Probing the extent of the non-thermal emission from the Vela X region at TeV energies with H.E.S.S
- Abramowski, A.
- Acero, Fabio
- Aharonian, F.
- Akhperjanian, A. G.
- Anton, G.
- Balenderan, S.
- Balzer, Agnès
- Barnacka, A.
- Becherini, Y.
- Tjus, J. Becker
- Bernlöhr, K.
- Birsin, E.
- Biteau, J.
- Bochow, A.
- Boisson, C.
- Bolmont, J.
- Bordas, P.
- Brucker, J.
- Brun, F.
- Brun, P.
- Bulik, T.
- Carrigan, S.
- Casanova, S.
- Cerruti, M.
- Chadwick, P. M.
- Charbonnier, A.
- Chaves, R. C. G.
- Cheesebrough, A.
- Cologna, G.
- Conrad, J.
- Couturier, C.
- Dalton, M.
- Daniel, M. K.
- Davids, I. D.
- Degrange, B.
- Deil, C.
- Dewilt, P.
- Dickinson, H. J.
- Djannati-Ataï, A.
- Domainko, W.
- Drury, L. O'C.
- Dubois, F.
- Dubus, G.
- Dutson, K.
- Dyks, J.
- Dyrda, M.
- Egberts, K.
- Eger, P.
- Espigat, P.
- Fallon, L.
- Farnier, C.
- Fegan, S.
- Feinstein, F.
- Fernandes, M. V.
- Fernandez, D.
- Fiasson, A.
- Fontaine, G.
- Förster, A.
- Ling, M. Füss
- Gajdus, M.
- Gallant, Y. A.
- Garrigoux, T.
- Gast, H.
- Giebels, B.
- Glicenstein, J. F.
- Glück, B.
- Göring, D.
- Grondin, M. -H.
- Häffner, S.
- Hague, J. D.
- Hahn, J.
- Hampf, D.
- Harris, J.
- Heinz, S.
- Heinzelmann, G.
- Henri, G.
- Hermann, G.
- Hillert, A.
- Hinton, J. A.
- Hofmann, W.
- Hofverberg, P.
- Holler, M.
- Horns, D.
- Jacholkowska, A.
- Jahn, C.
- Jamrozy, M.
- Jung, I.
- Kastendieck, M. A.
- Ski, K. Katarzyń
- Katz, U.
- Kaufmann, S.
- Khélifi, B.
- Klochkov, D.
- Niak, W. Kluź
- Kneiske, T.
- Komin, Nu.
- Kosack, K.
- Kossakowski, R.
- Krayzel, F.
- Krüger, P. P.
- Laffon, H.
- Lamanna, G.
- Lenain, J. -P.
- Lennarz, D.
- Lohse, T.
- Lopatin, A.
- Lu, C. -C.
- Marandon, V.
- Marcowith, Alexandre
- Masbou, Julien
- Maurin, G.
- Maxted, N.
- Mayer, M.
- Mccom, T. J. L.
- Medina, M. C.
- Méhault, J.
- Menzler, U.
- Moderski, R.
- Mohamed, M.
- Moulin, Emmanuel
- Naumann, C. L.
- Naumann-Godo, M.
- Denaurois, M.
- Nedbal, D.
- Nguyen, N.
- Niemiec, J.
- Nolan, S. J.
- Ohm, S.
- Awilhelmi, E. Deoñ
- Opitz, B.
- Ostrowski, M.
- Oya, I.
- Panter, M.
- Parsons, D.
- Pazarribas, M.
- Pekeur, N. W.
- Pelletier, G.
- Perez, J.
- Petrucci, P. -O.
- Peyaud, B.
- Pita, S.
- Pühlhofer, G.
- Punch, M.
- Quirrenbach, A.
- Raue, M.
- Reimer, A.
- Reimer, O.
- Renaud, Matthieu
- Delosreyes, R.
- Rieger, F.
- Ripken, J.
- Rob, L.
- Rosier-Lees, S.
- Rowell, G.
- Rudak, B.
- Rulten, C. B.
- Sahakian, V.
- Sanchez, D. A.
- Santangelo, A.
- Schlickeiser, R.
- Schulz, A.
- Schwanke, U.
- Schwarzburg, S.
- Schwemmer, S.
- Sheidaei, F.
- Skilton, J. L.
- Sol, H.
- Spengler, G.
- Stawarz, L.
- Steenkamp, R.
- Stegmann, C.
- Stinzing, F.
- Stycz, K.
- Sushch, I.
- Szostek, A.
- Tavernet, J. -P.
- Terrier, R.
- Tluczykont, M.
- Trichard, C.
- Valerius, K.
- Vaneldik, C.
- Vasileiadis, George
- Venter, C.
- Viana, A.
- Vincent, P.
- Völk, H. J.
- Volpe, F.
- Vorobiov, S.
- Vorster, M.
- Wagner, S. J.
- Ward, M.
- White, R.
- Wierzcholska, A.
- Wouters, D.
- Zacharias, M.
- Zajczyk, A.
- Zdziarski, A. A.
- Zech, A.
- Zechlin, H. -S.
DOIAbstract
Vela X is a region of extended radio emission in the western part of the Vela constellation: one of the nearest pulsar wind nebulae (PWNe), and associated with the energetic Vela pulsar (PSR B0833-45). Extended very-high-energy (VHE) $\gamma$-ray emission (HESS $\mathrm{J0835\mhyphen 455}$) was discovered using the H.E.S.S. experiment in 2004. The VHE $\gamma$-ray emission was found to be coincident with a region of X-ray emission discovered with ${\it ROSAT}$ above 1.5 keV (the so-called \textit{Vela X cocoon}): a filamentary structure extending southwest from the pulsar to the centre of Vela X. A deeper observation of the entire Vela X nebula region, also including larger offsets from the cocoon, has been performed with H.E.S.S. This re-o...
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