286 results on '"Vittorini, V."'
Search Results
2. The Bright $��$-ray Flare of 3C 279 in June 2015: AGILE Detection and Multifrequency Follow-up Observations
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Pittori, C., Lucarelli, F., Verrecchia, F., Raiteri, C. M., Villata, M., Vittorini, V., Tavani, M., Puccetti, S., Perri, M., Donnarumma, I., Vercellone, S., Acosta-Pulido, J. A., Bachev, R., Benitez, E., Borman, G. A., Carnerero, M. I., Carosati, D., Chen, W. P., Ehgamberdiev, Sh. A., Goded, A., Grishina, T. S., Hiriart, D., Hsiao, H. Y., Jorstad, S. G., Kimeridze, G. N., Kopatskaya, E. N., Kurtanidze, O. M., Kurtanidze, S. O., Larionov, V. M., Larionova, L. V., Marscher, A. P., Mirzaqulov, D. O., Morozova, D. A., Nilsson, K., Samal, M. R., Sigua, L. A., Spassov, B., Strigachev, A., Takalo, L. O., Antonelli, L. A., Bulgarelli, A., Cattaneo, P., Colafrancesco, S., Giommi, P., Longo, F., Morselli, A., and Paoletti, F.
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High Energy Astrophysical Phenomena (astro-ph.HE) ,Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics::Solar and Stellar Astrophysics ,FOS: Physical sciences - Abstract
We report the AGILE detection and the results of the multifrequency follow-up observations of a bright $��$-ray flare of the blazar 3C 279 in June 2015. We use AGILE-GRID and Fermi-LAT $��$-ray data, together with Swift-XRT, Swift-UVOT, and ground-based GASP-WEBT optical observations, including polarization information, to study the source variability and the overall spectral energy distribution during the $��$-ray flare. The $��$-ray flaring data, compared with as yet unpublished simultaneous optical data which allow to set constraints on the big blue bump disk luminosity, show very high Compton dominance values of $\sim 100$, with a ratio of $��$-ray to optical emission rising by a factor of three in a few hours. The multi-wavelength behavior of the source during the flare challenges one-zone leptonic theoretical models. The new observations during the June 2015 flare are also compared with already published data and non-simultaneous historical 3C 279 archival data., 13 pages, 5 figures,5 Tables. Accepted for publication in ApJ
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- 2018
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3. High spatial resolution correlation of AGILE TGFs and global lightning activity above the equatorial belt
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Fuschino F, Marisaldi M, Labanti C, Barbiellini G, Del Monte E, Bulgarelli A, Trifoglio M, Gianotti F, Galli M, Argan A, Trois A, Tavani M, Moretti E, Giuliani A, Longo F, Costa E, Caraveo P, Cattaneo PW, Chen A, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Lapshov I, Lazzarotto F, Lipari P, Mereghetti S, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Piano G, Pilia M, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rubini A, Sabatini S, Soffitta P, Striani E, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Antonelli LA, Colafrancesco S, Cutini S, Giommi P, Lucarelli F, Pittori C, Santolamazza P, Verrecchia F, Salotti L., D'AMMANDO, FILIPPO, F., Fuschino, M., Marisaldi, C., Labanti, G., Barbiellini, Monte, E., A., Bulgarelli, M., Trifoglio, F., Gianotti, M., Galli, A., Argan, A., Troi, M., Tavani, E., Moretti, A., Giuliani, Longo, Francesco, E., Costa, P., Caraveo, P. W., Cattaneo, A., Chen, F., D'Ammando, Paris, G., Cocco, G., Persio, G., I., Donnarumma, Y., Evangelista, M., Feroci, A., Ferrari, M., Fiorini, I., Lapshov, F., Lazzarotto, P., Lipari, S., Mereghetti, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, P., Picozza, G., Piano, M., Pilia, M., Prest, G., Pucella, M., Rapisarda, A., Rappoldi, A., Rubini, S., Sabatini, P., Soffitta, E., Striani, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, D., Zanello, L. A., Antonelli, S., Colafrancesco, S., Cutini, P., Giommi, F., Lucarelli, C., Pittori, P., Santolamazza, F., Verrecchia, L., Salotti, Fuschino F, Marisaldi M, Labanti C, Barbiellini G, Del Monte E, Bulgarelli A, Trifoglio M, Gianotti F, Galli M, Argan A, Trois A, Tavani M, Moretti E, Giuliani A, Longo F, Costa E, Caraveo P, Cattaneo PW, Chen A, DAmmando F, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Lapshov I, Lazzarotto F, Lipari P, Mereghetti S, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Picozza P, Piano G, Pilia M, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rubini A, Sabatini S, Soffitta P, Striani E, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Antonelli LA, Colafrancesco S, Cutini S, Giommi P, Lucarelli F, Pittori C, Santolamazza P, Verrecchia F, and Salotti L
