Fermi Large Area Telescope observations of the Vela-X Pulsar Wind Nebula
- Abdo, A.A.
- Ackermann, Markus
- Ajello, Marco
- Allafort, A.
- Baldini, Luca
- Ballet, Jean
- Barbiellini, Guido
- Bastieri, D.
- Bechtol, K.
- Bellazzini, R.
- Berenji, B.
- D. Blandford, R.
- D. Bloom, E.
- Bonamente, E.
- W. Borgland, A.
- Bouvier, A.
- Bregeon, J.
- Brez, A.
- Brigida, M.
- Bruel, Pascal
- H. Burnett, T.
- Buson, S.
- A. Caliandro, G.
- A. Cameron, R.
- Caraveo, P. A.
- Carrigan, S.
- M. Casandjian, J.
- Cecchi, C.
- Celik, O.
- Chekhtman, A.
- C. Chung, C.
- Chiang, J.
- Ciprini, S.
- Claus, R.
- Cohen-Tanugi, J.
- Conrad, J.
- de Angelis, A.
- de Palma, F.
- Dormody, M.
- Do Couto E Silva, E.
- S. Drell, P.
- Dubois, R.
- Dumora, D.
- Farnier, C.
- Favuzzi, C.
- J. Fegan, S.
- B. Focke, W.
- Fortin, P.
- Frailis, M.
- Fukazawa, Y.
- Funk, S.
- Fusco, P.
- Gargano, F.
- Gehrels, N.
- Germani, S.
- Giavitto, G.
- Giglietto, N.
- Giordano, F.
- Glanzman, T.
- Godfrey, G.
- A. Grenier, I.
- Grondin, M.-H.
- E. Grove, J.
- Guillemot, L.
- Guiriec, S.
- K. Harding, A.
- Hayashida, M.
- Hays, E.
- Horan, D.
- E. Hughes, R.
- S. Jackson, M.
- Johannesson, G.
- S. Johnson, A.
- J. Johnson, T.
- N. Johnson, W.
- Johnston, S.
- Kamae, T.
- Katagiri, H.
- Kataoka, J.
- Kawai, N.
- Kerr, M.
- Knödlseder, Jürgen
- Kuss, M.
- Lande, J.
- Latronico, L.
- Lee, S.-H.
- Lemoine-Goumard, M.
- Llena Garde, M.
- Longo, F.
- Loparco, F.
- Lott, B.
- N. Lovellette, M.
- Lubrano, P.
- Makeev, A.
- Marelli, M.
- N. Mazziotta, M.
- E. Mcenery, J.
- Meurer, C.
- F. Michelson, P.
- Mitthumsiri, W.
- Mizuno, T.
- A. Moiseev, A.
- Monte, C.
- E. Monzani, M.
- Morselli, A.
- V. Moskalenko, I.
- Murgia, S.
- Nakamori, T.
- L. Nolan, P.
- P. Norris, J.
- Noutsos, A.
- Nuss, E.
- Ohsugi, T.
- Omodei, N.
- Orlando, E.
- F. Ormes, J.
- Ozaki, M.
- Paneque, D.
- H. Panetta, J.
- Parent, D.
- Pelassa, V.
- Pepe, M.
- Pesce-Rollins, M.
- Pierbattista, M.
- Piron, F.
- Porter, T.A.
- Raino, S.
- Rando, R.
- S. Ray, P.
- Rea, N.
- Reimer, A.
- Reimer, O.
- Reposeur, T.
- Ritz, S.
- Y. Rodriguez, A.
- W. Romani, R.
- Roth, M.
- Ryde, F.
- F.-W. Sadrozinski, H.
- Sanchez, D.
- Sander, A.
- M. Saz Parkinson, P.
- D. Scargle, J.
- Sgro, C.
- J. Siskind, E.
- Smith, David Stanley
- D. Smith, P.
- Spandre, G.
- Spinelli, P.
- S. Strickman, M.
- J. Suson, D.
- Tajima, H.
- Takahashi, H.
- Takahashi, T.
- Tanaka, T.
- B. Thayer, J.
- G. Thayer, J.
- J. Thompson, D.
- Tibaldo, L.
- F. Torres, D.
- Tosti, G.
- Tramacere, A.
- Uchiyama, Y.
- L. Usher, T.
- van Etten, A.
- Vasileiou, V.
- Venter, C.
- Vilchez, N.
- Vitale, V.
- P. Waite, A.
- Wang, P.
- Weltevrede, P.
- L. Winer, B.
- S. Wood, K.
- Ylinen, T.
- Ziegler, M.
DOIAbstract
21 pages, 5 figures, accepted for publication in Astrophysical JournalWe report on gamma-ray observations in the off-pulse window of the Vela pulsar PSR B0833-45, using 11 months of survey data from the Fermi Large Area Telescope (LAT). This pulsar is located in the 8 degree diameter Vela supernova remnant, which contains several regions of non-thermal emission detected in the radio, X-ray and gamma-ray bands. The gamma-ray emission detected by the LAT lies within one of these regions, the 2*3 degrees area south of the pulsar known as Vela-X. The LAT flux is signicantly spatially extended with a best-fit radius of 0.88 +/- 0.12 degrees for an assumed radially symmetric uniform disk. The 200 MeV to 20 GeV LAT spectrum of this source is well ...
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