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Fermi Large Area Telescope Performance after 10 Years of Operation

  • M. Ajello
  • , W. B. Atwood
  • , M. Axelsson
  • , R. Bagagli
  • , M. Bagni
  • , L. Baldini
  • , D. Bastieri
  • , F. Bellardi
  • , R. Bellazzini
  • , E. Bissaldi
  • , E. D. Bloom
  • , R. Bonino
  • , J. Bregeon
  • , A. Brez
  • , P. Bruel
  • , R. Buehler
  • , S. Buson
  • , R. A. Cameron
  • , P. A. Caraveo
  • , E. Cavazzuti
  • M. Ceccanti, S. Chen, C. C. Cheung, S. Ciprini, I. Cognard, J. Cohen-Tanugi, S. Cutini, F. D'Ammando, P. De La Torre Luque, F. De Palma, S. W. Digel, F. Dirirsa, N. Di Lalla, L. Di Venere, A. Domínguez, D. Fabiani, E. C. Ferrara, A. Fiori, G. Foglia, Y. Fukazawa, P. Fusco, F. Gargano, D. Gasparrini, M. Giroletti, T. Glanzman, D. Green, S. Griffin, M. H. Grondin, J. E. Grove, L. Guillemot, S. Guiriec, M. Gustafsson, E. Hays, D. Horan, G. Jóhannesson, T. J. Johnson, T. Kamae, M. Kerr, M. Kuss, S. Larsson, L. Latronico, M. Lemoine-Goumard, J. Li, I. Liodakis, F. Longo, F. Loparco, M. N. Lovellette, P. Lubrano, S. Maldera, A. Manfreda, G. Martí-Devesa, M. N. Mazziotta, N. Menon, I. Mereu, M. Meyer, P. F. Michelson, M. Minuti, W. Mitthumsiri, T. Mizuno, M. Mongelli, M. E. Monzani, I. V. Moskalenko, M. Negro, E. Nuss, R. Ojha, M. Orienti, E. Orlando, A. Paccagnella, V. S. Paliya, D. Paneque, Z. Pei, J. S. Perkins, M. Pesce-Rollins, M. Pinchera, F. Piron, H. Poon, T. A. Porter, R. Primavera, G. Principe, J. L. Racusin, S. Rain, R. Rando, B. Rani, E. Rapposelli, M. Razzano, S. Razzaque, A. Reimer, O. Reimer, J. J. Russell, N. Saggini, P. M. Saz Parkinson, N. Scolieri, D. Serini, C. Sgr, E. J. Siskind, D. A. Smith, G. Spandre, P. Spinelli, D. J. Suson, H. Tajima, J. G. Thayer, D. J. Thompson, L. Tibaldo, D. F. Torres, G. Tosti, J. Valverde, L. Vigiani, G. Zaharijas
  • Clemson University
  • University of California at Santa Cruz
  • Stockholm University
  • KTH Royal Institute of Technology
  • University of Pisa
  • INFN
  • University of Padova
  • Istituto Nazionale di Fisica Nucleare, Sezione di Pisa
  • Politecnico di Bari
  • INFN Sezione di Bari
  • Stanford Linear Accelerator Center
  • INFN Sezione di Torino
  • University of Turin
  • Laboratoire de Physique Subatomique et de Cosmologie de Grenoble
  • c/o DESY
  • University of Würzburg
  • INAF Istituto di Astrofisica Spaziale e Fisica Cosmica, Milan
  • Science and Research Directorate
  • Naval Research Laboratory
  • INFN Roma Tor Vergata
  • conventionnée avec l'Université d'Orléans
  • CNRS
  • Laboratoire Univers et Particules de Montpellier
  • INFN Sezione di Perugia
  • INAF Istituto di Radioastronomia
  • University of Salento
  • Sezione di Lecce
  • Université Savoie Mont Blanc
  • Complutense University
  • NASA Goddard Space Flight Center
  • University of Maryland
  • Hiroshima University
  • Max-Planck-Institut für Physik
  • UMR 5797
  • George Washington University
  • Georg-August-Universität Göttingen
  • University of Iceland
  • George Mason University
  • University of Tokyo
  • Oskar Klein Centre
  • Dalarna University
  • University of Turku
  • INFN Sezione di Trieste
  • University of Trieste
  • University of Innsbruck
  • University of Perugia
  • Friedrich-Alexander University (FAU) Erlangen-Nürnberg and Universitätsklinikum Erlangen
  • Faculty of Science, Mahidol University
  • Biochemical and Environmental Engineering
  • Korea Astronomy and Space Science Institute
  • American University
  • University of Johannesburg
  • University of Hong Kong
  • NYCB Real-Time Computing Inc.
  • Univ. Bordeaux
  • Purdue University Northwest
  • Nagoya University
  • IRAP/CNRS
  • Campus UAB
  • Institut d’Estudis Espacials de Catalunya (IEEC)
  • Pompeu Fabra University (UPF)
  • University of Nova Gorica

Résultats de recherche: Contribution à un journalArticleRevue par des pairs

Résumé

The Large Area Telescope (LAT), the primary instrument for the Fermi Gamma-ray Space Telescope (Fermi) mission, is an imaging, wide field-of-view, high-energy gamma-ray telescope, covering the energy range from 30 MeV to more than 300 GeV. We describe the performance of the instrument at the 10 yr milestone. LAT performance remains well within the specifications defined during the planning phase, validating the design choices and supporting the compelling case to extend the duration of the Fermi mission. The details provided here will be useful when designing the next generation of high-energy gamma-ray observatories.

langue originaleAnglais
Numéro d'article12
journalAstrophysical Journal, Supplement Series
Volume256
Numéro de publication1
Les DOIs
étatPublié - 1 sept. 2021

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