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The AGILE Mission

Author(s)
Tavani, M.
Giommi, Paolo  
Argan, A.
Barbiellini, G.
Crisconio, Marino  
more
Subjects

instrumentation detec...

techniques: image pro...

techniques: high angu...

gamma rays: observati...

X-rays: general

techniques high angul...

techniques image proc...

Date Issued
2009-08-01
Mission(s)
AGILE  
Abstract
Context. AGILE is an Italian Space Agency mission dedicated to observing the gamma-ray Universe. The AGILE's very innovative instrumentation for the first time combines a gamma-ray imager (sensitive in the energy range 30 MeV–50 GeV), a hard X-ray imager (sensitive in the range 18–60 keV), a calorimeter (sensitive in the range 350 keV–100 MeV), and an anticoincidence system. AGILE was successfully launched on 2007 April 23 from the Indian base of Sriharikota and was inserted in an equatorial orbit with very low particle background.

Aims. AGILE provides crucial data for the study of active galactic nuclei, gamma-ray bursts, pulsars, unidentified gamma-ray sources, galactic compact objects, supernova remnants, TeV sources, and fundamental physics by microsecond timing.

Methods. An optimal sky angular positioning (reaching 0.1 degrees in gamma-rays and 1–2 arcmin in hard X-rays) and very large fields of view (2.5 sr and 1 sr, respectively) are obtained by the use of Silicon detectors integrated in a very compact instrument.

Results. AGILE surveyed the gamma-ray sky and detected many Galactic and extragalactic sources during the first months of observations. Particular emphasis is given to multifrequency observation programs of extragalactic and galactic objects.

Conclusions. AGILE is a successful high-energy gamma-ray mission that reached its nominal scientific performance. The AGILE Cycle-1 pointing program started on 2007 December 1, and is open to the international community through a Guest Observer Program.
URI
https://hdl.handle.net/20.500.13025/1251
ISSN
0004-6361
Journal
Astronomy and Astrophysics
DOI
10.1051/0004-6361/200810527
http://dx.doi.org/10.1051/0004-6361/200810527
54dcce0c8580fe1368eeb3ee
URL
http://adsabs.harvard.edu/abs/2009A&A...502..995T
http://www.aanda.org/articles/aa/abs/2009/30/aa10527-08/aa10527-08.html
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