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The Fermi-LAT Lightcurve Repository

  • S. Abdollahi
  • , M. Ajello
  • , L. Baldini
  • , J. Ballet
  • , D. Bastieri
  • , J. Becerra Gonzalez
  • , R. Bellazzini
  • , A. Berretta
  • , E. Bissaldi
  • , R. Bonino
  • , A. Brill
  • , P. Bruel
  • , E. Burns
  • , S. Buson
  • , R. A. Cameron
  • , R. Caputo
  • , P. A. Caraveo
  • , N. Cibrario
  • , S. Ciprini
  • , P. Cristarella Orestano
  • M. Crnogorcevic, S. Cutini, F. D’Ammando, S. De Gaetano, S. W. Digel, N. Di Lalla, L. Di Venere, A. Domínguez, V. Fallah Ramazani, S. J. Fegan, E. C. Ferrara, A. Fiori, H. Fleischhack, A. Franckowiak, Y. Fukazawa, P. Fusco, V. Gammaldi, F. Gargano, S. Garrappa, C. Gasbarra, D. Gasparrini, N. Giglietto, F. Giordano, M. Giroletti, D. Green, I. A. Grenier, S. Guiriec, M. Gustafsson, E. Hays, D. Horan, X. Hou, G. Jóhannesson, M. Kerr, D. Kocevski, M. Kuss, L. Latronico, J. Li, I. Liodakis, F. Longo, F. Loparco, L. Lorusso, B. Lott, M. N. Lovellette, P. Lubrano, S. Maldera, A. Manfreda, G. Martí-Devesa, M. N. Mazziotta, I. Mereu, M. Meyer, P. F. Michelson, T. Mizuno, M. E. Monzani, A. Morselli, I. V. Moskalenko, M. Negro, N. Omodei, E. Orlando, J. F. Ormes, D. Paneque, G. Panzarini, J. S. Perkins, M. Persic, M. Pesce-Rollins, R. Pillera, T. A. Porter, G. Principe, J. L. Racusin, S. Rainò, R. Rando, B. Rani, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, M. Sánchez-Conde, P. M.Saz Parkinson, Jeff Scargle, L. Scotton, D. Serini, C. Sgrò, E. J. Siskind, G. Spandre, P. Spinelli, D. J. Suson, H. Tajima, D. J. Thompson, D. F. Torres, J. Valverde, T. Venters, Z. Wadiasingh, S. Wagner, K. Wood
  • IRAP/CNRS
  • Clemson University
  • University of Pisa
  • CEA/UVSQ/CNRS
  • INFN
  • University of Padova
  • Instituto de Astrofisica de Canarias
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • University of Perugia
  • Politecnico di Bari
  • INFN Sezione di Bari
  • INFN Sezione di Torino
  • University of Turin
  • NASA Goddard Space Flight Center
  • Louisiana State University
  • University of Würzburg
  • Kavli Institute for Particle Astrophysics and Cosmology
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • INFN Roma Tor Vergata
  • Science and Research Directorate
  • INFN Sezione di Perugia
  • University of Maryland
  • INAF Istituto di Radioastronomia
  • Complutense University
  • Ruhr-University Bochum
  • Catholic University of America
  • Hiroshima University
  • Universidad Autónoma de Madrid
  • University of Rome “Tor Vergata”
  • Max-Planck-Institut für Physik
  • Laboratoire de Probabilités et Modèles Aléatoires
  • George Washington University
  • Georg-August-Universität Göttingen
  • Yunnan Observatories
  • Chinese Academy of Sciences
  • University of Iceland
  • KTH Royal Institute of Technology
  • Naval Research Laboratory
  • NASA Marshall Space Flight Center
  • University of Science and Technology of China
  • University of Turku
  • University of Trieste
  • INFN Sezione di Trieste
  • Univ. Bordeaux
  • The Aerospace Corporation
  • University of Innsbruck
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • Vatican Observatory
  • Biochemical and Environmental Engineering
  • University of Denver
  • INAF Osservatorio Astronomico di Padova
  • Korea Astronomy and Space Science Institute
  • American University
  • University of Johannesburg
  • University of California at Santa Cruz
  • NASA Ames Research Center
  • Laboratoire Univers et Particules de Montpellier
  • NYCB Real-Time Computing Inc.
  • Purdue University Northwest
  • Nagoya University
  • Campus UAB
  • Pompeu Fabra University (UPF)
  • Institut d’Estudis Espacials de Catalunya (IEEC)
  • Praxis Inc.

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

The Fermi Large Area Telescope (LAT) lightcurve repository (LCR) is a publicly available, continually updated library of gamma-ray lightcurves of variable Fermi-LAT sources generated over multiple timescales. The Fermi-LAT LCR aims to provide publication-quality lightcurves binned on timescales of 3, 7, and 30 days for 1525 sources deemed variable in the source catalog of the first 10 yr of Fermi-LAT observations. The repository consists of lightcurves generated through full likelihood analyses that model the sources and the surrounding region, providing fluxes and photon indices for each time bin. The LCR is intended as a resource for the time-domain and multimessenger communities by allowing users to search LAT data quickly to identify correlated variability and flaring emission episodes from gamma-ray sources. We describe the sample selection and analysis employed by the LCR and provide an overview of the associated data access portal.

langue originaleAnglais
Numéro d'article31
journalAstrophysical Journal, Supplement Series
Volume265
Numéro de publication2
Les DOIs
étatPublié - 1 avr. 2023

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