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| Fältnamn | Indikatorer | Metadata |
|---|---|---|
| 000 | 11330naa a2203109 4500 | |
| 001 | oai:DiVA.org:su-109246 | |
| 003 | SwePub | |
| 008 | 141117s2014 | |||||||||||000 ||eng| | |
| 024 | 7 | a https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-1092462 URI |
| 024 | 7 | a https://doi.org/10.1088/2041-8205/794/1/L12 DOI |
| 040 | a (SwePub)su | |
| 041 | a engb eng | |
| 042 | 9 SwePub | |
| 072 | 7 | a ref2 swepub-contenttype |
| 072 | 7 | a art2 swepub-publicationtype |
| 100 | 1 | a Abramowski, A.4 aut |
| 245 | 1 0 | a DISCOVERY OF THE HARD SPECTRUM VHE gamma-RAY SOURCE HESS J1641-463 |
| 264 | 1 | c 2014 |
| 338 | a print2 rdacarrier | |
| 500 | a AuthorCount:231; | |
| 520 | a 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. | |
| 650 | 7 | a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe |
| 650 | 7 | a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng |
| 653 | a cosmic rays | |
| 653 | a gamma rays: general | |
| 653 | a ISM: individual objects (SNR G338.3-0.0 | |
| 653 | a SNR G338.5+0.1) | |
| 700 | 1 | a Aharonian, F.4 aut |
| 700 | 1 | a Benkhali, F. Ait4 aut |
| 700 | 1 | a Akhperjanian, A. G.4 aut |
| 700 | 1 | a Uner, E. O. Ang4 aut |
| 700 | 1 | a Backes, M.4 aut |
| 700 | 1 | a Balenderan, S.4 aut |
| 700 | 1 | a Balzer, A.4 aut |
| 700 | 1 | a Barnacka, A.4 aut |
| 700 | 1 | a Becherini, Y.4 aut |
| 700 | 1 | a Tjus, J. Becker4 aut |
| 700 | 1 | a Berge, D.4 aut |
| 700 | 1 | a Bernhard, S.4 aut |
| 700 | 1 | a Bernloehr, K.4 aut |
| 700 | 1 | a Birsin, E.4 aut |
| 700 | 1 | a Biteau, J.4 aut |
| 700 | 1 | a Boettcher, M.4 aut |
| 700 | 1 | a Boisson, C.4 aut |
| 700 | 1 | a Bolmont, J.4 aut |
| 700 | 1 | a Bordas, P.4 aut |
| 700 | 1 | a Bregeon, J.4 aut |
| 700 | 1 | a Brun, F.4 aut |
| 700 | 1 | a Brun, P.4 aut |
| 700 | 1 | a Bryan, M.4 aut |
| 700 | 1 | a Bulik, T.4 aut |
| 700 | 1 | a Carrigan, S.4 aut |
| 700 | 1 | a Casanova, S.4 aut |
| 700 | 1 | a Chadwick, P. M.4 aut |
| 700 | 1 | a Chakraborty, N.4 aut |
| 700 | 1 | a Chalme-Calvet, R.4 aut |
| 700 | 1 | a Chaves, R. C. G.4 aut |
| 700 | 1 | a Chretien, M.4 aut |
| 700 | 1 | a Colafrancesco, S.4 aut |
| 700 | 1 | a Cologna, G.4 aut |
| 700 | 1 | a Conrad, Janu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)conrad |
| 700 | 1 | a Couturier, C.4 aut |
| 700 | 1 | a Cui, Y.4 aut |
| 700 | 1 | a Dalton, M.4 aut |
