English
Related papers

Related papers: Gamma-ray blazars: the view from AGILE

200 papers

PKS 1510-089 is a powerful Flat Spectrum Radio Quasar at z=0.361 with radiative output dominated by the gamma-ray emission. In the last two years PKS 1510-089 showed high variability over all the electromagnetic spectrum and in particular…

High Energy Astrophysical Phenomena · Physics 2009-10-07 F. D'Ammando , C. M. Raiteri , M. Villata , P. Romano , S. Covino , H. Krimm , M. Tavani , the AGILE , GASP-WEBT Collaborations

During the period July 2007 - January 2009, the AGILE satellite, together with several other space- and ground-based observatories monitored the activity of the flat-spectrum radio quasar 3C 454.3, yielding the longest multiwavelength…

High Energy Astrophysical Phenomena · Physics 2019-08-14 S. Vercellone

AGILE is a small gamma-ray astronomy satellite, with good spatial resolution, excellent timing capabilities and an unprecedented large field of view (~1/5 of the sky). It will be the next mission dedicated to high energy astrophysics in the…

Astrophysics · Physics 2007-05-23 A. Pellizzoni , A. Chen , M. Conti , A. Giuliani , S. Mereghetti , M. Tavani , S. Vercellone

In July 2007, the blazar 3C 454.3 underwent a flare in the optical, reaching R~13 on July 19. Then the optical flux decreased by one magnitude, being R~14 when the source was detected by the gamma-ray satellite AGILE, that observed the…

Astrophysics · Physics 2009-11-13 G. Ghisellini , L. Foschini , F. Tavecchio , E. Pian

The AGILE satellite, in orbit since 2007, localized up to October 2009 about 1 Gamma Ray Burst (GRB) per month with the hard X-ray imager SuperAGILE (18 - 60 keV) (with a rate reduced by a factor 2-3 in spinning mode) and is detecting…

High Energy Astrophysical Phenomena · Physics 2019-08-13 F. Longo , G. Barbiellini , E. Del Monte , M. Marisaldi , F. Fuschino , A. Giuliani

Since its early phases of operation, the AGILE satellite is observing Gamma Ray Bursts (GRBs) over an energy range potentially spanning six orders of magnitude. In the hard X-ray band the SuperAGILE imager provides localization of about one…

The AGILE satellite, operating since mid 2007 and primarily devoted to high-energy astrophysics, is one of the only three currently operating space instruments capable of detecting Terrestrial Gamma-Ray Flashes (TGFs), together with RHESSI…

High Energy Astrophysical Phenomena · Physics 2022-03-02 M. Marisaldi , F. Fuschino , C. Labanti , A. Bulgarelli , F. Gianotti , M. Trifoglio , M. Tavani , A. Argan , E. Del Monte , F. Longo , G. Barbiellini , A. Giuliani , A. Trois

The AGILE satellite detected transient high-energy gamma-ray emission from the X-ray binary V404 Cygni, during the June 2015 outburst observed in radio, optical, X-ray and soft gamma-ray frequencies. The activity was observed by AGILE in…

High Energy Astrophysical Phenomena · Physics 2017-04-26 G. Piano , P. Munar-Adrover , F. Verrecchia , M. Tavani , S. A. Trushkin

We take into account the constraints from the observed extragalactic gamma-ray background to estimate the maximum duty cycle allowed for a selected sample of WMAP Blazars, in order to be detectable by AGILE and GLAST gamma-ray experiments.…

Astrophysics · Physics 2009-06-23 Carlotta Pittori , Elisabetta Cavazzuti , Sergio Colafrancesco , Paolo Giommi

AGILE is an innovative, cost-effective gamma-ray mission proposed to the ASI Program of Small Scientific Missions. It is planned to detect gamma-rays in the 30 MeV - 50 GeV energy band and operate as an {\bf Observatory} open to the…

We report on 18 months of multiwavelength observations of the blazar 3C 454.3 (Crazy Diamond) carried out in July 2007-January 2009. We show the results of the AGILE campaigns which took place on May-June 2008, July-August 2008, and October…

High Energy Astrophysical Phenomena · Physics 2015-05-18 S. Vercellone , F. D'Ammando , V. Vittorini , I. Donnarumma , G. Pucella , M. Tavani , A. Ferrari , C. M. Raiteri , M. Villata , P. Romano , H. Krimm , A. Tiengo , A. W. Chen , G. Giovannini , T. Venturi , M. Giroletti , Y. Y. Kovalev , K. Sokolovsky , A. B. Pushkarev , M. L. Lister , A. Argan , G. Barbiellini , A. Bulgarelli , P. Caraveo , P. W. Cattaneo , V. Cocco , E. Costa , E. Del Monte , G. De Paris , G. Di Cocco , Y. Evangelista , M. Feroci , M. Fiorini , F. Fornari , T. Froysland , F. Fuschino , M. Galli , F. Gianotti , C. Labanti , I. Lapshov , F. Lazzarotto , P. Lipari , F. Longo , A. Giuliani , M. Marisaldi , S. Mereghetti , A. Morselli , A. Pellizzoni , L. Pacciani , F. Perotti , G. Piano , P. Picozza , M. Pilia , M. Prest , M. Rapisarda , A. Rappoldi , S. Sabatini , P. Soffitta , E. Striani , M. Trifoglio , A. Trois , E. Vallazza , A. Zambra , D. Zanello , C. Pittori , F. Verrecchia , P. Santolamazza , P. Giommi , S. Colafrancesco , L. Salotti , I. Agudo , H. D. Aller , M. F. Aller , A. A. Arkharov , U. Bach , R. Bachev , P. Beltrame , E. Benitez , M. Boettcher , C. S. Buemi , P. Calcidese , D. Capezzali , D. Carosati , W. P. Chen , D. Da Rio , A. Di Paola , M. Dolci , D. Dultzin , E. Forne , J. L. Gomez , M. A. Gurwell , V. A. Hagen-Thorn , A. Halkola , J. Heidt , D. Hiriart , T. Hovatta , H. Y. Hsiao , S. G. Jorstad , G. Kimeridze , T. S. Konstantinova , E. N. Kopatskaya , E. Koptelova , O. Kurtanidze , A. Lahteenmaki , V. M. Larionov , P. Leto , R. Ligustri , E. Lindfors , J. M. Lopez , A. P. Marscher , R. Mujica , M. Nikolashvili , K. Nilsson

In recent years, a new generation of space missions offered great opportunities of discovery in high-energy astrophysics. In this article we focus on the scientific operations of the Gamma-Ray Imaging Detector (GRID) onboard the AGILE space…

Since its early phases of operation, the AGILE mission is successfully observing Gamma Ray Bursts (GRBs) in the hard X-ray band with the SuperAGILE imager and in the MeV range with the Mini-Calorimeter. Up to now, three firm GRB detections…

Some pulsars have their maximum observable energy output in the gamma-ray band, offering the possibility of using these high-energy photons as probes of the particle acceleration and interaction processes in pulsar magnetospheres. After an…

Astrophysics · Physics 2009-06-23 D. J. Thompson