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AGILE satellite ,terrestrial gamma ray flashes ,CsI calorimeter ,satellite optical observations ,global lightning ,Atmospheric Processes: Lightning ,Lightning [Atmospheric Processes] ,Atmospheric Processes: Atmospheric electricity ,AGILE, TGF, global lightning activity ,Atmospheric electricity [Atmospheric Processes] - Abstract
The AGILE satellite detects Terrestrial Gamma-ray Flashes (TGFs) in the 0.35-100 MeV energy range using its Mini-Calorimeter (MCAL) instrument with an average detection rate of 10 TGFs/month. Thanks to its Low Earth Orbit with only 2.5 degree of inclination, AGILE guarantees an unprecedented exposure above the equator, where both lightning activity and TGF detection peak. Here we report the comparison between the AGILE TGFs detected between March 2009 and February 2010 and full climatology lightning worldwide distribution based on satellite optical observations from LIS (Lightning Imaging Sensor) and OTD (Optical Transient Detector) instruments. This approach is complementary to the one-to-one TGF/lightning correlations by ground-based sferics measurements. Based on mono and bi-dimensional Kolmogorov-Smirnov tests, we show that the AGILE TGFs and time-averaged global lightning in the equatorial area are not drawn from the same distribution. However, we find significant regional differences in the degree of correlation as well as in the TGF/lightning ratio. In the case of south east Asia we find a 87% probability for the TGF and lightning being samples of the same distribution. This result supports the idea that the physical conditions at play in TGF generation can have strong geographical and climatological modulation. Based on the assumption that the observed range of TGF/flash ratio holds at all latitudes we can estimate a global rate of (N) over dot similar or equal to 220 divided by 570 TGFs per day. The observed TGF/flash geographical modulation as well as the TGF global rate estimate are in agreement with previous observations. Citation: Fuschino, F., et al. (2011), High spatial resolution correlation of AGILE TGFs and global lightning activity above the equatorial belt, Geophys. Res. Lett., 38, L14806, doi:10.1029/2011GL047817.
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- 2011
4. The AGILE Mission
- Author
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Tavani M, Barbiellini G, Argan A, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Costa E, Del Monte E, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Fornari F, Fuschino F, Froysland T, Frutti M, Galli M, Gianotti F, Giuliani A, Labanti C, Lapshov I, Lazzarotto F, Liello F, Lipari P, Longo F, Mattaini E, Marisaldi M, Mastropietro M, Mauri A, Mauri F, Mereghetti S, Morelli E, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Piano G, Picozza P, Pontoni C, Porrovecchio G, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rossi E, Rubini A, Soffitta P, Traci A, Trifoglio M, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Pittori C, Preger B, Santolamazza P, Verrecchia F, Giommi P, Colafrancesco S, Antonelli A, Cutini S, Gasparrini D, Stellato S, Fanari G, Primavera R, Tamburelli F, Viola F, Guarrera G, Salotti L, D'Amico F, Marchetti E, Crisconio M, Sabatini P, Annoni G, Alia S, Longoni A, Sanquerin R, Battilana M, Concari P, Dessimone E, Grossi R, Parise A, Monzani F, Artina E, Pavesi R, Marseguerra G, Nicolini L, Scandelli L, Soli L, Vettorello V, Zardetto E, Bonati A, Maltecca L, D'Alba E, Patane M, Babini G, Onorati F, Acquaroli