| 700 | 1 | a Davids, I. D.4 aut |
| 700 | 1 | a Degrange, B.4 aut |
| 700 | 1 | a Deil, C.4 aut |
| 700 | 1 | a deWilt, P.4 aut |
| 700 | 1 | a Djannati-Atai, A.4 aut |
| 700 | 1 | a Domainko, W.4 aut |
| 700 | 1 | a Donath, A.4 aut |
| 700 | 1 | a Drury, L. O 'C.4 aut |
| 700 | 1 | a Dubus, G.4 aut |
| 700 | 1 | a Dutson, K.4 aut |
| 700 | 1 | a Dyks, J.4 aut |
| 700 | 1 | a Dyrda, M.4 aut |
| 700 | 1 | a Edwards, T.4 aut |
| 700 | 1 | a Egberts, K.4 aut |
| 700 | 1 | a Eger, P.4 aut |
| 700 | 1 | a Espigat, P.4 aut |
| 700 | 1 | a Farnier, Christianu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)cfarn |
| 700 | 1 | a Fegan, S.4 aut |
| 700 | 1 | a Feinstein, F.4 aut |
| 700 | 1 | a Fernandes, M. V.4 aut |
| 700 | 1 | a Fernandez, D.4 aut |
| 700 | 1 | a Fiasson, A.4 aut |
| 700 | 1 | a Fontaine, G.4 aut |
| 700 | 1 | a Foerster, A.4 aut |
| 700 | 1 | a Fuessling, M.4 aut |
| 700 | 1 | a Gabici, S.4 aut |
| 700 | 1 | a Gajdus, M.4 aut |
| 700 | 1 | a Gallant, Y. A.4 aut |
| 700 | 1 | a Garrigoux, T.4 aut |
| 700 | 1 | a Giavitto, G.4 aut |
| 700 | 1 | a Giebels, B.4 aut |
| 700 | 1 | a Glicenstein, J. F.4 aut |
| 700 | 1 | a Gottschall, D.4 aut |
| 700 | 1 | a Grondin, M. -H4 aut |
| 700 | 1 | a Grudzinska, M.4 aut |
| 700 | 1 | a Hadasch, D.4 aut |
| 700 | 1 | a Haeffner, S.4 aut |
| 700 | 1 | a Hahn, J.4 aut |
| 700 | 1 | a Harris, J.4 aut |
| 700 | 1 | a Heinzelmann, G.4 aut |
| 700 | 1 | a Henri, G.4 aut |
| 700 | 1 | a Hermann, G.4 aut |
| 700 | 1 | a Hervet, O.4 aut |
| 700 | 1 | a Hillert, A.4 aut |
| 700 | 1 | a Hinton, J. A.4 aut |
| 700 | 1 | a Hofmann, W.4 aut |
| 700 | 1 | a Hofverberg, P.4 aut |
| 700 | 1 | a Holler, M.4 aut |
| 700 | 1 | a Horns, D.4 aut |
| 700 | 1 | a Ivascenko, A.4 aut |
| 700 | 1 | a Jacholkowska, A.4 aut |
| 700 | 1 | a Jahn, C.4 aut |
| 700 | 1 | a Jamrozy, M.4 aut |
| 700 | 1 | a Janiak, M.4 aut |
| 700 | 1 | a Jankowsky, F.4 aut |
| 700 | 1 | a Jung-Richardt, I.4 aut |
| 700 | 1 | a Kastendieck, M. A.4 aut |
| 700 | 1 | a Katarzynski, K.4 aut |
| 700 | 1 | a Katz, U.4 aut |
| 700 | 1 | a Kaufmann, S.4 aut |
| 700 | 1 | a Khelifi, B.4 aut |
| 700 | 1 | a Kieffer, M.4 aut |
| 700 | 1 | a Klepser, S.4 aut |
| 700 | 1 | a Klochkov, D.4 aut |
| 700 | 1 | a Kluzniak, W.4 aut |
| 700 | 1 | a Kolitzus, D.4 aut |
| 700 | 1 | a Komin, Nu.4 aut |
| 700 | 1 | a Kosack, K.4 aut |
| 700 | 1 | a Krakau, S.4 aut |
| 700 | 1 | a Krayzel, F.4 aut |
