2021ApJS..256...12A

Query : 2021ApJS..256...12A

2021ApJS..256...12A - Astrophys. J., Suppl. Ser., 256, 12-12 (2021/September-0)

Fermi Large Area Telescope performance after 10 years of operation.

AJELLO M., ATWOOD W.B., AXELSSON M., BAGAGLI R., BAGNI M., BALDINI L., BASTIERI D., BELLARDI F., BELLAZZINI R., BISSALDI E., BLOOM E.D., BONINO R., BREGEON J., BREZ A., BRUEL P., BUEHLER R., BUSON S., CAMERON R.A., CARAVEO P.A., CAVAZZUTI E., CECCANTI M., CHEN S., CHEUNG C.C., CIPRINI S., COGNARD I., COHEN-TANUGI J., CUTINI S., D'AMMANDO F., DE LA TORRE LUQUE P., DE PALMA F., DIGEL S.W., DIRIRSA F., DI LALLA N., DI VENERE L., DOMINGUEZ A., FABIANI D., FERRARA E.C., FIORI A., FOGLIA G., FUKAZAWA Y., FUSCO P., GARGANO F., GASPARRINI D., GIROLETTI M., GLANZMAN T., GREEN D., GRIFFIN S., GRONDIN M.-H., GROVE J.E., GUILLEMOT L., GUIRIEC S., GUSTAFSSON M., HAYS E., HORAN D., JOHANNESSON G., JOHNSON T.J., KAMAE T., KERR M., KUSS M., LARSSON S., LATRONICO L., LEMOINE-GOUMARD M., LI J., LIODAKIS I., LONGO F., LOPARCO F., LOVELLETTE M.N., LUBRANO P., MALDERA S., MANFREDA A., MARTI-DEVESA G., MAZZIOTTA M.N., MENON N., MEREU I., MEYER M., MICHELSON P.F., MINUTI M., MITTHUMSIRI W., MIZUNO T., MONGELLI M., MONZANI M.E., MOSKALENKO I.V., NEGRO M., NUSS E., OJHA R., ORIENTI M., ORLANDO E., PACCAGNELLA A., PALIYA V.S., PANEQUE D., PEI Z., PERKINS J.S., PESCE-ROLLINS M., PINCHERA M., PIRON F., POON H., PORTER T.A., PRIMAVERA R., PRINCIPE G., RACUSIN J.L., RAINO S., RANDO R., RANI B., RAPPOSELLI E., RAZZANO M., RAZZAQUE S., REIMER A., REIMER O., RUSSELL J.J., SAGGINI N., SAZ PARKINSON P.M., SCOLIERI N., SERINI D., SGRO C., SISKIND E.J., SMITH D.A., SPANDRE G., SPINELLI P., SUSON D.J., TAJIMA H., THAYER J.G., THOMPSON D.J., TIBALDO L., TORRES D.F., TOSTI G., VALVERDE J., VIGIANI L. and ZAHARIJAS G.

Abstract (from CDS):

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.

Abstract Copyright: © 2021. The American Astronomical Society. All rights reserved.

Journal keyword(s): Gamma-ray telescopes - Calibration

Simbad objects: 11

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Number of rows : 11
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 PSR J0437-47 Psr 04 37 15.7994581776 -47 15 08.544351636           DC 1032 0
2 V* CM Tau Psr 05 34 31.9474694616 +22 00 52.153698024           ~ 5476 0
3 PSR J0614-3329 Psr 06 14 10.3479 -33 29 54.116           ~ 134 1
4 NAME Vela SNR 08 34.0 -45 50           ~ 1331 2
5 PSR J1231-1411 Psr 12 31 11.3069 -14 11 43.628           ~ 139 0
6 GrW 170817 GWE 13 09 48.0850 -23 22 53.343           ~ 2683 0
7 NAME Galactic Center reg 17 45 39.60213 -29 00 22.0000           ~ 16269 0
8 NAME Sgr A* X 17 45 40.03599 -29 00 28.1699           ~ 4970 3
9 NAME G2 Dust Cloud IR 17 45 40.04 -29 00 28.1           ~ 209 0
10 PSR B1937+21.4 Psr 19 39 38.560096 +21 34 59.13552           ~ 1142 0
11 PSR J1959+2048 Psr 19 59 36.7643141520 +20 48 14.896407996   21.08 20.16 19.53 18.79 G: 854 3

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