The AGILE Mission

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.

[1]  Giselher G. Lichti,et al.  Second Cos $B$ Catalog of High-energy gamma-ray Sources , 1981 .

[2]  Columbia,et al.  The Parkes Multibeam Pulsar Survey - III. Young Pulsars and the Discovery and Timing of 200 Pulsars , 2003, astro-ph/0303473.

[3]  C. Fichtel,et al.  Gamma-Ray Astrophysics , 1980 .

[4]  Brenda L. Dingus,et al.  Supplement to the Second EGRET Catalog of High-Energy Gamma-Ray Sources , 1996 .

[5]  S. Hunter,et al.  EGRET Observations of Radio-bright Supernova Remnants , 1996 .

[6]  J. R. P. Angel,et al.  Multiple object spectroscopy - The Medusa spectrograph , 1980 .

[7]  P. N. Bhat,et al.  Evidence for sub-millisecond structure in a γ-ray burst , 1992, Nature.

[8]  D. Palmer,et al.  BATSE observations of gamma-ray burst spectra. I: Spectral diversity , 1993 .

[9]  Giulio Fedel,et al.  The AGILE silicon tracker: an innovative γ-ray instrument for space , 2003 .

[10]  D. L. Bertsch,et al.  Calibration of the Energetic Gamma-Ray Experiment Telescope (EGRET) for the Compton Gamma-Ray Observatory , 1993 .

[11]  R. Maiolino,et al.  Texas in Tuscany : XXI Symposium on Relativistic Astrophysics, Florence, Italy 9-13 December 2002 , 2003 .

[12]  George W. Clark,et al.  High-energy cosmic gamma-ray observations from the OSO-3 satellite. , 1972 .

[13]  A. Moiseev,et al.  A wide aperture telescope for high energy gamma rays detection , 1995 .

[14]  M. Casolino,et al.  The GILDA mission: a new technique for a gamma-ray telescope in the energy range 20 MeV-100 GeV , 1995 .

[15]  D. Thompson,et al.  High energy gamma ray results from the second small astronomy satellite , 1975 .

[16]  D. Thompson,et al.  Discovery of a Nonblazar Gamma-Ray Transient Source Near the Galactic Plane: GRO J1838–04 , 1997, astro-ph/9702053.

[17]  Carl E. Fichtel,et al.  Galaxies and gamma-ray astronomy , 1979 .

[18]  K. Moriarty,et al.  The U (6,6) ⊗ O (3,1) peripheral absorption model and the production of 2+ and 1+ mesons , 1972 .

[19]  Marco Tavani,et al.  Simulation of the AGILE gamma-ray imaging detector performance: Part II , 2002 .

[20]  D. L. Bertsch,et al.  The Second EGRET Catalog of High-Energy Gamma-Ray Sources , 1995 .

[21]  V. Bidoli,et al.  Experiment NINA: investigation of low energy nuclear fluxes in the near-Earth space , 1997 .

[22]  E. Vallazza,et al.  The AGILE silicon tracker: testbeam results of the prototype silicon detector , 2002 .

[23]  M. Tavani,et al.  On the duty-cycle of ?-ray blazars: On the duty-cycle of ?-ray blazars , 2004 .

[24]  K. Bernlöhr,et al.  The H.E.S.S. Survey of the Inner Galaxy in Very High Energy Gamma Rays , 2005 .

[25]  A. Hall Applied Optics. , 2022, Science.