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Fermi large area telescope second source catalog

  • P. L. Nolan
  • , A. A. Abdo
  • , M. Ackermann
  • , M. Ajello
  • , A. Allafort
  • , E. Antolini
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , K. Bechtol
  • , A. Belfiore
  • , R. Bellazzini
  • , B. Berenji
  • , G. F. Bignami
  • , R. D. Blandford
  • , E. D. Bloom
  • , E. Bonamente
  • J. Bonnell, A. W. Borgland, E. Bottacini, A. Bouvier, T. J. Brandt, J. Bregeon, M. Brigida, P. Bruel, R. Buehler, T. H. Burnett, S. Buson, G. A. Caliandro, R. A. Cameron, R. Campana, B. Cañadas, A. Cannon, P. A. Caraveo, J. M. Casandjian, E. Cavazzuti, M. Ceccanti, C. Cecchi, Ö Çelik, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, R. Chipaux, S. Ciprini, R. Claus, J. Cohen-Tanugi, L. R. Cominsky, J. Conrad, R. Corbet, S. Cutini, F. D'Ammando, D. S. Davis, A. De Angelis, M. E. Decesar, M. Deklotz, A. De Luca, P. R. Den Hartog, F. De Palma, C. D. Dermer, S. W. Digel, E. Do Couto E Silva, P. S. Drell, A. Drlica-Wagner, R. Dubois, D. Dumora, T. Enoto, L. Escande, D. Fabiani, L. Falletti, C. Favuzzi, S. J. Fegan, E. C. Ferrara, W. B. Focke, P. Fortin, M. Frailis, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, N. Gehrels, S. Germani, B. Giebels, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, T. Glanzman, G. Godfrey, I. A. Grenier, M. H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, M. Gustafsson, D. Hadasch, Y. Hanabata, A. K. Harding, M. Hayashida, E. Hays, A. B. Hill, D. Horan, X. Hou, R. E. Hughes, G. Iafrate, R. Itoh, G. Jóhannesson, R. P. Johnson, T. E. Johnson, A. S. Johnson, T. J. Johnson, T. Kamae, H. Katagiri, J. Kataoka, J. Katsuta, N. Kawai, M. Kerr, J. Knödlseder, D. Kocevski, M. Kuss, J. Lande, D. Landriu, L. Latronico, M. Lemoine-Goumard, A. M. Lionetto, M. Llena Garde, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, M. Marelli, E. Massaro, M. N. Mazziotta, W. McConville, J. E. McEnery, J. Mehault, P. F. Michelson, M. Minuti, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, M. Mongelli, C. Monte, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, T. Nakamori, M. Naumann-Godo, J. P. Norris, E. Nuss, T. Nymark, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei, E. Orlando, J. F. Ormes, M. Ozaki, D. Paneque, J. H. Panetta, D. Parent, J. S. Perkins, M. Pesce-Rollins, M. Pierbattista, M. Pinchera, F. Piron, G. Pivato, T. A. Porter, J. L. Racusin, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, T. Reposeur, S. Ritz, L. S. Rochester, R. W. Romani, M. Roth, R. Rousseau, F. Ryde, H. F.W. Sadrozinski, D. Salvetti, D. A. Sanchez, P. M. Saz Parkinson, C. Sbarra, J. D. Scargle, T. L. Schalk, C. Sgrò, M. S. Shaw, C. Shrader, E. J. Siskind, D. A. Smith, G. Spandre, P. Spinelli, T. E. Stephens, M. S. Strickman, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, J. G. Thayer, J. B. Thayer, D. J. Thompson, L. Tibaldo, O. Tibolla, F. Tinebra, M. Tinivella, D. F. Torres, G. Tosti, E. Troja, Y. Uchiyama, J. Vandenbroucke, A. Van Etten, B. Van Klaveren, V. Vasileiou, G. Vianello, V. Vitale, A. P. Waite, E. Wallace, P. Wang, M. Werner, B. L. Winer, D. L. Wood, K. S. Wood, M. Wood, Z. Yang, S. Zimmer
  • Kavli Institute for Particle Astrophysics and Cosmology
  • George Mason University
  • Naval Research Laboratory
  • German Electron Synchrotron
  • National Institute for Nuclear Physics
  • University of Perugia
  • University of California at Santa Cruz
  • Stockholm University
  • Oskar Klein Centre
  • KTH Royal Institute of Technology
  • CEA-IRFU/CNRS/Université Paris Diderot
  • University of Trieste
  • University of Padua
  • University of Pavia
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • NASA Goddard Space Flight Center
  • University of Maryland
  • IRAP
  • Polytechnic University of Bari
  • École polytechnique
  • University of Washington
  • Campus UAB
  • University of Rome Tor Vergata
  • University College Dublin
  • Italian Space Agency
  • University of Maryland Baltimore County
  • Artep Inc
  • National Academy of Sciences
  • Service de Physique Théorique
  • ASI Science Data Center
  • Université Montpellier 2
  • Sonoma State University
  • National Institute for Astrophysics
  • University of Udine
  • Stellar Solutions Inc.
  • Centre d'Etudes Nucléaires Bordeaux-Gradingnan (CENBG)
  • Osservatorio Astronomico di Trieste
  • Hiroshima University
  • Max Planck Institute for Nuclear Physics
  • Heidelberg University 
  • Max Planck Institute for Radio Astronomy
  • University of Alabama in Huntsville
  • Kyoto University
  • University of Southampton
  • Ohio State University
  • University of Iceland
  • Ibaraki University
  • Waseda University
  • Tokyo Institute of Technology
  • RIKEN
  • University of Rome La Sapienza
  • Boise State University
  • JAXA Institute of Space and Astronautical Science
  • Max Planck Institute for Extraterrestrial Physics
  • University of Denver
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • Harvard & Smithsonian
  • Innsbruck Medical University
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Wyle Laboratories, Inc.
  • Purdue University Northwest
  • Nagoya University
  • University of Würzburg
  • ICREA
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • Praxis, Inc.

Research output: Contribution to journalArticlepeer-review

1263 Citations (Scopus)

Abstract

We present the second catalog of high-energy γ-ray sources detected by the Large Area Telescope (LAT), the primary science instrument on the Fermi Gamma-ray Space Telescope (Fermi), derived from data taken during the first 24months of the science phase of the mission, which began on 2008 August 4. Source detection is based on the average flux over the 24month period. The second Fermi-LAT catalog (2FGL) includes source location regions, defined in terms of elliptical fits to the 95% confidence regions and spectral fits in terms of power-law, exponentially cutoff power-law, or log-normal forms. Also included are flux measurements in five energy bands and light curves on monthly intervals for each source. Twelve sources in the catalog are modeled as spatially extended. We provide a detailed comparison of the results from this catalog with those from the first Fermi-LAT catalog (1FGL). Although the diffuse Galactic and isotropic models used in the 2FGL analysis are improved compared to the 1FGL catalog, we attach caution flags to 162 of the sources to indicate possible confusion with residual imperfections in the diffuse model. The 2FGL catalog contains 1873 sources detected and characterized in the 100MeV to 100GeV range of which we consider 127 as being firmly identified and 1171 as being reliably associated with counterparts of known or likely γ-ray-producing source classes.

Original languageEnglish
Article number31
JournalAstrophysical Journal, Supplement Series
Volume199
Issue number2
DOIs
Publication statusPublished - Apr 2012
Externally publishedYes

Keywords

  • catalogs
  • gamma rays: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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