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Detection of 16 gamma-ray pulsars through blind frequency searches using the Fermi LAT

  • A. A. Abdo
  • , M. Ackermann
  • , M. Ajello
  • , B. Anderson
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , M. G. Baring
  • , D. Bastieri
  • , B. M. Baughman
  • , K. Bechtol
  • , R. Bellazzini
  • , B. Berenji
  • , G. F. Bignami
  • , R. D. Blandford
  • , E. D. Bloom
  • , E. Bonamente
  • , A. W. Borgland
  • J. Bregeon, A. Brez, M. Brigida, P. Bruel, T. H. Burnett, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, J. M. Casandjian, C. Cecchi, Ö Çelik, A. Chekhtman, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. Conrad, S. Cutini, C. D. Dermer, A. De Angelis, A. De Luca, F. De Palma, S. W. Digel, M. Dormody, E. Do Couto E Silva, P. S. Drell, R. Dubois, D. Dumora, C. Farnier, C. Favuzzi, S. J. Fegan, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, B. Giebels, N. Giglietto, P. Giommi, F. Giordano, T. Glanzman, G. Godfrey, I. A. Grenier, M. H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, C. Gwon, Y. Hanabata, A. K. Harding, M. Hayashida, E. Hays, R. E. Hughes, G. Jóhannesson, R. P. Johnson, T. J. Johnson, W. N. Johnson, T. Kamae, H. Katagiri, J. Kataoka, N. Kawai, M. Kerr, J. Knödlseder, M. L. Kocian, M. Kuss, J. Lande, L. Latronico, M. Lemoine-Goumard, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, A. Makeev, M. Marelli, M. N. Mazziotta, W. McConville, J. E. McEnery, C. Meurer, P. F. Michelson, W. Mitthumsiri, T. Mizuno, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, P. L. Nolan, J. P. Norris, E. Nuss, T. Ohsugi, N. Omodei, E. Orlando, J. F. Ormes, D. Paneque, D. Parent, V. Pelassa, M. Pepe, M. Pesce-Rollins, M. Pierbattista, F. Piron, T. A. Porter, J. R. Primack, S. Rainò, R. Rando, P. S. Ray, M. Razzano, N. Rea, A. Reimer, O. Reimer, T. Reposeur, S. Ritz, L. S. Rochester, A. Y. Rodriguez, R. W. Romani, F. Ryde, H. F.W. Sadrozinski, D. Sanchez, A. Sander, P. M. Saz Parkinson, J. D. Scargle, C. Sgrò, E. J. Siskind, D. A. Smith, P. D. Smith, G. Spandre, P. Spinelli, J. L. Starck, M. S. Strickman, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, J. G. Thayer, D. J. Thompson, L. Tibaldo, O. Tibolla, D. F. Torres, G. Tosti, A. Tramacere, Y. Uchiyama, T. L. Usher, A. Van Etten, V. Vasileiou, N. Vilchez, V. Vitale, A. P. Waite, P. Wang, K. Watters, B. L. Winer, M. T. Wolff, K. S. Wood, T. Ylinen, M. Ziegler
  • Naval Research Laboratory
  • Kavli Institute for Particle Astrophysics and Cosmology
  • Santa Cruz Institute for Particle Physics
  • Oskar Klein Centre
  • Stockholm University
  • Sezione di Pisa
  • Université Paris Diderot
  • Istituto Nazionale di Fisica Nucleare, Sezione di Trieste
  • Università di Trieste
  • Rice University
  • Sezione di Padova
  • Università di Padova
  • The Ohio State University
  • Istituto Universitario di Studi Superiori
  • Sezione di Perugia
  • Università di Perugia
  • Dell'Università e Del Politecnico di Bari
  • Istituto Nazionale di Fisica Nucleare, Sezione di Bari
  • Laboratoire Leprince-Ringuet
  • University of Washington
  • INAF-Istituto di Astrofisica Spaziale e Fisica Cosmica
  • NASA/Goddard Space Flight Center
  • George Mason University
  • Laboratoire Univers et Particules de Montpellier
  • AlbaNova
  • Agenzia Spaziale Italiana
  • Università di Udine
  • Université Bordeaux 1
  • Université Victor Segalen Bordeaux II
  • Hiroshima University
  • University of Maryland, College Park
  • University of Alabama in Huntsville
  • Waseda University
  • Institute of Physical and Chemical Research (RIKEN)
  • Institute of Science Tokyo
  • CNRS Centre National de la Recherche Scientifique
  • Sezione di Roma Tor Vergata
  • University of Denver
  • Max-Planck Institut für extraterrestrische Physik
  • University of Amsterdam
  • Universitat Autònoma de Barcelona
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Purdue University Calumet
  • Japan Aerospace Exploration Agency
  • Max-Planck-Institut for Nuclear Physics
  • Institució Catalana de Recerca i Estudis Avançats
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Maryland, Baltimore County (UMBC)
  • Università di Roma Tor Vergata
  • University of Kalmar

Research output: Contribution to journalArticlepeer-review

342 Citations (Scopus)

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.

Original languageEnglish
Pages (from-to)840-844
Number of pages5
JournalScience
Volume325
Issue number5942
DOIs
Publication statusPublished - 2009
Externally publishedYes

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