| 700 | 1 | a Krueger, P. P.4 aut |
| 700 | 1 | a Laffon, H.4 aut |
| 700 | 1 | a Lamanna, G.4 aut |
| 700 | 1 | a Lau, J.4 aut |
| 700 | 1 | a Lefaucheur, J.4 aut |
| 700 | 1 | a Lefranc, V.4 aut |
| 700 | 1 | a Lemiere, A.4 aut |
| 700 | 1 | a Lemoine-Goumard, M.4 aut |
| 700 | 1 | a Lenain, J. -P4 aut |
| 700 | 1 | a Lohse, T.4 aut |
| 700 | 1 | a Lopatin, A.4 aut |
| 700 | 1 | a Lu, C. -C4 aut |
| 700 | 1 | a Marandon, V.4 aut |
| 700 | 1 | a Marcowith, A.4 aut |
| 700 | 1 | a Marx, R.4 aut |
| 700 | 1 | a Maurin, G.4 aut |
| 700 | 1 | a Maxted, N.4 aut |
| 700 | 1 | a Mayer, M.4 aut |
| 700 | 1 | a McComb, T. J. L.4 aut |
| 700 | 1 | a Mehault, J.4 aut |
| 700 | 1 | a Meintjes, P. J.4 aut |
| 700 | 1 | a Menzler, U.4 aut |
| 700 | 1 | a Meyer, Manuelu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)mmanu |
| 700 | 1 | a Mitchell, A. M. W.4 aut |
| 700 | 1 | a Moderski, R.4 aut |
| 700 | 1 | a Mohamed, M.4 aut |
| 700 | 1 | a Morå, Knutu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)kdund |
| 700 | 1 | a Moulin, E.4 aut |
| 700 | 1 | a Murach, T.4 aut |
| 700 | 1 | a de Naurois, M.4 aut |
| 700 | 1 | a Niemiec, J.4 aut |
| 700 | 1 | a Nolan, S. J.4 aut |
| 700 | 1 | a Oakes, L.4 aut |
| 700 | 1 | a Odaka, H.4 aut |
| 700 | 1 | a Ohm, S.4 aut |
| 700 | 1 | a Opitz, B.4 aut |
| 700 | 1 | a Ostrowski, M.4 aut |
| 700 | 1 | a Oya, I.4 aut |
| 700 | 1 | a Panter, M.4 aut |
| 700 | 1 | a Parsons, R. D.4 aut |
| 700 | 1 | a Arribas, M. Paz4 aut |
| 700 | 1 | a Pekeur, N. W.4 aut |
| 700 | 1 | a Pelletier, G.4 aut |
| 700 | 1 | a Petrucci, P. -O4 aut |
| 700 | 1 | a Peyaud, B.4 aut |
| 700 | 1 | a Pita, S.4 aut |
| 700 | 1 | a Poon, H.4 aut |
| 700 | 1 | a Puehlhofer, G.4 aut |
| 700 | 1 | a Punch, M.4 aut |
| 700 | 1 | a Quirrenbach, A.4 aut |
| 700 | 1 | a Raab, S.4 aut |
| 700 | 1 | a Reichardt, I.4 aut |
| 700 | 1 | a Reimer, A.4 aut |
| 700 | 1 | a Reimer, O.4 aut |
| 700 | 1 | a Renaud, M.4 aut |
| 700 | 1 | a Reyes, R. de Los4 aut |
| 700 | 1 | a Rieger, F.4 aut |
| 700 | 1 | a Romoli, C.4 aut |
| 700 | 1 | a Rosier-Lees, S.4 aut |
| 700 | 1 | a Rowell, G.4 aut |
| 700 | 1 | a Rudak, B.4 aut |
| 700 | 1 | a Rulten, C. B.4 aut |
| 700 | 1 | a Sahakian, V.4 aut |
| 700 | 1 | a Salek, D.4 aut |
| 700 | 1 | a Sanchez, D. A.4 aut |
| 700 | 1 | a Santangelo, A.4 aut |
| 700 | 1 | a Schlickeiser, R.4 aut |
| 700 | 1 | a Schuessler, F.4 aut |
| 700 | 1 | a Schulz, A.4 aut |