L, Angelucci M, Morelli B, Agostara C, Cerone M, Michetti A, Tempesta P, D'Eramo S, Rocca F, Giannini F, Borghi G, Garavelli B, Conte M, Balasini M, Ferrario I, Vanotti M, Collavo E, Giacomazzo M., D'AMMANDO, FILIPPO, M., Tavani, G., Barbiellini, A., Argan, F., Boffelli, A., Bulgarelli, P., Caraveo, P. W., Cattaneo, A. W., Chen, V., Cocco, E., Costa, F., D'Ammando, E. D., Monte, G. D., Pari, G. D., Cocco, G. D., Persio, I., Donnarumma, Y., Evangelista, M., Feroci, A., Ferrari, M., Fiorini, F., Fornari, F., Fuschino, T., Froysland, M., Frutti, M., Galli, F., Gianotti, A., Giuliani, C., Labanti, I., Lapshov, F., Lazzarotto, F., Liello, P., Lipari, Longo, Francesco, E., Mattaini, M., Marisaldi, M., Mastropietro, A., Mauri, F., Mauri, S., Mereghetti, E., Morelli, A., Morselli, L., Pacciani, A., Pellizzoni, F., Perotti, G., Piano, P., Picozza, C., Pontoni, G., Porrovecchio, M., Prest, G., Pucella, M., Rapisarda, A., Rappoldi, E., Rossi, A., Rubini, P., Soffitta, A., Traci, M., Trifoglio, A., Troi, E., Vallazza, S., Vercellone, V., Vittorini, A., Zambra, D., Zanello, C., Pittori, B., Preger, P., Santolamazza, F., Verrecchia, P., Giommi, S., Colafrancesco, A., Antonelli, S., Cutini, D., Gasparrini, S., Stellato, G., Fanari, R., Primavera, F., Tamburelli, F., Viola, G., Guarrera, L., Salotti, F., D'Amico, E., Marchetti, M., Crisconio, P., Sabatini, G., Annoni, S., Alia, A., Longoni, R., Sanquerin, M., Battilana, P., Concari, E., Dessimone, R., Grossi, A., Parise, F., Monzani, E., Artina, R., Pavesi, G., Marseguerra, L., Nicolini, L., Scandelli, L., Soli, V., Vettorello, E., Zardetto, A., Bonati, L., Maltecca, E., D'Alba, M., Patane, G., Babini, F., Onorati, L., Acquaroli, M., Angelucci, B., Morelli, C., Agostara, M., Cerone, A., Michetti, P., Tempesta, S., D'Eramo, F., Rocca, F., Giannini, G., Borghi, B., Garavelli, M., Conte, M., Balasini, I., Ferrario, M., Vanotti, E., Collavo, M., Giacomazzo, Tavani M, Barbiellini G, Argan A, Boffelli F, Bulgarelli A, Caraveo P, Cattaneo PW, Chen AW, Cocco V, Costa E, DAmmando F, Del Monte E, De Paris G, Di Cocco G, Di Persio G, Donnarumma I, Evangelista Y, Feroci M, Ferrari A, Fiorini M, Fornari F, Fuschino F, Froysland T, Frutti M, Galli M, Gianotti F, Giuliani A, Labanti C, Lapshov I, Lazzarotto F, Liello F, Lipari P, Longo F, Mattaini E, Marisaldi M, Mastropietro M, Mauri A, Mauri F, Mereghetti S, Morelli E, Morselli A, Pacciani L, Pellizzoni A, Perotti F, Piano G, Picozza P, Pontoni C, Porrovecchio G, Prest M, Pucella G, Rapisarda M, Rappoldi A, Rossi E, Rubini A, Soffitta P, Traci A, Trifoglio M, Trois A, Vallazza E, Vercellone S, Vittorini V, Zambra A, Zanello D, Pittori C, Preger B, Santolamazza P, Verrecchia F, Giommi P, Colafrancesco S, Antonelli A, Cutini S, Gasparrini D, Stellato S, Fanari G, Primavera R, Tamburelli F, Viola F, Guarrera G, Salotti L, D'Amico F, Marchetti E, Crisconio M, Sabatini P, Annoni G, Alia S, Longoni A, Sanquerin R, Battilana M, Concari P, Dessimone E, Grossi R, Parise A, Monzani F, Artina E, Pavesi R, Marseguerra G, Nicolini L, Scandelli L, Soli L, Vettorello V, Zardetto E, Bonati A, Maltecca L, D'Alba E, Patane M, Babini G, Onorati F, Acquaroli L, Angelucci M, Morelli B, Agostara C, Cerone M, Michetti A, Tempesta P, D'Eramo S, Rocca F, Giannini F, Borghi G, Garavelli B, Conte M, Balasini M, Ferrario I, Vanotti M, Collavo E, and Giacomazzo M
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Agile ,Active galactic nucleus ,gamma and X ray detection ,Astrophysics::High Energy Astrophysical Phenomena ,media_common.quotation_subject ,satellite ,FOS: Physical sciences ,Astrophysics ,High Energy Gamma-ray Astronomy ,Pulsar ,astro-ph ,Angular resolution ,media_common ,Physics ,Calorimeter (particle physics) ,Astrophysics (astro-ph) ,Detector ,AGILE satellite ,Detectors ,Astronomy and Astrophysics ,Universe ,Supernova ,Space and Planetary Science ,Orbit (dynamics) ,instrumentation: detectors – techniques: high angular resolution – techniques: image processing – gamma rays: observations – X-rays: general - Abstract
