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Multiwavelength evidence for quasi-periodic modulation in the gamma-ray blazar PG 1553+113

  • M. Ackermann
  • , M. Ajello
  • , A. Albert
  • , W. B. Atwood
  • , L. Baldini
  • , J. Ballet
  • , G. Barbiellini
  • , D. Bastieri
  • , J. Becerra Gonzalez
  • , R. Bellazzini
  • , E. Bissaldi
  • , R. D. Blandford
  • , E. D. Bloom
  • , R. Bonino
  • , E. Bottacini
  • , J. Bregeon
  • , P. Bruel
  • , R. Buehler
  • , S. Buson
  • , G. A. Caliandro
  • R. A. Cameron, R. Caputo, M. Caragiulo, P. A. Caraveo, E. Cavazzuti, C. Cecchi, A. Chekhtman, J. Chiang, G. Chiaro, S. Ciprini, J. Cohen-Tanugi, J. Conrad, S. Cutini, F. D'Ammando, A. De Angelis, F. De Palma, R. Desiante, L. Di Venere, A. Dominguez, P. S. Drell, C. Favuzzi, S. J. Fegan, E. C. Ferrara, W. B. Focke, L. Fuhrmann, Y. Fukazawa, P. Fusco, F. Gargano, D. Gasparrini, N. Giglietto, P. Giommi, F. Giordano, M. Giroletti, G. Godfrey, D. Green, I. A. Grenier, J. E. Grove, S. Guiriec, A. K. Harding, E. Hays, J. W. Hewitt, A. B. Hill, D. Horan, T. Jogler, G. Jóhannesson, A. S. Johnson, T. Kamae, M. Kuss, S. Larsson, L. Latronico, J. Li, L. Li, F. Longo, F. Loparco, B. Lott, M. N. Lovellette, P. Lubrano, J. Magill, S. Maldera, A. Manfreda, W. Max-Moerbeck, M. Mayer, M. N. Mazziotta, J. E. McEnery, P. F. Michelson, T. Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Murgia, E. Nuss, M. Ohno, T. Ohsugi, R. Ojha, N. Omodei, E. Orlando, J. F. Ormes, D. Paneque, T. J. Pearson, J. S. Perkins, M. Perri, M. Pesce-Rollins, V. Petrosian, F. Piron, G. Pivato, T. A. Porter, S. Rainò, R. Rando, M. Razzano, A. Readhead, A. Reimer, O. Reimer, A. Schulz, C. Sgrò, E. J. Siskind, F. Spada, G. Spandre, P. Spinelli, D. J. Suson, H. Takahashi, J. B. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, G. Tosti, E. Troja, Y. Uchiyama, G. Vianello, K. S. Wood, M. Wood, S. Zimmer, A. Berdyugin, R. H.D. Corbet, T. Hovatta, E. Lindfors, K. Nilsson, R. Reinthal, A. Sillanpää, A. Stamerra, L. O. Takalo, M. J. Valtonen
  • c/o DESY
  • Clemson University
  • Kavli Institute for Particle Astrophysics and Cosmology
  • University of California at Santa Cruz
  • University of Pisa
  • Universite Paris-Saclay
  • INFN Sezione di Trieste
  • University of Trieste
  • INFN
  • University of Padova
  • NASA Goddard Space Flight Center
  • University of Maryland
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN Sezione di Bari
  • INFN Sezione di Torino
  • University of Turin
  • Laboratoire Univers et Particules de Montpellier
  • Consorzio Interuniversitario per la Fisica Spaziale (CIFS)
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Science and Research Directorate
  • INFN Sezione di Perugia
  • University of Perugia
  • George Mason University
  • Osservatorio Astronomico di Roma
  • Stockholm University
  • Oskar Klein Centre
  • Royal Swedish Academy of Sciences
  • INAF Istituto di Radioastronomia
  • University of Bologna
  • and Physics University of Udine
  • Università Telematica Pegaso
  • Politecnico di Bari
  • Max-Planck-Institut für Radioastronomie
  • Hiroshima University
  • Naval Research Laboratory
  • University of North Florida
  • University of Southampton
  • University of Iceland
  • University of Tokyo
  • KTH Royal Institute of Technology
  • University of Sheffield
  • UMR 5797
  • National Radio Astronomy Observatory Socorro
  • California Institute of Technology
  • Sezione di Roma
  • Long Beach VA and University of California
  • University of Denver
  • Max-Planck-Institut für Physik
  • Medical University of Innsbruck
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Pompeu Fabra University (UPF)
  • University of Turku
  • Biochemical and Environmental Engineering
  • Aalto University
  • University of Turku
  • Osservatorio Astronomico di Torino
  • Scuola Normale Superiore di Pisa

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

We report for the first time a γ-ray and multiwavelength nearly periodic oscillation in an active galactic nucleus. Using the Fermi Large Area Telescope we have discovered an apparent quasi-periodicity in the γ-ray flux (E > 100 MeV) from the GeV/TeV BL Lac object PG 1553+113. The marginal significance of the 2.18 ± 0.08 year period γ-ray cycle is strengthened by correlated oscillations observed in radio and optical fluxes, through data collected in the Owens Valley Radio Observatory, Tuorla, Katzman Automatic Imaging Telescope, and Catalina Sky Survey monitoring programs and Swift-UVOT. The optical cycle appearing in ∼10 years of data has a similar period, while the 15 GHz oscillation is less regular than seen in the other bands. Further long-term multiwavelength monitoring of this blazar may discriminate among the possible explanations for this quasi-periodicity.

langue originaleAnglais
Numéro d'articleL41
journalAstrophysical Journal Letters
Volume813
Numéro de publication2
Les DOIs
étatPublié - 10 nov. 2015

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