| 700 | 1 | a Schwanke, U.4 aut |
| 700 | 1 | a Schwarzburg, S.4 aut |
| 700 | 1 | a Schwemmer, S.4 aut |
| 700 | 1 | a Sol, H.4 aut |
| 700 | 1 | a Spanier, F.4 aut |
| 700 | 1 | a Spengler, Gerritu Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)gspen |
| 700 | 1 | a Spies, F.4 aut |
| 700 | 1 | a Stawarz, L.4 aut |
| 700 | 1 | a Steenkamp, R.4 aut |
| 700 | 1 | a Stegmann, C.4 aut |
| 700 | 1 | a Stinzing, F.4 aut |
| 700 | 1 | a Stycz, K.4 aut |
| 700 | 1 | a Sushch, I.4 aut |
| 700 | 1 | a Tavernet, J. -P4 aut |
| 700 | 1 | a Tavernier, T.4 aut |
| 700 | 1 | a Taylor, A. M.4 aut |
| 700 | 1 | a Terrier, R.4 aut |
| 700 | 1 | a Tluczykont, M.4 aut |
| 700 | 1 | a Trichard, C.4 aut |
| 700 | 1 | a Valerius, K.4 aut |
| 700 | 1 | a Van Eldik, C.4 aut |
| 700 | 1 | a van Soelen, B.4 aut |
| 700 | 1 | a Vasileiadis, G.4 aut |
| 700 | 1 | a Veh, J.4 aut |
| 700 | 1 | a Venter, C.4 aut |
| 700 | 1 | a Viana, A.4 aut |
| 700 | 1 | a Vincent, P.4 aut |
| 700 | 1 | a Vink, J.4 aut |
| 700 | 1 | a Voelk, H. J.4 aut |
| 700 | 1 | a Volpe, F.4 aut |
| 700 | 1 | a Vorster, M.4 aut |
| 700 | 1 | a Vuillaume, T.4 aut |
| 700 | 1 | a Wagner, S. J.4 aut |
| 700 | 1 | a Wagner, P.4 aut |
| 700 | 1 | a Wagner, Robert M.u Stockholms universitet,Fysikum,Oskar Klein-centrum för kosmopartikelfysik (OKC)4 aut0 (Swepub:su)rwagner |
| 700 | 1 | a Ward, M.4 aut |
| 700 | 1 | a Weidinger, M.4 aut |
| 700 | 1 | a Weitzel, Q.4 aut |
| 700 | 1 | a White, R.4 aut |
| 700 | 1 | a Wierzcholska, A.4 aut |
| 700 | 1 | a Willmann, P.4 aut |
| 700 | 1 | a Woernlein, A.4 aut |
| 700 | 1 | a Wouters, D.4 aut |
| 700 | 1 | a Yang, R.4 aut |
| 700 | 1 | a Zabalza, V.4 aut |
| 700 | 1 | a Zaborov, D.4 aut |
| 700 | 1 | a Zacharias, M.4 aut |
| 700 | 1 | a Zdziarski, A. A.4 aut |
| 700 | 1 | a Zech, A.4 aut |
| 700 | 1 | a Zechlin, H. -S4 aut |
| 700 | 1 | a Fukui, Y.4 aut |
| 700 | 1 | a Sano, H.4 aut |
| 700 | 1 | a Fukuda, T.4 aut |
| 700 | 1 | a Yoshiike, S.4 aut |
| 710 | 2 | a Stockholms universitetb Fysikum4 org |
| 773 | 0 | t Astrophysical Journal Lettersg 794:1, s. L1-q 794:1<L1-x 2041-8205x 2041-8213 |
| 856 | 4 | u https://arxiv.org/abs/1408.5280y arXiv:1408.5280 |
| 856 | 4 8 | u https://urn.kb.se/resolve?urn=urn:nbn:se:su:diva-109246 |
| 856 | 4 8 | u https://doi.org/10.1088/2041-8205/794/1/L1 |
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- Abramowski, A.
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