AGILE is an Italian Space Agency mission dedicated to the observation of the gamma-ray Universe. The AGILE very innovative instrumentation combines for the first time 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) together with a Calorimeter (sensitive in the range 300 keV - 100 MeV) and an anticoincidence system. AGILE was successfully launched on April 23, 2007 from the Indian base of Sriharikota and was inserted in an equatorial orbit with a very low particle background. 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. An optimal angular resolution (reaching 0.1-0.2 degrees in gamma-rays, 1-2 arcminutes 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. The paper describes the AGILE Mission and its space and ground segments., 20 pages, 26 figures. submitted to Astron. & Astrophys
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- 2009
5. The Osmosys approach to multiformalism modelling of system
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FRANCESCHINIS G, IACONO M, VITTORINI V., MAZZOCCA, NICOLA, Franceschinis, G, Iacono, M, Mazzocca, Nicola, and Vittorini, V.
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- 2003
6. An Experience in Railway interlocking Systems Specification and Formal Verification
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CHIANESE R., LAZZARO A., MARMO P, PAPA D., VITTORINI V., MAZZOCCA, NICOLA, G. TARNAI, E. SCHNIEDER, Chianese, R., Lazzaro, A., Marmo, P., Mazzocca, N., Papa, D., Vittorini, Valeria, G. TARNAI E. SCHNIEDER, Marmo, P, Mazzocca, Nicola, and Vittorini, V.
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- 2003
7. An Experience in Railway interlocking System Specification and formal Verification
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CHIANESE R, LAZZARO A, MARMO P, PAPA D, VITTORINI V., MAZZOCCA, NICOLA, Chianese, R, Lazzaro, A, Marmo, P, Mazzocca, Nicola, Papa, D, and Vittorini, V.
- Abstract
L'Harmattan Hongrie publisher
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- 2003
8. Transient Gamma-ray Emission from Cygnus X-3 Detected by AGILE: Leptonic and Hadronic Emission Models
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Piano, G., Tavani, M., Vittorini, V., and Giuliani, A.
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High Energy Astrophysical Phenomena (astro-ph.HE) ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
The AGILE satellite detected several episodes of transient gamma-ray emission from Cygnus X-3. Cross-correlating the AGILE light curve with both X-ray and radio monitoring data, we found that the main events of gamma-ray activity were detected while the system was in soft spectral X-ray states, that coincide with local and often sharp minima of the hard X-ray flux, a few days before intense radio outbursts. This repetitive temporal coincidence between the gamma-ray transient emission and spectral state changes of the source turns out to be the spectral signature of high-energy activity from this microquasar. The gamma-ray differential spectrum of Cygnus X-3 (100 MeV - 3 GeV), which was obtained by averaging the data collected by AGILE during the gamma-ray events, is consistent with a power law of photon index {\alpha} = 2.0 +/- 0.2. Finally, we examined leptonic and hadronic emission models for the gamma-ray activity and found that both scenarios are valid. In particular, in the leptonic model - based on inverse Compton scatterings of mildly relativistic electrons on soft photons from both the Wolf-Rayet companion star and the accretion disk - the emitting particles may also contribute to the overall hard X-ray spectrum, possibly explaining the hard non-thermal power-law tail seen during special soft X-ray states in Cygnus X-3., Comment: 2012 Fermi Symposium proceedings - eConf C121028
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- 2013
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9. Efficient Model checking of properties of a distribuited application: a multimedia case study
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MAZZOCCA, NICOLA, SANTONE A, VAGLINI G, VITTORINI V., Mazzocca, Nicola, Santone, A, Vaglini, G, and Vittorini, V.
