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Fermi Large Area Telescope Performance After 10 Years Of Operation

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arxiv 2106.12203 v3 pith:XBHY7TN5 submitted 2021-06-23 astro-ph.IM

The Fermi LAT Collaboration: M. Ajello , W. B. Atwood , M. Axelsson , R. Bagagli , M. Bagni , L. Baldini , D. Bastieri , F. Bellardi
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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. Rainò 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. Sgrò 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
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classification astro-ph.IM
keywords fermitelescopegamma-rayperformanceareahigh-energyinstrumentlarge
verification ladder T0 review T1 audit T2 compute T3 formal
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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-year 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.

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