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  • Abramowski, A.Univ Hamburg (author)

Discovery of the Hard Spectrum VHE γ-Ray Source HESS J1641–463

  • Article/chapterEnglish2014

Publisher, publication year, extent ...

  • 2014
  • printrdacarrier

Numbers

  • LIBRIS-ID:oai:DiVA.org:lnu-38154
  • https://urn.kb.se/resolve?urn=urn:nbn:se:lnu:diva-38154URI
  • https://doi.org/10.1088/2041-8205/794/1/L1DOI

Supplementary language notes

  • Language:English
  • Summary in:English

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  • Subject category:ref swepub-contenttype
  • Subject category:art swepub-publicationtype

Notes

  • This Letter reports the discovery of a remarkably hard spectrum source, HESS J1641-463, by the High Energy Stereoscopic System (H.E.S.S.) in the very high energy (VHE) domain. HESS J1641-463 remained unnoticed by the usual analysis techniques due to confusion with the bright nearby source HESS J1640-465. It emerged at a significance level of 8.5 standard deviations after restricting the analysis to events with energies above 4 TeV. It shows a moderate flux level of phi(E > 1TeV) = (3.64 +/- 0.44(stat)+/- 0.73(sys)) x 10(-13) cm(-2) s(-1), corresponding to 1.8% of the Crab Nebula flux above the same energy, and a hard spectrum with a photon index of Gamma = 2.07 +/- 0.11(stat)+/- 0.20(sys). It is a point-like source, although an extension up to a Gaussian width of sigma = 3 arcmin cannot be discounted due to uncertainties in the H.E.S.S. point-spread function. The VHE gamma-ray flux of HESS J1641-463 is found to be constant over the observed period when checking time binnings from the year-by-year to the 28 minute exposure timescales. HESS J1641-463 is positionally coincident with the radio supernova remnant SNR G338.5+0.1. No X-ray candidate stands out as a clear association; however, Chandra and XMM-Newton data reveal some potential weak counterparts. Various VHE gamma-ray production scenarios are discussed. If the emission from HESS J1641-463 is produced by cosmic ray protons colliding with the ambient gas, then their spectrum must extend close to 1 PeV. This object may represent a source population contributing significantly to the galactic cosmic ray flux around the knee.

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  • Aharonian, F.Max Planck Inst Kernphys, Heidelberg, Germany (author)
  • Benkhali, F. AitMax Planck Inst Kernphys, Heidelberg, Germany (author)
  • Akhperjanian, A. G.Natl Acad Sci Republ Armenia (author)
  • Uner, E. O. AngHumboldt Univ (author)
  • Backes, M.Univ Namibia (author)
  • Balenderan, S.Univ Durham (author)
  • Balzer, A.Univ Amsterdam (author)
  • Barnacka, A.Uniwersytet Jagiello, Poland (author)
  • Becherini, YvonneLinnéuniversitetet,Institutionen för fysik och elektroteknik (IFE)(Swepub:lnu)yvbeaa (author)
  • Tjus, J. Becker (author)
  • Berge, D. (author)
  • Bernhard, S. (author)
  • Bernloehr, K. (author)
  • Birsin, E. (author)
  • Biteau, J. (author)
  • Boettcher, M. (author)
  • Boisson, C. (author)
  • Bolmont, J. (author)
  • Bordas, P. (author)
  • Bregeon, J. (author)
  • Brun, F. (author)
  • Brun, P. (author)
  • Bryan, M. (author)
  • Bulik, T. (author)
  • Carrigan, S. (author)
  • Casanova, S. (author)
  • Chadwick, P. M. (author)
  • Chakraborty, N. (author)
  • Chalme-Calvet, R. (author)
  • Chaves, R. C. G. (author)
  • Chretien, M. (author)
  • Colafrancesco, S. (author)
  • Cologna, G. (author)
  • Conrad, J. (author)
  • Couturier, C. (author)
  • Cui, Y. (author)
  • Dalton, M. (author)
  • Davids, I. D. (author)
  • Degrange, B. (author)
  • Deil, C. (author)
  • deWilt, P. (author)
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  • Oya, I. (author)
  • Panter, M. (author)
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  • Arribas, M. Paz (author)
  • Pekeur, N. W. (author)
  • Pelletier, G. (author)
  • Petrucci, P. -O (author)
  • Peyaud, B. (author)
  • Pita, S. (author)
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  • Punch, MichaelUniv Paris Diderot, APC, AstroParticule & Cosmology, CNRS,IN2P3,CEA,Irfu, Observ Paris,Sorbonne Paris C, 10 Rue Alice Domon & Leonie Duquet, F-75205 Paris 13, France(Swepub:lnu)mipuaa (author)
  • Quirrenbach, A. (author)
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  • Sahakian, V. (author)
  • Salek, D. (author)
  • Sanchez, D. A. (author)
  • Santangelo, A. (author)
  • Schlickeiser, R. (author)
  • Schuessler, F. (author)
  • Schulz, A. (author)
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  • Zacharias, M. (author)
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  • Zechlin, H. -S (author)
  • Fukui, Y. (author)
  • Sano, H. (author)
  • Fukuda, T. (author)
  • Yoshiike, S. (author)
  • Univ HamburgMax Planck Inst Kernphys, Heidelberg, Germany (creator_code:org_t)

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  • In:Astrophysical Journal Letters794:1, s. Article ID: L1-2041-82052041-8213

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