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- 2002
10. First results about on-ground calibration of the Silicon Tracker for the AGILE satellite
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AGILE Collaboration, Cattaneo, P. W., Argan, A., Boffelli, F., Bulgarelli, A., Buonomo, B., Chen, A. W., D'Ammando, F., Froysland, T., Fuschino, F., Galli, M., Gianotti, F., Giuliani, A., Longo, F., Marisaldi, M., Mazzitelli, G., Pellizzoni, A., Prest, M., Pucella, G., Quintieri, L., Rappoldi, A., Tavani, M., Trifoglio, M., Trois, A., Valente, P., Vallazza, E., Vercellone, S., Zambra, A., Barbiellini, G., Caraveo, P., Cocco, V., Costa, E., De Paris, G., Del Monte, E., Di Cocco, G., Donnarumma, I., Evangelista, Y., Feroci, M., Ferrari, A., Fiorini, M., Labanti, C., Lapshov, I., Lazzarotto, F., Lipari, P., Mastropietro, M., Mereghetti, S., Morelli, E., Moretti, E., Morselli, A., Pacciani, L., Perotti, F., Piano, G., Picozza, P., Pilia, M., Porrovecchio, G., Rapisarda, M., Rubini, A., Sabatini, S., Soffitta, P., Striani, E., Vittorini, V., Zanello, D., Colafrancesco, S., Giommi, P., Pittori, C., Santolamazza, P., Verrecchia, F., and Salotti, L.
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Physics - Instrumentation and Detectors ,Physics::Instrumentation and Detectors ,Astrophysics::Instrumentation and Methods for Astrophysics ,Physics::Accelerator Physics ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,Astrophysics - Instrumentation and Methods for Astrophysics ,Nuclear Experiment ,physics.ins-det ,Instrumentation and Methods for Astrophysics (astro-ph.IM) ,astro-ph.IM - Abstract
The AGILE scientific instrument has been calibrated with a tagged $\gamma$-ray beam at the Beam Test Facility (BTF) of the INFN Laboratori Nazionali di Frascati (LNF). The goal of the calibration was the measure of the Point Spread Function (PSF) as a function of the photon energy and incident angle and the validation of the Monte Carlo (MC) simulation of the silicon tracker operation. The calibration setup is described and some preliminary results are presented., Comment: Presented at the 2nd Roma International Conference on Astroparticle Physics 2009, Villa Mondragone, Rome, Italy, May 13-15 2009. Pages 6, Figures 10
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- 2011
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11. AGILE monitoring of the microquasar Cygnus X-3
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Piano, G., Bulgarelli, A., Tavani, M., Vittorini, V., McCollough, M., Pooley, G., and Trushkin, S.
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High Energy Astrophysical Phenomena (astro-ph.HE) ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
AGILE data on Cygnus X-3 are reviewed focussing on the correlation between the production of gamma-ray transient emission and spectral state changes of the source. AGILE clearly establishes a relation between enhanced gamma-ray emission and the "quenched" radio/hard X-ray states that precede in general major radio flares. We briefly discuss the theoretical implications of our findings., Comment: 2011 Fermi Symposium proceedings - eConf C110509
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- 2011
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12. AGILE detection of Cygnus X-3 ��-ray active states during the period mid-2009/mid-2010
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Bulgarelli, A., Tavani, M., Chen, A. W., Evangelista, Y., Trifoglio, M., Gianotti, F., Piano, G., Sabatini, S., Striani, E., Pooley, G., Trushkin, S., Nizhelskij, N. A., McCollough, M., Koljonen, K. I. I., Hannikainen, D., L��hteenm��ki, A., Tammi, J., Lavonen, N., Steeghs, D., Aboudan, A., Argan, A., Barbiellini, G., Campana, R., Caraveo, P., Cattaneo, P. W., Cocco, V., Contessi, T., Costa, E., D'Ammando, F., Del Monte, E., De Paris, G., Di Cocco, G., Donnarumma, I., Feroci, M., Fiorini, M., Fuschino, F., Galli, M., Giuliani, A., Giusti, M., Labanti, C., Lapshov, I., Lazzarotto, F., Lipari, P., Longo, F., Marisaldi, M., Mereghetti, S., Morelli, E., Moretti, E., Morselli, A., Pacciani, L., Pellizzoni, A., Perotti, F., Picozza, P., Pilia, M., Prest, M., Pucella, G., Rapisarda, M., Rappoldi, A., Rubini, A., Soffitta, P., Trois, A., Vallazza, E., Vercellone, S., Vittorini, V., Zambra, A., Zanello, D., Giommi, P., Pittori, C., Verrecchia, F., Santolamazza, P., Lucarelli, F., Colafrancesco, S., and Salotti, L.
