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Fermi large area telescope first source catalog

  • A. A. Abdo
  • , M. Ackermann
  • , M. Ajello
  • , A. Allafort
  • , E. Antolini
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , B. M. Baughman
  • , K. Bechtol
  • , R. Bellazzini
  • , F. Belli
  • , B. Berenji
  • , D. Bisello
  • , R. D. Blandford
  • , E. D. Bloom
  • , E. Bonamente
  • J. Bonnell, A. W. Borgland, A. Bouvier, J. Bregeon, A. Brez, M. Brigida, P. Bruel, T. H. Burnett, G. Busetto, S. Buson, G. A. Caliandro, R. A. Cameron, R. Campana, B. Canadas, P. A. Caraveo, S. Carrigan, J. M. Casandjian, E. Cavazzuti, M. Ceccanti, C. Cecchi, Ö Çelik, E. Charles, A. Chekhtman, C. C. Cheung, J. Chiang, A. N. Cillis, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. Conrad, R. Corbet, D. S. Davis, M. Deklotz, P. R. Den Hartog, 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, D. Fabiani, C. Farnier, 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, G. Giavitto, 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, S. E. Healey, A. B. Hill, D. Horan, R. E. Hughes, G. Iafrate, G. Jóhannesson, A. S. Johnson, R. P. Johnson, T. J. Johnson, W. N. Johnson, T. Kamae, H. Katagiri, J. Kataoka, N. Kawai, M. Kerr, J. Knödlseder, D. Kocevski, M. Kuss, J. Lande, D. Landriu, L. Latronico, S. H. Lee, M. Lemoine-Goumard, A. M. Lionetto, M. Llena Garde, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, A. Makeev, B. Marangelli, M. Marelli, E. Massaro, M. N. Mazziotta, W. McConville, J. E. McEnery, P. F. Michelson, M. Minuti, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, M. Mongelli, C. Monte, M. E. Monzani, E. Moretti, A. Morselli, I. V. Moskalenko, S. Murgia, H. Nakajima, T. Nakamori, M. Naumann-Godo, P. L. Nolan, J. P. Norris, E. Nuss, M. Ohno, T. Ohsugi, N. Omodei, E. Orlando, J. F. Ormes, M. Ozaki, A. Paccagnella, D. Paneque, J. H. Panetta, D. Parent, V. Pelassa, M. Pepe, M. Pesce-Rollins, M. Pinchera, F. Piron, T. A. Porter, L. Poupard, S. Rainò, R. Rando, P. S. Ray, M. Razzano, S. Razzaque, N. Rea, A. Reimer, O. Reimer, T. Reposeur, J. Ripken, S. Ritz, L. S. Rochester, A. Y. Rodriguez, R. W. Romani, M. Roth, H. F.W. Sadrozinski, D. Salvetti, D. Sanchez, A. Sander, P. M. Saz Parkinson, J. D. Scargle, T. L. Schalk, G. Scolieri, C. Sgrò, M. S. Shaw, E. J. Siskind, D. A. Smith, P. D. Smith, G. Spandre, P. Spinelli, J. L. Starck, T. E. Stephens, E. Striani, M. S. Strickman, A. W. Strong, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, J. B. Thayer, J. G. Thayer, D. J. Thompson, L. Tibaldo, O. Tibolla, F. Tinebra, D. F. Torres, G. Tosti, A. Tramacere, Y. Uchiyama, T. L. Usher, A. Van Etten, V. Vasileiou, N. Vilchez, V. Vitale, A. P. Waite, E. Wallace, P. Wang, K. Watters, B. L. Winer, K. S. Wood, Z. Yang, T. Ylinen, M. Ziegler
  • Naval Research Laboratory
  • National Research Council
  • Kavli Institute for Particle Astrophysics and Cosmology
  • National Institute for Nuclear Physics
  • University of Perugia
  • University of California at Santa Cruz
  • Stockholm University
  • Lund University
  • Oskar Klein Centre
  • CEA-IRFU/CNRS/Université Paris Diderot
  • University of Trieste
  • University of Padua
  • Ohio State University
  • University of Rome Tor Vergata
  • NASA Goddard Space Flight Center
  • University of Maryland
  • Polytechnic University of Bari
  • École polytechnique
  • University of Washington
  • Autonomous University of Barcelona
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Italian Space Agency
  • University of Maryland Baltimore County
  • George Mason University
  • Universidad de Buenos Aires
  • Université Montpellier 2
  • Stellar Solutions Inc.
  • University of Udine
  • University of Pavia
  • IN2P3 - Institut National de Physique Nucléaire et de Physique Des Particules
  • Université de Bordeaux
  • Osservatorio Astronomico di Trieste
  • Hiroshima University
  • National Institute for Astrophysics
  • Max Planck Institute for Radio Astronomy
  • University of Alabama in Huntsville
  • ICREA
  • Université Grenoble Alpes
  • Waseda University
  • Tokyo Institute of Technology
  • RIKEN
  • CNRS
  • University of Rome La Sapienza
  • University of Denver
  • JAXA Institute of Space and Astronautical Science
  • Max Planck Institute for Extraterrestrial Physics
  • Innsbruck Medical University
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Universities Space Research Association
  • Purdue University Northwest
  • University of Würzburg
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Geneva
  • KTH Royal Institute of Technology
  • Linnaeus University

Research output: Contribution to journalArticlepeer-review

1022 Citations (Scopus)

Abstract

We present a catalog of high-energy gamma-ray sources detected by the Large Area Telescope (LAT), the primary science instrument on the Fermi Gamma-ray Space Telescope (Fermi), during the first 11 months of the science phase of the mission, which began on 2008 August 4. The First Fermi-LAT catalog (1FGL) contains 1451 sources detected and characterized in the 100MeV to 100GeV range. Source detection was based on the average flux over the 11 month period, and the threshold likelihood Test Statistic is 25, corresponding to a significance of just over 4σ. The 1FGL catalog includes source location regions, defined in terms of elliptical fits to the 95% confidence regions and power-law spectral fits as well as flux measurements in five energy bands for each source. In addition, monthly light curves are provided. Using a protocol defined before launch we have tested for several populations of gamma-ray sources among the sources in the catalog. For individual LAT-detected sources we provide firm identifications or plausible associations with sources in other astronomical catalogs. Identifications are based on correlated variability with counterparts at other wavelengths, or on spin or orbital periodicity. For the catalogs and association criteria that we have selected, 630 of the sources are unassociated. Care was taken to characterize the sensitivity of the results to the model of interstellar diffuse gamma-ray emission used to model the bright foreground, with the result that 161 sources at low Galactic latitudes and toward bright local interstellar clouds are flagged as having properties that are strongly dependent on the model or as potentially being due to incorrectly modeled structure in the Galactic diffuse emission.

Original languageEnglish
Pages (from-to)405-436
Number of pages32
JournalAstrophysical Journal, Supplement Series
Volume188
Issue number2
DOIs
Publication statusPublished - 2010
Externally publishedYes

Keywords

  • Catalogs
  • Gamma rays: general

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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