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Diffuse Galactic gamma-ray emission with H.E.S.S.
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Abramowski, A.
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Aharonian, F.
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Ait Benkhali, F.
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Akhperjanian, A. G.
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Angüner, E. O.
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Backes, M.
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Balenderan, S.
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Balzer, A.
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Barnacka, Anna [SAP14011957]
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Becherini, Y.
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Becker Tjus, J.
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Berge, D.
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Bernhard, S.
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Bernlöhr, K.
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Birsin, E.
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Biteau, J.
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Böttcher, M.
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Boisson, C.
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Bolmont, J.
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Bordas, P.
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Bregeon, J.
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Brun, F.
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Brun, P.
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Bryan, M.
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Bulik, T.
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Carrigan, S.
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Casanova, S.
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Chadwick, P. M.
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Chakraborty, N.
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Chalme-Calvet, R.
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Chaves, R. C. G.
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Chrétien, M.
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Colafrancesco, S.
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Cologna, G.
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Conrad, J.
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Couturier, C.
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Cui, Y.
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Davids, I. D.
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Degrange, B.
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Deil, C.
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deWilt, P.
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Djannati-Ataï, A.
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Domainko, W.
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Donath, A.
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Drury, L. O’C.
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Dubus, G.
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Dutson, K.
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Dyks, J.
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Dyrda, M.
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Edwards, T.
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Egberts, K.
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Eger, P.
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Espigat, P.
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Farnier, C.
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Fegan, S.
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Feinstein, F.
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Fernandes, M. V.
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Fernandez, D.
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Fiasson, A.
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Fontaine, G.
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Förster, A.
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Füßling, M.
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Gabici, S.
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Gajdus, M.
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Gallant, Y. A.
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Garrigoux, T.
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Giavitto, G.
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Giebels, B.
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Glicenstein, J. F.
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Gottschall, D.
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Grondin, M.-H.
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Grudzińska, M.
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Hadasch, D.
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Häffner, S.
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Hahn, J.
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Harris, J.
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Heinzelmann, G.
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Henri, G.
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Hermann, G.
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Hervet, O.
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Hillert, A.
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Hinton, J. A.
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Hofmann, W.
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Hofverberg, P.
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Holler, M.
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Horns, D.
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Ivascenko, A.
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Jacholkowska, A.
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Jahn, C.
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Jamrozy, Marek [SAP11016371]
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Janiak, M.
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Jankowsky, F.
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Jung-Richardt, I.
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Kastendieck, M. A.
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Katarzyński, K.
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Katz, U.
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Kaufmann, S.
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Khélifi, B.
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Kieffer, M.
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Klepser, S.
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Klochkov, D.
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Kluźniak, W.
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Kolitzus, D.
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Komin, Nu.
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Kosack, K.
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Krakau, S.
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Krayzel, F.
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Krüger, P. P.
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Laffon, H.
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Lamanna, G.
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Lefaucheur, J.
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Lefranc, V.
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Lemière, A.
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Lemoine-Goumard, M.
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Lenain, J.-P.
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Lohse, T.
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Lopatin, A.
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Lu, C.-C.
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Marandon, V.
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Marcowith, A.
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Marx, R.
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Maurin, G.
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Maxted, N.
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Mayer, M.
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McComb, T. J. L.
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Méhault, J.
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Meintjes, P. J.
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Menzler, U.
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Meyer, M.
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Mitchell, A. M. W.
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Moderski, R.
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Mohamed, M.
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Morå, K.
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Moulin, E.
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Murach, T.
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de Naurois, M.
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Niemiec, J.
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Nolan, S. J.
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Oakes, L.
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Odaka, H.
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Ohm, S.
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Opitz, B.
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Ostrowski, Michał [SAP11009779]
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Oya, I.
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Panter, M.
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Parsons, R. D.
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Paz Arribas, M.
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Pekeur, N. W.
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Pelletier, G.
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Petrucci, P.-O.
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Peyaud, B.
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Pita, S.
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Poon, H.
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Pühlhofer, G.
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Punch, M.
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Quirrenbach, A.
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Raab, S.
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Reichardt, I.
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Reimer, A.
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Reimer, O.
