Skip to main navigation Skip to search Skip to main content

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
  • National Institute for Nuclear Physics
  • University of Padua
  • Polytechnic University of Bari
  • SLAC National Accelerator Laboratory
  • University of Turin
  • Laboratoire de Physique Subatomique et de Cosmologie (LPSC)
  • École polytechnique
  • German Electron Synchrotron
  • University of Würzburg
  • Istituto di Astrofisica Spaziale e Fisica Cosmica di Bologna
  • Italian Space Agency
  • Naval Research Laboratory
  • Université d'Orléans
  • CNRS
  • Université Montpellier 2
  • National Institute for Astrophysics
  • University of Salento
  • Université Savoie Mont Blanc
  • Complutense University
  • NASA Goddard Space Flight Center
  • University of Maryland
  • Hiroshima University
  • Max Planck Institute for Physics (Werner Heisenberg Institute)
  • Centre d'Etudes Nucléaires Bordeaux-Gradingnan (CENBG)
  • George Washington University
  • University of Göttingen
  • University of Iceland
  • George Mason University
  • The University of Tokyo
  • Oskar Klein Centre
  • Dalarna University
  • University of Turku
  • University of Trieste
  • University of Innsbruck
  • University of Perugia
  • Friedrich-Alexander University Erlangen-Nürnberg
  • Faculty of Science, Mahidol University
  • University of Maryland Baltimore County
  • Korea Astronomy and Space Science Institute
  • American University Washington DC
  • The University of Hong Kong
  • NYCB Real-Time Computing Inc.
  • Université de Bordeaux
  • Purdue University Northwest
  • Nagoya University
  • IRAP
  • Campus UAB
  • Institut d'Estudis Espacials de Catalunya
  • ICREA
  • University of Nova Gorica

Research output: Contribution to journalArticlepeer-review

66 Citations (Scopus)

Abstract

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.

Original languageEnglish
Article number12
JournalAstrophysical Journal, Supplement Series
Volume256
Issue number1
DOIs
Publication statusPublished - Sept 2021

ASJC Scopus subject areas

  • Astronomy and Astrophysics
  • Space and Planetary Science

Fingerprint

Dive into the research topics of 'Fermi Large Area Telescope Performance after 10 Years of Operation'. Together they form a unique fingerprint.

Cite this