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The second catalog of active galactic nuclei detected by the Fermi large area telescope

  • M. Ackermann
  • , M. Ajello
  • , A. Allafort
  • , E. Antolini
  • , W. B. Atwood
  • , M. Axelsson
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , K. Bechtol
  • , R. Bellazzini
  • , B. Berenji
  • , R. D. Blandford
  • , E. D. Bloom
  • , E. Bonamente
  • , A. W. Borgland
  • , E. Bottacini
  • , A. Bouvier
  • , J. Bregeon
  • M. Brigida, P. Bruel, R. Buehler, T. H. Burnett, S. Buson, G. A. Caliandro, R. A. Cameron, P. A. Caraveo, J. M. Casandjian, E. Cavazzuti, C. Cecchi, E. Charles, C. C. Cheung, J. Chiang, S. Ciprini, R. Claus, J. Cohen-Tanugi, J. Conrad, L. Costamante, S. Cutini, A. De Angelis, F. De Palma, C. D. Dermer, S. W. Digel, E. Do Couto E Silva, P. S. Drell, R. Dubois, L. Escande, C. Favuzzi, S. J. Fegan, E. C. Ferrara, J. Finke, 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, J. E. Grove, S. Guiriec, M. Gustafsson, D. Hadasch, M. Hayashida, E. Hays, S. E. Healey, D. Horan, X. Hou, R. E. Hughes, G. Iafrate, G. Jóhannesson, A. S. Johnson, W. N. Johnson, T. Kamae, H. Katagiri, J. Kataoka, J. Knödlseder, M. Kuss, J. Lande, S. Larsson, L. Latronico, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, G. M. Madejski, M. N. Mazziotta, W. McConville, J. E. McEnery, P. F. Michelson, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, C. Monte, M. E. Monzani, E. Moretti, A. Morselli, I. V. Moskalenko, S. Murgia, T. Nakamori, M. Naumann-Godo, P. L. Nolan, J. P. Norris, E. Nuss, M. Ohno, T. Ohsugi, A. Okumura, N. Omodei, M. Orienti, E. Orlando, J. F. Ormes, M. Ozaki, D. Paneque, D. Parent, M. Pesce-Rollins, M. Pierbattista, S. Piranomonte, F. Piron, G. Pivato, T. A. Porter, S. Rainò, R. Rando, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, S. Ritz, L. S. Rochester, R. W. Romani, M. Roth, D. A. Sanchez, C. Sbarra, J. D. Scargle, T. L. Schalk, C. Sgrò, M. S. Shaw, E. J. Siskind, G. Spandre, P. Spinelli, A. W. Strong, D. J. Suson, H. Tajima, H. Takahashi, T. Takahashi, T. Tanaka, J. G. Thayer, J. B. Thayer, D. J. Thompson, L. Tibaldo, M. Tinivella, D. F. Torres, G. Tosti, E. Troja, Y. Uchiyama, J. Vandenbroucke, V. Vasileiou, G. Vianello, V. Vitale, A. P. Waite, E. Wallace, P. Wang, B. L. Winer, D. L. Wood, K. S. Wood, S. Zimmer
  • Stanford University
  • INFN Sezione di Perugia
  • University of Perugia
  • University of California at Santa Cruz
  • Stockholm University
  • Oskar Klein Centre
  • KTH Royal Institute of Technology
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Universite Paris-Saclay
  • INFN Sezione di Trieste
  • University of Trieste
  • INFN
  • University of Padova
  • Politecnico di Bari
  • INFN Sezione di Bari
  • University of Washington
  • University of Sheffield
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Science and Research Directorate
  • National Research Council
  • Naval Research Laboratory
  • ASI Science Data Center
  • Laboratoire Univers et Particules de Montpellier
  • and Physics University of Udine
  • Univ. Bordeaux
  • NASA Goddard Space Flight Center
  • Ip Paris
  • INAF-Trieste
  • Hiroshima University
  • INAF Istituto di Radioastronomia
  • Center for Space Plasma and Aeronomic Research
  • Kyoto University
  • UMR 5797
  • The Ohio State University
  • University of Iceland
  • Ibaraki University
  • Waseda University
  • IRAP/CNRS
  • University of Maryland
  • Sezione di Roma
  • Boise State University
  • ISAS/JAXA
  • Max Planck Institut für Extraterrestrische Physik
  • University of Denver
  • Max-Planck-Institut für Physik
  • George Mason University
  • Osservatorio Astronomico di Roma
  • Medical University of Innsbruck
  • Max-Planck-Institut für Kernphysik
  • NASA Ames Research Center
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Nagoya University
  • Pompeu Fabra University (UPF)
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • University of Rome “Tor Vergata”
  • Praxis Inc.

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Résumé

The second catalog of active galactic nuclei (AGNs) detected by the Fermi Large Area Telescope (LAT) in two years of scientific operation is presented. The second LAT AGN catalog (2LAC) includes 1017 γ-ray sources located at high Galactic latitudes (|b| > 10°) that are detected with a test statistic (TS) greater than 25 and associated statistically with AGNs. However, some of these are affected by analysis issues and some are associated with multiple AGNs. Consequently, we define a Clean Sample which includes 886 AGNs, comprising 395 BLLacertae objects (BLLac objects), 310 flat-spectrum radio quasars (FSRQs), 157 candidate blazars of unknown type (i.e., with broadband blazar characteristics but with no optical spectral measurement yet), 8 misaligned AGNs, 4 narrow-line Seyfert 1 (NLS1s), 10 AGNs of other types, and 2 starburst galaxies. Where possible, the blazars have been further classified based on their spectral energy distributions (SEDs) as archival radio, optical, and X-ray data permit. While almost all FSRQs have a synchrotron-peak frequency <1014 Hz, about half of the BLLac objects have a synchrotron-peak frequency >1015 Hz. The 2LAC represents a significant improvement relative to the first LAT AGN catalog (1LAC), with 52% more associated sources. The full characterization of the newly detected sources will require more broadband data. Various properties, such as γ-ray fluxes and photon power-law spectral indices, redshifts, γ-ray luminosities, variability, and archival radio luminosities and their correlations are presented and discussed for the different blazar classes. The general trends observed in 1LAC are confirmed.

langue originaleAnglais
Numéro d'article171
journalAstrophysical Journal
Volume743
Numéro de publication2
Les DOIs
étatPublié - 20 déc. 2011

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