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High Energy Astrophysical Phenomena (astro-ph.HE) ,FOS: Physical sciences - Abstract
Cygnus X-3 (Cyg X-3) is a well-known microquasar producing variable emission at all wavelengths. Cyg X-3 is a prominent X-ray binary producing relativistic jets, and studying its high energy emission is crucial for the understanding of the fundamental acceleration processes in accreting compact objects. Aims. Our goal is to study extreme particle acceleration and ��-ray production above 100 MeV during special spectral states of Cyg X- 3 usually characterized by a low hard X-ray flux and enhanced soft X-ray states. We observed Cyg X-3 with the AGILE satellite in extended time intervals from 2009 Jun.-Jul., and 2009 Nov.-2010 Jul. We report here the results of the AGILE ��-ray monitoring of Cyg X-3 as well as the results from extensive multiwavelength campaigns involving radio (RATAN-600, AMI-LA and Mets��hovi Radio Observatories) and X-ray monitoring data (XTE and Swift). We detect a series of repeated ��-ray flaring activity from Cyg X-3 that correlate with the soft X-ray states and episodes of decreasing or non-detectable hard X-ray emission. Furthermore, we detect ��-ray enhanced emission that tends to be associated with radio flares greater than 1 Jy at 15 GHz, confirming a trend already detected in previous observations. The source remained active above 100 MeV for an extended period of time (almost 1.5 months in 2009 Jun.-Jul. and 1 month in 2010 May). We study in detail the short timescale ��-ray flares that occurred before or near the radio peaks. Our results confirm the transient nature of the extreme particle acceleration from the microquasar Cyg X-3. A series of repeated ��-ray flares shows correlations with radio and X-ray emission confirming a well established trend of emission. We compare our results with Fermi-LAT and MAGIC TeV observations of Cyg X-3., 16 pages, 8 figures, 7 tables; A&A (2011)
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- 2011
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13. Characterization of a tagged $��$-ray beam line at the DA$��$NE Beam Test Facility
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Cattaneo, P. W., Argan, A., Boffelli, F., Bulgarelli, A., Buonomo, B., Chen, A. W., D'Ammando, F., Froysland, T., Fuschino, F., Galli, M., Gianotti, F., Giuliani, A., Longo, F., Marisaldi, M., Mazzitelli, G., Pellizzoni, A., Prest, M., Pucella, G., Quintieri, L., Rappoldi, A., Tavani, M., Trifoglio, M., Trois, A., Valente, P., Vallazza, E., Vercellone, S., Zambra, A., Barbiellini, G., Caraveo, P., Cocco, V., Costa, E., De Paris, G., Del Monte, E., Di Cocco, G., Donnarumma, I., Evangelista, Y., Feroci, M., Ferrari, A., Fiorini, M., Labanti, C., Lapshov, I., Lazzarotto, F., Lipari, P., Mastropietro, M., Mereghetti, S., Morelli, E., Moretti, E., Morselli, A., Pacciani, L., Perotti, F., Piano, G., Picozza, P., Pilia, M., Porrovecchio, G., Rapisarda, M., Rubini, A., Sabatini, S., Soffitta, P., Striani, E., Vittorini, V., Zanello, D., Colafrancesco, S., Giommi, P., Pittori, C., Santolamazza, P., Verrecchia, F., and Salotti, L.
