A1 Vertaisarvioitu alkuperäisartikkeli tieteellisessä lehdessä
Fermi Large Area Telescope Performance after 10 Years of Operation
Tekijät: Ajello M, Atwood WB, Axelsson M, Bagagli R, Bagni M, Baldini L, Bastieri D, Bellardi F, Bellazzini R, Bissaldi E, Bloom ED, Bonino R, Bregeon J, Brez A, Bruel P, Buehler R, Buson S, Cameron RA, Caraveo PA, Cavazzuti E, Ceccanti M, Chen S, Cheung CC, Ciprini S, Cognard I, Cohen-Tanugi J, Cutini S, D'Ammando F, Luque PD, de Palma F, Digel SW, Dirirsa F, Di Lalla N, Di Venere L, Dominguez A, Fabiani D, Ferrara EC, Fiori A, Foglia G, Fukazawa Y, Fusco P, Gargano F, Gasparrini D, Giroletti M, Glanzman T, Green D, Griffin S, Grondin MH, Grove JE, Guillemot L, Guiriec S, Gustafsson M, Hays E, Horan D, Johannesson G, Johnson TJ, Kamae T, Kerr M, Kuss M, Larsson S, Latronico L, Lemoine-Goumard M, Li J, Liodakis I, Longo F, Loparco F, Lovellette MN, Lubrano P, Maldera S, Manfreda A, Marti-Devesa G, Mazziotta MN, Menon N, Mereu I, Meyer M, Michelson PF, Minuti M, Mitthumsiri W, Mizuno T, Mongelli M, Monzani ME, Moskalenko IV, Negro M, Nuss E, Ojha R, Orienti M, Orlando E, Paccagnella A, Paliya VS, Paneque D, Pei Z, Perkins JS, Pesce-Rollins M, Pinchera M, Piron F, Poon H, Porter TA, Primavera R, Principe G, Racusin JL, Raino S, Rando R, Rani B, Rapposelli E, Razzano M, Razzaque S, Reimer A, Reimer O, Russell JJ, Saggini N, Parkinson PMS, Scolieri N, Serini D, Sgro C, Siskind EJ, Smith DA, Spandre G, Spinelli P, Suson DJ, Tajima H, Thayer JG, Thompson DJ, Tibaldo L, Torres DF, Tosti G, Valverde J, Vigiani L, Zaharijas G
Kustantaja: IOP PUBLISHING LTD
Julkaisuvuosi: 2021
Journal: Astrophysical Journal Supplement
Tietokannassa oleva lehden nimi: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
Lehden akronyymi: ASTROPHYS J SUPPL S
Artikkelin numero: ARTN 12
Vuosikerta: 256
Numero: 1
Sivujen määrä: 25
ISSN: 0067-0049
eISSN: 1538-4365
DOI: https://doi.org/10.3847/1538-4365/ac0ceb
Rinnakkaistallenteen osoite: https://research.utu.fi/converis/portal/detail/Publication/67227031
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.
Ladattava julkaisu This is an electronic reprint of the original article. |