FERMI/LARGE AREA TELESCOPE BRIGHT GAMMA-RAY SOURCE LIST

Abdo, Aa; Ackermann, M; Ajello, M; Atwood, Wb; Axelsson, M; Baldini, Luca; Ballet, J; Band, Dl; Barbiellini, G; Bastieri, D; Battelino, M; Baughman, Bm; Bechtol, K; Bellazzini, R; Berenji, B; Bignami, Gf; Blandford, Rd; Bloom, Ed; Bonamente, E; Borgland, Aw; Bouvier, A; Bregeon, J; Brez, A; Brigida, M; Bruel, P; Burnett, Th; Caliandro, Ga; Cameron, Ra; Caraveo, Pa; Casandjian, Jm; Cavazzuti, E; Cecchi, C; Charles, E; Chekhtman, A; Cheung, Cc; Chiang, J; Ciprini, S; Claus, R; Cohen Tanugi, J; Cominsky, Lr; Conrad, J; Corbet, R; Costamante, L; Cutini, S; Davis, Ds; Dermer, Cd; de Angelis, A; de Luca, A; de Palma, F; Digel, Sw; Dormody, M; Silva, Ede; Drell, Ps; Dubois, R; Dumora, D; Farnier, C; Favuzzi, C; Fegan, Sj; Ferrara, Ec; Focke, Wb; Frailis, M; Fukazawa, Y; Funk, S; Fusco, P; Gargano, F; Gasparrini, D; Gehrels, N; Germani, S; Giebels, B; Giglietto, N; Giommi, P; Giordano, F; Glanzman, T; Godfrey, G; Grenier, Ia; Grondin, Mh; Grove, Je; Guillemot, L; Guiriec, S; Hanabata, Y; Harding, Ak; Hartman, Rc; Hayashida, M; Hays, E; Healey, Se; Horan, D; Hughes, Re; Johannesson, G; Johnson, As; Johnson, Rp; Johnson, Tj; Johnson, Wn; Kamae, T; Katagiri, H; Kataoka, J; Kawai, N; Kerr, M; Knodlseder, J; Kocevski, D; Kocian, Ml; Komin, N; Kuehn, F; Kuss, M; Lande, J; Latronico, L; Lee, Sh; Lemoine Goumard, M; Longo, F; Loparco, F; Lott, B; Lovellette, Mn; Lubrano, P; Madejski, Gm; Makeev, A; Marelli, M; Mazziotta, Mn; Mcconville, W; Mcenery, Je; Mcglynn, S; Meurer, C; Michelson, Pf; Mitthumsiri, W; Mizuno, T; Moiseev, Aa; Monte, C; Monzani, Me; Moretti, E; Morselli, A; Moskalenko, Iv; Murgia, S; Nakamori, T; Nolan, Pl; Norris, Jp; Nuss, E; Ohno, M; Ohsugi, T; Omodei, N; Orlando, E; Ormes, Jf; Ozaki, M; Paneque, D; Panetta, Jh; Parent, D; Pelassa, V; Pepe, M; Pesce Rollins, M; Piron, F; Porter, Ta; Poupard, L; Raino, S; Rando, R; Ray, Ps; Razzano, Massimiliano; Rea, N; Reimer, A; Reimer, O; Reposeur, T; Ritz, S; Rochester, Ls; Rodriguez, Ay; Romani, Rw; Roth, M; Ryde, F; Sadrozinski, Hfw; Sanchez, D; Sander, A; Parkinson, Pms; Scargle, Jd; Schalk, Tl; Sellerholm, A; Sgro, C; Shaw, Ms; Shrader, C; Sierpowska Bartosik, A; Siskind, Ej; Smith, Da; Smith, Pd; Spandre, G; Spinelli, P; Starck, Jl; Stephens, Te; Strickman, Ms; Strong, Aw; Suson, Dj; Tajima, H; Takahashi, H; Takahashi, T; Tanaka, T; Thayer, Jb; Thayer, Jg; Thompson, Dj; Tibaldo, L; Tibolla, O; Torres, Df; Tosti, G; Tramacere, A; Uchiyama, Y; Usher, Tl; Van Etten, A; Vilchez, N; Vitale, V; Waite, Ap; Wallace, E; Wang, P; Watters, K; Winer, Bl; Wood, Ks; Ylinen, T; Ziegler, M.

doi:10.1088/0067-0049/183/1/46

Following its launch in 2008 June, the Fermi Gamma-ray Space Telescope (Fermi) began a sky survey in August. The Large Area Telescope (LAT) on Fermi in three months produced a deeper and better resolved map of the γ-ray sky than any previous space mission. We present here initial results for energies above 100 MeV for the 205 most significant (statistical significance greater than ~10σ) γ-ray sources in these data. These are the best characterized and best localized point-like (i.e., spatially unresolved) γ-ray sources in the early mission data.