- Subjects
Physics::Instrumentation and Detectors ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Instrumentation and Detectors (physics.ins-det) ,Instrumentation and Methods for Astrophysics (astro-ph.IM) - Abstract
At the core of the AGILE scientific instrument, designed to operate on a satellite, there is the Gamma Ray Imaging Detector (GRID) consisting of a Silicon Tracker (ST), a Cesium Iodide Mini-Calorimeter and an Anti-Coincidence system of plastic scintillator bars. The ST needs an on-ground calibration with a $��$-ray beam to validate the simulation used to calculate the energy response function and the effective area versus the energy and the direction of the $��$ rays. A tagged $��$-ray beam line was designed at the Beam Test Facility (BTF) of the INFN Laboratori Nazionali of Frascati (LNF), based on an electron beam generating $��$ rays through bremsstrahlung in a position-sensitive target. The $��$-ray energy is deduced by difference with the post-bremsstrahlung electron energy \cite{prest}-\cite{hasan}. The electron energy is measured by a spectrometer consisting of a dipole magnet and an array of position sensitive silicon strip detectors, the Photon Tagging System (PTS). The use of the combined BTF-PTS system as tagged photon beam requires understanding the efficiency of $��$-ray tagging, the probability of fake tagging, the energy resolution and the relation of the PTS hit position versus the $��$-ray energy. This paper describes this study comparing data taken during the AGILE calibration occurred in 2005 with simulation., 23 pages; 17 figures. Second and final version accepted by Nucl. Instr. & Meth. A
- Published
- 2011
- Full Text
- View/download PDF
14. AGILE detection of extreme gamma-ray activity from the blazar PKS 1510-089 during March 2009
- Author
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D'Ammando, F., Raiteri, C. M., Villata, M., Romano, P., Pucella, G., Krimm, H. A., Covino, S., Orienti, M., Giovannini, G., Vercellone, S., Pian, E., Donnarumma, I., Vittorini, V., Tavani, M., Argan, A., Barbiellini, G., Boffelli, F., Bulgarelli, A., Caraveo, P., Cattaneo, P. W., Chen, A. W., Cocco, V., Costa, E., Del Monte, E., De Paris, G., Di Cocco, G., Evangelista, Y., Feroci, M., Ferrari, A., Fiorini, M., Froysland, T., Frutti, M., Fuschino, F., Galli, M., Gianotti, F., Giuliani, A., Labanti, C., Lapshov, I., Lazzarotto, F., Lipari, P., Longo, F., Marisaldi, M., Mereghetti, S., Morselli, A., Pacciani, L., Pellizzoni, A., Perotti, F., Piano, G., Picozza, P., Pilia, M., Porrovecchio, G., Prest, Michela, Rapisarda, M., Rappoldi, A., Rubini, A., Sabatini, S., Soffitta, P., Striani, E., Trifoglio, M., Trois, A., Vallazza, E., Zambra, A., Zanello, D., Agudo, I., Aller, H. D., Aller, M. F., Arkharov, A. A., Bach, U., Benitez, E., Berdyugin, A., Blinov, D. A., Buemi, C. S., Chen, W. P., Di Paola, A., Dolci, M., Forne, E., Fuhrmann, L., Gomez, J. L., Gurwell, M. A., Jordan, B., Jorstad, S. G., Heidt, J., Hiriart, D., Hovatta, T., Hsiao, H. Y., Kimeridze, G., Konstantinova, T. S., Kopatskaya, E. N., Koptelova, E., Kurtanidze, O. M., Kurtanidze, S. O., Larionov, V. M., Lahteenmaki, A., Leto, P., Lindfors, E., Marscher, A. P., Mcbreen, B., Mchardy, I. M., Morozova, D. A., Nilsson, K., Pasanen, M., Roca Sogorb, M., Sillanpaa, A., Takalo, L. O., Tornikoski, M., Trigilio, C., Troitsky, I. S., Umana, G., Antonelli, L. A., Colafrancesco, S., Pittori, C., Santolamazza, P., Verrecchia, F., Giommi, P., and Salotti, L.
