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    Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT

    Access Status
    Fulltext not available
    Authors
    Abdo, A.
    Ackermann, M.
    Ajello, M.
    Anderson, B.
    Atwood, W.
    Axelsson, M.
    Baldini, L.
    Ballet, J.
    Barbiellini, G.
    Baring, M.
    Bastieri, D.
    Baughman, B.
    Bechtol, K.
    Bellazzini, R.
    Berenji, B.
    Bignami, G.
    Blandford, R.
    Bloom, E.
    Bonamente, E.
    Borgland, A.
    Bregeon, J.
    Brez, A.
    Brigida, M.
    Bruel, P.
    Burnett, T.
    Caliandro, G.
    Cameron, R.
    Caraveo, P.
    Casandjian, J.
    Cecchi, C.
    Celik, O.
    Chekhtman, A.
    Cheung, C.
    Chiang, J.
    Ciprini, S.
    Claus, R.
    Cohen-Tanugi, J.
    Conrad, J.
    Cutini, S.
    Dermer, C.
    de Angelis, A.
    De Luca, A.
    de Palma, F.
    Digel, S.
    Dormody, M.
    Do Couto e Silva, E.
    Drell, P.
    Dubois, R.
    Dumora, D.
    Farnier, C.
    Favuzzi, C.
    Fegan, S.
    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, I.
    Grondin, M.
    Grove, J.
    Guillemot, L.
    Guiriec, S.
    Gwon, C.
    Hanabata, Y.
    Harding, A.
    Hayashida, M.
    Hays, E.
    Hughes, R.
    Johannesson, G.
    Johnson, R.
    Johnson, T.
    Johnson, W.
    Kamae, T.
    Katagiri, H.
    Kataoka, J.
    Kawai, N.
    Kerr, M.
    Knödlseder, J.
    Kocian, M.
    Kuss, M.
    Lande, J.
    Latronico, L.
    Lemoine-Goumard, M.
    Longo, F.
    Loparco, F.
    Lott, B.
    Lovellette, M.
    Lubrano, P.
    Madejski, G.
    Makeev, A.
    Marelli, M.
    Mazziotta, M.
    McConville, W.
    McEnery, J.
    Meurer, C.
    Michelson, P.
    Mitthumsiri, W.
    Mizuno, T.
    Monte, C.
    Monzani, M.
    Morselli, A.
    Moskalenko, I.
    Murgia, S.
    Nolan, P.
    Norris, J.
    Nuss, E.
    Ohsugi, T.
    Omodei, N.
    Orlando, E.
    Ormes, J.
    Paneque, D.
    Parent, D.
    Pelassa, V.
    Pepe, M.
    Pesce-Rollins, M.
    Pierbattista, M.
    Piron, F.
    Porter, T.
    Primack, J.
    Raino, S.
    Rando, R.
    Ray, P.
    Razzano, M.
    Rea, N.
    Reimer, A.
    Reimer, O.
    Reposeur, T.
    Ritz, S.
    Rochester, L.
    Rodriguez, A.
    Romani, R.
    Ryde, F.
    Sadrozinski, H.
    Sanchez, D.
    Sander, A.
    Saz Parkinson, P.
    Scargle, J.
    Sgro, C.
    Siskind, E.
    Smith, D.
    Smith, P.
    Spandre, G.
    Spinelli, P.
    Starck, J.
    Strickman, M.
    Suson, D.
    Tajima, H.
    Takahashi, H.
    Takahashi, T.
    Tanaka, T.
    Thayer, J.
    Thompson, D.
    Tibaldo, L.
    Tibolla, Omar
    Torres, D.
    Tosti, G.
    Tramacere, A.
    Uchiyama, Y.
    Usher, T.
    Van Etten, A.
    Vasileiou, V.
    Vilchez, N.
    Vitale, V.
    Waite, A.
    Wang, P.
    Watters, K.
    Winer, B.
    Wolff, M.
    Wood, K.
    Ylinen, T.
    Ziegler, M.
    Date
    2009
    Type
    Journal Article
    
    Metadata
    Show full item record
    Citation
    Abdo, A. and Ackermann, M. and Ajello, M. and Anderson, B. and Atwood, W. and Axelsson, M. and Baldini, L. et al. 2009. Detection of 16 Gamma-Ray Pulsars Through Blind Frequency Searches Using the Fermi LAT. Science. 325: pp. 840-844.
    Source Title
    Science
    Additional URLs
    http://www.sciencemag.org/content/325/5942/840.full.pdf
    ISSN
    0036-8075
    URI
    http://hdl.handle.net/20.500.11937/5186
    Collection
    • Curtin Research Publications
    Abstract

    Pulsars are rapidly rotating, highly magnetized neutron stars emitting radiation across the electromagnetic spectrum. Although there are more than 1800 known radio pulsars, until recently only seven were observed to pulse in gamma rays, and these were all discovered at other wavelengths. The Fermi Large Area Telescope (LAT) makes it possible to pinpoint neutron stars through their gamma-ray pulsations. We report the detection of 16 gamma-ray pulsars in blind frequency searches using the LAT. Most of these pulsars are coincident with previously unidentified gamma-ray sources, and many are associated with supernova remnants. Direct detection of gamma-ray pulsars enables studies of emission mechanisms, population statistics, and the energetics of pulsar wind nebulae and supernova remnants.

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