We report the AGILE gamma-ray observations and the results of the multiwavelength campaigns on seven flaring blazars detected by the mission: During two multiwavelength campaigns, we observed gamma-ray activity from two Flat Spectrum Radio Quasars of the Virgo region, e.g. 3C 279 and 3C 273 (the latter being the first extragalactic source simultaneously observed with the gamma-ray telescope and the hard X ray imager of the mission). Due to the large FOV of the AGILE/GRID instrument, we achieved an almost continuous coverage of the FSRQ 3C 454.3. The source showed flux above 10(-6) photons/cm(2)/s (E> 100 MeV) and showed day by day variability during all the AGILE observing periods. In the EGRET era, the source was found in high gamma-ray activity only once. An other blazar, PKS 1510-089 was frequently found in high gamma-ray activity. S5 0716+71, an intermediate BL Lac object, exhibited a very high gamma-ray activity and fast gamma-ray variability during a period of intense optical activity. We observed high gamma-ray activity from W Comae, a BL Lac object, and Mrk 421, a high energy peaked BL Lac object. For this source, a multiwavelength campaign from optical to TeV has been performed. (C) 2010 Elsevier B.V. All rights reserved.

The flaring blazars of the first 1.5 years of the AGILE mission

D'AMMANDO, FILIPPO;
2011

Abstract

We report the AGILE gamma-ray observations and the results of the multiwavelength campaigns on seven flaring blazars detected by the mission: During two multiwavelength campaigns, we observed gamma-ray activity from two Flat Spectrum Radio Quasars of the Virgo region, e.g. 3C 279 and 3C 273 (the latter being the first extragalactic source simultaneously observed with the gamma-ray telescope and the hard X ray imager of the mission). Due to the large FOV of the AGILE/GRID instrument, we achieved an almost continuous coverage of the FSRQ 3C 454.3. The source showed flux above 10(-6) photons/cm(2)/s (E> 100 MeV) and showed day by day variability during all the AGILE observing periods. In the EGRET era, the source was found in high gamma-ray activity only once. An other blazar, PKS 1510-089 was frequently found in high gamma-ray activity. S5 0716+71, an intermediate BL Lac object, exhibited a very high gamma-ray activity and fast gamma-ray variability during a period of intense optical activity. We observed high gamma-ray activity from W Comae, a BL Lac object, and Mrk 421, a high energy peaked BL Lac object. For this source, a multiwavelength campaign from optical to TeV has been performed. (C) 2010 Elsevier B.V. All rights reserved.
2011
Pacciani L; Bulgarelli A; Chen AW; DAmmando F; Donnarumma I; Giuliani A; Longo F; Pucella G; Tavani M; Vercellone S; Vittorini V; Argan A; Barbiellini G; Boffelli F; Caraveo P; Cattaneo PW; Cocco V; Costa E; De Paris G; Del Monte E; Di Cocco G; Evangelista Y; Ferrari A; Feroci M; Fiorini M; Froysland T; Fuschino F; Galli M; Gianotti F; Labanti C; Lapshov I; Lazzarotto F; Lipari P; Marisaldi M; Mastropietro M; Mereghetti S; Morelli E; Moretti E; Morselli A; Pellizzoni A; Perotti F; Piano G; Picozza P; Pilia M; Porrovecchio G; Prest M; Rapisarda M; Rappoldi A; Rubini A; Sabatini S; Soffitta P; Trifoglio M; Trois A; Vallazza E; Zambra A; Zanello D; Antonelli LA; Colafrancesco S; Giommi P; Pittori C; Verrecchia F; Santolamazza P; Salotti L
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/11585/595798
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