Aims. We report the gamma-ray activity from the intermediate BL Lac S5 0716+714 during observations acquired by the AGILE satellite in September and October 2007. These detections of activity were contemporaneous with a period of intense optical activity, which was monitored by GASP-WEBT. This simultaneous optical and gamma-ray coverage allows us to study in detail the light curves, time lags, gamma-ray photon spectrum, and Spectral Energy Distributions (SEDs) during different states of activity. Methods. AGILE observed the source with its two co-aligned imagers, the Gamma-Ray Imaging Detector ( GRID) and the hard X-ray imager (Super-AGILE), which are sensitive to the 30 MeV-50 GeV and 18-60 keV energy ranges, respectively. Observations were completed in two different periods, the first between 2007 September 4-23, and the second between 2007 October 24-November 1. Results. Over the period 2007 September 7-12, AGILE detected gamma-ray emission from the source at a significance level of 9.6-sigma with an average flux (E > 100 MeV) of ( 97 +/- 15) x 10(-8) photons cm(-2) s(-1), which increased by a factor of at least four within three days. No emission was detected by Super-AGILE for the energy range 18-60 keV to a 3-sigma upper limit of 10 mCrab in 335 ks. In October 2007, AGILE repointed toward S5 0716+714 following an intense optical flare, measuring an average flux of (47 +/- 11) x 10(-8) photons cm(-2) s(-1) at a significance level of 6.0-sigma. Conclusions. The gamma-ray flux of S5 0716+714 detected by AGILE is the highest ever detected for this blazar and one of the most intense gamma-ray fluxes detected from a BL Lac object. The SED of mid-September appears to be consistent with the synchrotron self-Compton (SSC) emission model, but only by including two SSC components of different variabilities.
AGILE detection of variable gamma-ray activity from the blazar S5 0716+714 in September-October 2007 / Chen AW; DAmmando F; Villata M; Raiteri CM; Tavani M; Vittorini V; Bulgarelli A; Donnarumma I; Ferrari A; Giuliani A; Longo F; Pacciani L; Pucella G; Vercellone S; Argan A; Barbiellini G; Boffelli F; Caraveo P; Carosati D; Cattaneo PW; Cocco V; Costa E; Del Monte E; De Paris G; Di Cocco G; Evangelista Y; Feroci M; Fiorini M; Froysland T; Frutti M; Fuschino F; Galli M; Gianotti F; Kurtanidze OM; Labanti C; Lapshov I; Larionov VM; Lazzarotto F; Lipari P; Marisaldi M; Mastropietro M; Mereghetti S; Morelli E; Morselli A; Pasanen M; Pellizzoni A; Perotti F; Picozza P; Porrovecchio G; Prest M; Rapisarda M; Rappoldi A; Rubini A; Soffitta P; Trifoglio M; Trois A; Vallazza E; Zambra A; Zanello D; Cutini S; Gasparrini D; Pittori C; Santolamazza P; Verrecchia F; Giommi P; Antonelli LA; Colafrancesco S; Salotti L. - In: ASTRONOMY & ASTROPHYSICS. - ISSN 0004-6361. - STAMPA. - 489:3(2008), pp. 37-41. [10.1051/0004-6361:200810553]
AGILE detection of variable gamma-ray activity from the blazar S5 0716+714 in September-October 2007
D'AMMANDO, FILIPPO;
2008
Abstract
Aims. We report the gamma-ray activity from the intermediate BL Lac S5 0716+714 during observations acquired by the AGILE satellite in September and October 2007. These detections of activity were contemporaneous with a period of intense optical activity, which was monitored by GASP-WEBT. This simultaneous optical and gamma-ray coverage allows us to study in detail the light curves, time lags, gamma-ray photon spectrum, and Spectral Energy Distributions (SEDs) during different states of activity. Methods. AGILE observed the source with its two co-aligned imagers, the Gamma-Ray Imaging Detector ( GRID) and the hard X-ray imager (Super-AGILE), which are sensitive to the 30 MeV-50 GeV and 18-60 keV energy ranges, respectively. Observations were completed in two different periods, the first between 2007 September 4-23, and the second between 2007 October 24-November 1. Results. Over the period 2007 September 7-12, AGILE detected gamma-ray emission from the source at a significance level of 9.6-sigma with an average flux (E > 100 MeV) of ( 97 +/- 15) x 10(-8) photons cm(-2) s(-1), which increased by a factor of at least four within three days. No emission was detected by Super-AGILE for the energy range 18-60 keV to a 3-sigma upper limit of 10 mCrab in 335 ks. In October 2007, AGILE repointed toward S5 0716+714 following an intense optical flare, measuring an average flux of (47 +/- 11) x 10(-8) photons cm(-2) s(-1) at a significance level of 6.0-sigma. Conclusions. The gamma-ray flux of S5 0716+714 detected by AGILE is the highest ever detected for this blazar and one of the most intense gamma-ray fluxes detected from a BL Lac object. The SED of mid-September appears to be consistent with the synchrotron self-Compton (SSC) emission model, but only by including two SSC components of different variabilities.I documenti in IRIS sono protetti da copyright e tutti i diritti sono riservati, salvo diversa indicazione.
