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Incremental Fermi Large Area Telescope Fourth Source Catalog

  • S. Abdollahi
  • , F. Acero
  • , L. Baldini
  • , J. Ballet
  • , D. Bastieri
  • , R. Bellazzini
  • , B. Berenji
  • , A. Berretta
  • , E. Bissaldi
  • , R. D. Blandford
  • , E. Bloom
  • , R. Bonino
  • , A. Brill
  • , R. J. Britto
  • , P. Bruel
  • , T. H. Burnett
  • , S. Buson
  • , R. A. Cameron
  • , R. Caputo
  • , P. A. Caraveo
  • D. Castro, S. Chaty, C. C. Cheung, G. Chiaro, N. Cibrario, S. Ciprini, J. Coronado-Blázquez, M. Crnogorcevic, S. Cutini, F. D'Ammando, S. De Gaetano, S. W. Digel, N. Di Lalla, F. Dirirsa, L. Di Venere, A. Domínguez, V. Fallah Ramazani, S. J. Fegan, E. C. Ferrara, A. Fiori, H. Fleischhack, A. Franckowiak, Y. Fukazawa, S. Funk, P. Fusco, G. Galanti, V. Gammaldi, F. Gargano, S. Garrappa, D. Gasparrini, F. Giacchino, N. Giglietto, F. Giordano, M. Giroletti, T. Glanzman, D. Green, I. A. Grenier, M. H. Grondin, L. Guillemot, S. Guiriec, M. Gustafsson, A. K. Harding, E. Hays, J. W. Hewitt, D. Horan, X. Hou, G. Jóhannesson, C. Karwin, T. Kayanoki, M. Kerr, M. Kuss, D. Landriu, S. Larsson, L. Latronico, M. Lemoine-Goumard, J. Li, I. Liodakis, F. Longo, F. Loparco, B. Lott, P. Lubrano, S. Maldera, D. Malyshev, A. Manfreda, G. Martí-Devesa, M. N. Mazziotta, I. Mereu, M. Meyer, P. F. Michelson, N. Mirabal, W. Mitthumsiri, T. Mizuno, A. A. Moiseev, M. E. Monzani, A. Morselli, I. V. Moskalenko, M. Negro, E. Nuss, N. Omodei, M. Orienti, E. Orlando, D. Paneque, Z. Pei, J. S. Perkins, M. Persic, M. Pesce-Rollins, V. Petrosian, R. Pillera, H. Poon, T. A. Porter, G. Principe, S. Rainò, R. Rando, B. Rani, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, T. Reposeur, M. Sánchez-Conde, P. M. Saz Parkinson, L. Scotton, D. Serini, C. Sgrò, E. J. Siskind, D. A. Smith, G. Spandre, P. Spinelli, K. Sueoka, D. J. Suson, H. Tajima, D. Tak, J. B. Thayer, D. J. Thompson, D. F. Torres, E. Troja, J. Valverde, K. Wood, G. Zaharijas
  • IRAP/CNRS
  • CEA/UVSQ/CNRS
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • INFN
  • University of Padova
  • California State University-Los Angeles
  • University of Perugia
  • Politecnico di Bari
  • INFN Sezione di Bari
  • Stanford Linear Accelerator Center
  • INFN Sezione di Torino
  • University of Turin
  • NASA Goddard Space Flight Center
  • University of the Free State
  • University of Washington
  • University of Würzburg
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Center for Astrophysics | Harvard & Smithsonian
  • Naval Research Laboratory
  • INFN Roma Tor Vergata
  • Science and Research Directorate
  • Universidad Autónoma de Madrid
  • University of Maryland
  • INFN Sezione di Perugia
  • INAF Istituto di Radioastronomia
  • Ethiopian Space Science and Technology Institute
  • Complutense University
  • Ruhr-University Bochum
  • University of Pisa
  • Catholic University of America
  • Hiroshima University
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • c/o DESY
  • Max-Planck-Institut für Physik
  • Univ. Bordeaux
  • conventionnée avec l'Université d'Orléans
  • CNRS
  • George Washington University
  • Georg-August-Universität Göttingen
  • MST-8, Los Alamos National Laboratory
  • University of North Florida
  • Yunnan Observatories
  • Chinese Academy of Sciences
  • University of Iceland
  • Stockholm University
  • Clemson University
  • KTH Royal Institute of Technology
  • Oskar Klein Centre
  • Dalarna University
  • University of Science and Technology of China
  • University of Turku
  • INFN Sezione di Trieste
  • University of Trieste
  • University of Innsbruck
  • Biochemical and Environmental Engineering
  • Faculty of Science, Mahidol University
  • Laboratoire Univers et Particules de Montpellier
  • INAF-Trieste
  • Korea Astronomy and Space Science Institute
  • American University
  • University of Johannesburg
  • University of California at Santa Cruz
  • University of Hong Kong
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Nagoya University
  • Campus UAB
  • Institut d’Estudis Espacials de Catalunya (IEEC)
  • Pompeu Fabra University (UPF)
  • Praxis Inc.
  • University of Nova Gorica

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

We present an incremental version (4FGL-DR3, for Data Release 3) of the fourth Fermi Large Area Telescope (LAT) catalog of 3-ray sources. Based on the first 12 years of science data in the energy range from 50 MeV to 1 TeV, it contains 6658 sources. The analysis improves on that used for the 4FGL catalog over eight years of data: more sources are fit with curved spectra, we introduce a more robust spectral parameterization for pulsars, and we extend the spectral points to 1 TeV. The spectral parameters, spectral energy distributions, and associations are updated for all sources. Light curves are rebuilt for all sources with 1 yr intervals (not 2 month intervals). Among the 5064 original 4FGL sources, 16 were deleted, 112 are formally below the detection threshold over 12 yr (but are kept in the list), while 74 are newly associated, 10 have an improved association, and seven associations were withdrawn. Pulsars are split explicitly between young and millisecond pulsars. Pulsars and binaries newly detected in LAT sources, as well as more than 100 newly classified blazars, are reported. We add three extended sources and 1607 new point sources, mostly just above the detection threshold, among which eight are considered identified, and 699 have a plausible counterpart at other wavelengths. We discuss the degree-scale residuals to the global sky model and clusters of soft unassociated point sources close to the Galactic plane, which are possibly related to limitations of the interstellar emission model and missing extended sources.

langue originaleAnglais
Numéro d'article53
journalAstrophysical Journal, Supplement Series
Volume260
Numéro de publication2
Les DOIs
étatPublié - 1 juin 2022

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