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Catalog of Long-term Transient Sources in the First 10 yr of Fermi-LAT Data

  • The Fermi-Lat Collaboration
  • , L. Baldini
  • , J. Ballet
  • , D. Bastieri
  • , J. Becerra Gonzalez
  • , R. Bellazzini
  • , A. Berretta
  • , E. Bissaldi
  • , R. D. Blandford
  • , E. D. Bloom
  • , R. Bonino
  • , E. Bottacini
  • , P. Bruel
  • , S. Buson
  • , R. A. Cameron
  • , P. A. Caraveo
  • , E. Cavazzuti
  • , S. Chen
  • , G. Chiaro
  • , D. Ciangottini
  • N. Cibario, S. Ciprini, P. Cristarella Orestano, M. Crnogorcevic, S. Cutini, F. D'Ammando, P. De La Torre Luque, F. De Palma, S. W. Digel, N. Di Lalla, F. Dirirsa, L. Di Venere, A. Domínguez, A. Fiori, H. Fleischhack, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, F. Gargano, D. Gasparrini, S. Germani, N. Giglietto, F. Giordano, M. Giroletti, D. Green, I. A. Grenier, S. Griffin, S. Guiriec, M. Gustafsson, J. W. Hewitt, D. Horan, R. Imazawa, G. Jóhannesson, M. Kerr, D. Kocevski, M. Kuss, S. Larsson, L. Latronico, J. Li, I. Liodakis, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, S. Maldera, A. Manfreda, G. Martí-Devesa, H. Matake, M. N. Mazziotta, I. Mereu, M. Meyer, N. Mirabal, W. Mitthumsiri, T. Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, S. Nagasawa, M. Negro, R. Ojha, M. Orienti, E. Orlando, M. Palatiello, V. Paliya, D. Paneque, Z. Pei, M. Persic, M. Pesce-Rollins, V. Petrosian, H. Poon, T. A. Porter, G. Principe, J. L. Racusin, S. Rain, R. Rando, B. Rani, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, P. M. Saz Parkinson, L. Scotton, D. Serini, C. Sgr, E. J. Siskind, G. Spandre, P. Spinelli, D. J. Suson, H. Tajima, D. Tak, D. F. Torres, G. Tosti, E. Troja, K. Wood, M. Yassine, G. Zaharijas, E. Cavazzuti
  • University of Pisa
  • Université Paris-Saclay
  • National Institute for Nuclear Physics
  • University of Padua
  • Instituto de Astrofísica de Canarias
  • University of Perugia
  • Polytechnic University of Bari
  • SLAC National Accelerator Laboratory
  • University of Turin
  • École polytechnique
  • University of Würzburg
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Italian Space Agency
  • University of Maryland
  • National Institute for Astrophysics
  • University of Salento
  • Université Savoie Mont Blanc
  • Complutense University
  • Catholic University of America
  • NASA Goddard Space Flight Center
  • Ruhr University Bochum
  • Hiroshima University
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • George Washington University
  • University of Göttingen
  • University of North Florida
  • University of Iceland
  • KTH Royal Institute of Technology
  • Naval Research Laboratory
  • NASA Marshall Space Flight Center
  • Oskar Klein Centre
  • Dalarna University
  • German Electron Synchrotron
  • University of Turku
  • University of Trieste
  • University of Innsbruck
  • University of Maryland Baltimore County
  • Faculty of Science, Mahidol University
  • The University of Tokyo
  • University of Udine
  • Aryabhatta Research Institute of Observational Sciences
  • Osservatorio Astronomico di Trieste
  • Korea Astronomy and Space Science Institute
  • American University Washington DC
  • University of California at Santa Cruz
  • The University of Hong Kong
  • Université Montpellier 2
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Nagoya University
  • Campus UAB
  • ICREA
  • Institut d'Estudis Espacials de Catalunya
  • Praxis, Inc.
  • University of Nova Gorica

Research output: Contribution to journalArticlepeer-review

14 Citations (Scopus)

Abstract

We present the first Fermi Large Area Telescope (LAT) catalog of long-term γ-ray transient sources (1FLT). This comprises sources that were detected on monthly time intervals during the first decade of Fermi-LAT operations. The monthly timescale allows us to identify transient and variable sources that were not yet reported in other Fermi-LAT catalogs. The monthly data sets were analyzed using a wavelet-based source detection algorithm that provided the candidate new transient sources. The search was limited to the extragalactic regions of the sky to avoid the dominance of the Galactic diffuse emission at low Galactic latitudes. The transient candidates were then analyzed using the standard Fermi-LAT maximum likelihood analysis method. All sources detected with a statistical significance above 4σ in at least one monthly bin were listed in the final catalog. The 1FLT catalog contains 142 transient γ-ray sources that are not included in the 4FGL-DR2 catalog. Many of these sources (102) have been confidently associated with active galactic nuclei (AGNs): 24 are associated with flat-spectrum radio quasars, 1 with a BL Lac object, 70 with blazars of uncertain type, 3 with radio galaxies, 1 with a compact steep-spectrum radio source, 1 with a steep-spectrum radio quasar, and 2 with AGNs of other types. The remaining 40 sources have no candidate counterparts at other wavelengths. The median γ-ray spectral index of the 1FLT-AGN sources is softer than that reported in the latest Fermi-LAT AGN general catalog. This result is consistent with the hypothesis that detection of the softest γ-ray emitters is less efficient when the data are integrated over year-long intervals.

Original languageEnglish
Article number13
JournalAstrophysical Journal, Supplement Series
Volume256
Issue number1
DOIs
Publication statusPublished - Sept 2021

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

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