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Renaud, M.
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de los Reyes, R.
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Rieger, F.
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Romoli, C.
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Rosier-Lees, S.
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Rowell, G.
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Rudak, B.
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Rulten, C. B.
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Sahakian, V.
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Salek, D.
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Sanchez, D. A.
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Santangelo, A.
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Schlickeiser, R.
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Schüssler, F.
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Schulz, A.
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Schwanke, U.
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Schwarzburg, S.
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Schwemmer, S.
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Sol, H.
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Spanier, F.
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Spengler, G.
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Spies, F.
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Stawarz, Łukasz [SAP11018649]
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Steenkamp, R.
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Stegmann, C.
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Stinzing, F.
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Stycz, K.
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Sushch, I.
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Tavernet, J.-P.
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Tavernier, T.
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Taylor, A. M.
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Terrier, R.
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Tluczykont, M.
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Trichard, C.
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Valerius, K.
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van Eldik, C.
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van Soelen, B.
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Vasileiadis, G.
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Veh, J.
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Venter, C.
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Viana, A.
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Vincent, P.
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Vink, J.
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Völk, H. J.
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Volpe, F.
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Vorster, M.
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Vuillaume, T.
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Wagner, S. J.
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Wagner, P.
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Wagner, R. M.
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Ward, M.
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Weidinger, M.
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Weitzel, Q.
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White, R.
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Wierzcholska, Alicja [USOS30589]
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Willmann, P.
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Wörnlein, A.
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Wouters, D.
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Yang, R.
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Zabalza, V.
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Zaborov, D.
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Zacharias, M.
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Zdziarski, A. A.
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Zech, A.
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Zechlin, H.-S.
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Fukui, Y.
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dc.date.accessioned
2015-04-25T09:20:05Z
dc.date.available
2015-04-25T09:20:05Z
dc.date.issued
2014
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dc.identifier.issn
1550-7998
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dc.identifier.uri
http://ruj.uj.edu.pl/xmlui/handle/item/5739
dc.language
eng
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dc.title
Diffuse Galactic gamma-ray emission with H.E.S.S.
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dc.type
JournalArticle
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dc.abstract.en
Diffuse $\gamma$-ray emission is the most prominent observable signature of celestial cosmic-ray interactions at high energies. While already being investigated at GeVenergies over several decades, assessments of diffuse $\gamma$-ray emission at TeVenergies remain sparse. After completion of the systematic survey of the inner Galaxy, the H.E.S.S. experiment is in a prime position to observe large-scale diffuse emission at TeVenergies. Data of the H.E.S.S. Galactic Plane Survey are investigated in regions off known $\gamma$-ray sources. Corresponding $\gamma$-ray flux measurements were made over an extensive grid of celestial locations. Longitudinal and latitudinal profiles of the observed $\gamma$-ray fluxes show characteristic excess emission not attributable to known $\gamma$-ray sources. For the first time large-scale $\gamma$-ray emission along the Galactic plane using imaging atmospheric Cherenkov telescopes has been observed. While the background subtraction technique limits the ability to recover modest variation on the scale of the H.E.S.S. field of view or larger, which is characteristic of the inverse Compton scatter-induced Galactic diffuse emission, contributions of neutral pion decay as well as emission from unresolved $\gamma$-ray sources can be recovered in the observed signal to a large fraction. Calculations show that the minimum $\gamma$-ray emission from $\pi^{0}$ decay represents a significant contribution to the total signal. This detection is interpreted as a mix of diffuse Galactic $\gamma$-ray emission and unresolved sources
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dc.description.volume
90
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dc.description.number
12
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dc.identifier.doi
10.1103/PhysRevD.90.122007
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dc.identifier.eissn
1550-2368
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dc.title.journal
Physical Review. D, Particles, Fields, Gravitation, and Cosmology
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dc.contributor.institution
H.E.S.S. Collaboration
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dc.language.container
eng
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dc.affiliation
Wydział Fizyki, Astronomii i Informatyki Stosowanej : Instytut – Obserwatorium Astronomiczne
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dc.subtype
Article
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dc.identifier.articleid
122007
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dc.rights.original
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[2014 A]: 35
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