson
  • , A. Djannati-Ataï
  • L. O.C. Drury, G. Dubus, D. Emmanoulopoulos, P. Espigat, F. Feinstein, G. Fontaine, Y. Fuchs, S. Funk, Y. A. Gallant, B. Giebels, S. Gillessen, J. F. Glicenstein, P. Goret, C. Hadjichrisüdis, M. Hauser, G. Heinzelmann, G. Henri, G. Hermann, J. A. Hinton, W. Hofmann, M. Holleran, D. Horns, A. Jacholkowska, O. C. de Jager, B. Khélifi, N. Komin, A. Konopelko, I. J. Latham, R. le Gallou, A. Lemière, M. Lemoine-Goumard, N. Leroy, T. Lohse, J. M. Martin, O. Martineau-Huynh, A. Marcowith, C. Masterson, T. J.L. McComb, M. de Naurois, S. J. Nolan, A. Noutsos, K. J. Orford, J. L. Osborne, M. Ouchrif, M. Panter, G. Pelletier, S. Pita, G. Pühlhofer, M. Punch, B. C. Raubenheimer, M. Raue, J. Raux, S. M. Rayner, A. Reimer, O. Reimer, J. Ripken, L. Rob, L. Rolland, G. Rowell, V. Sahakian, L. Saugé, S. Schlenker, R. Schlickeiser, C. Schuster, U. Schwanke, M. Siewert, H. Sol, D. Spangler, R. Steenkamp, C. Stegmann, J. P. Tavernet, R. Terrier, C. G. Théoret, M. Tluczykont, G. Vasileiadis, C. Venter, P. Vincent, H. J. Völk, S. J. Wagner
  • Max-Planck-Institut für Kernphysik
  • Yerevan Physics Institute
  • CNRS
  • Universität Hamburg
  • Institut für Physik
  • Humboldt-Universität zu Berlin
  • Sorbonne Univ.
  • Department of Physics
  • Durham University
  • Ip Paris
  • European Associated Laboratory for Gamma-Ray Astronomy
  • Astroparticule and Cosmol APC
  • Dublin Institute for Advanced Studies
  • Landessternwarte Heidelberg
  • Laboratoire Univers et Particules de Montpellier
  • Institut Pierre Simon Laplace, CNRS and CEA
  • Unit for Space Physics
  • North-West University
  • Universités Paris VI and VII
  • Institut für Theoretische Physik
  • Ruhr-University Bochum
  • Charles University
  • University of Namibia

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

27 Citations (Scopus)

Résumé

We present the result of 28 h of observations of the nearby starburst galaxy NGC 253 with the HESS detector in 2003. We find no evidence for very high energy y-ray emission from this object. Gamma-ray emission above 400 GeV from NGC 253 had been reported by the CANGAROO collaboration in 2002. From the HESS data we derive upper limits on the flux above 300 GeV of 1.9 × 10 -12 photons cm-2 s-1 for a point-like source and 6.3 × 10-12 photons cm-2 s-1 for a source of radius 0.5° as reported by CANGAROO, both at a confidence level of 99%. These upper limits are inconsistent with the spectrum reported by CANGAROO. The expected very high energy γ-ray emission from this object is discussed in the framework of a galactic wind propagation model.

langue originaleAnglais
Pages (de - à)177-183
Nombre de pages7
journalAstronomy and Astrophysics
Volume442
Numéro de publication1
Les DOIs
étatPublié - 1 janv. 2005
Modification externeOui

Empreinte digitale

Examiner les sujets de recherche de « A search for very high energy γ-ray emission from the starburst galaxy NGC253 with HESS ». Ensemble, ils forment une empreinte digitale unique.

Contient cette citation