- Subjects
radio quasar PKS 1510-089 ,AGILE satellite ,gamma-ray ,observations from UV to hard X-ray and radio - Published
- 2011
15. AGILE detection of extreme γ-ray activity from the blazar PKS 1510-089 during March 2009. Multifrequency analysis
- Author
-
D' Ammando, F, Raiteri, C, Villata, M, Romano, P, Pucella, G, Krimm, H, Covino, S, Orienti, M, Giovannini, G, Vercellone, S, Pian, E, Donnarumma, I, Vittorini, V, Tavani, M, Argan, A, Barbiellini, G, Boffelli, F, Bulgarelli, A, Caraveo, P, Cattaneo, P, Chen, A, Cocco, V, Costa, E, Del Monte, E, de Paris, G, Di Cocco, G, Evangelista, Y, Feroci, M, Ferrari, A, Fiorini, M, Froysland, T, Frutti, M, Fuschino, F, Galli, M, Gianotti, F, Giuliani, A, Labanti, C, Lapshov, I, Lazzarotto, F, Lipari, P, Longo, F, Marisaldi, M, Mereghetti, S, Morselli, A, Pacciani, L, Pellizzoni, A, Perotti, F, Piano, G, Picozza, P, Pilia, M, Porrovecchio, G, Prest, M, Rapisarda, M, Rappoldi, A, Rubini, A, Sabatini, S, Soffitta, P, Striani, E, Trifoglio, M, Trois, A, Vallazza, E, Zambra, A, Zanello, D, Agudo, I, Aller, H, Aller, M, Arkharov, A, Bach, U, Benitez, E, Berdyugin, A, Blinov, D, Buemi, C, Chen, W, di Paola, A, Dolci, M, Forn#232, E, Fuhrmann, L, G#242, Mez, J, Gurwell, M, Jordan, B, Jorstad, S, Heidt, J, Hiriart, D, Hovatta, T, Hsiao, H, Kimeridze, G, Konstantinova, T, Kopatskaya, E, Koptelova, E, Kurtanidze, O, Kurtanidze, S, Larionov, V, Lahteenmaki, A, Leto, P, Lindfors, E, Marscher, A, Mcbreen, B, Mchardy, I, Morozova, D, Nilsson, K, Pasanen, M, Roca Sogorb, M, Sillanpaa, A, Takalo, L, Tornikoski, M, Trigilio, Corrado, Troitsky, I, Umana, G, Antonelli, L, Colafrancesco, S, Pittori, C, Santolamazza, P, Verrecchia, F, Giommi, P, and Salotti, L.
- Published
- 2011
16. Nets building Blocks
- Author
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BASILE F, CHIACCHIO P, VITTORINI V., MAZZOCCA, NICOLA, Basile, F, Chiacchio, P, Mazzocca, Nicola, and Vittorini, V.
- Abstract
Los Angeles USA
- Published
- 1999
17. Efficient Model Checking of Properties of a Multimedia Application
- Author
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Mazzocca, M., Santone, A., Vaglini, Gigliola, VITTORINI V., DE FRANCESCO, A, Mazzocca, Nicola, Vaglini, G, and Vittorini, V.
- Abstract
North Falmouth, Massachusetts (USA)
- Published
- 1999
18. Modelling Flexible Manufacturing System: a Petri NEt Modular Approach
- Author
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BASILE P, CHIACCHIO N, VITTORINI V., MAZZOCCA, NICOLA, Basile, P, Chiacchio, N, Mazzocca, Nicola, and Vittorini, V.
- Abstract
Zaragoza, Spain
- Published
- 1999
19. Building formal models of concurrent and distribited system: an experience in applicability with two different Petri nets approaches
- Author
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MAZZOCCA, NICOLA, RUSSO S, VITTORINI V., Mazzocca, Nicola, Russo, S, and Vittorini, V.
- Published
- 1999
20. The December 2009 gamma-ray flare of 3C 454.3: the multifrequency campaign
- Author
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Pacciani, L., Vittorini, V., Tavani, M., Fiocchi, M. T., Vercellone, S., D'Ammando, F., Sakamoto, T., Pian, E., Raiteri, C. M., Villata, M., Sasada, M., Itoh, R., Yamanaka, M., Uemura, M., Striani, E., Fugazza, D., Tiengo, A., Krimm, H. A., Stroh, M. C., Falcone, A. D., Curran, P. A., Sadun, A. C., Lahteenmaki, A., Tornikoski, M., Aller, H. D., Aller, M. F., Lin, C. S., Larionov, V. M., Leto, P., Takalo, L. O., Berdyugin, A., Gurwell, M. A., Bulgarelli, A., Chen, A. W., Donnarumma, I., Giuliani, A., Longo, F., Pucella, G., Argan, A., Caraveo, G. Barbiellini P., Cattaneo, P. W., Cocco, V., Costa, E., De Paris, G., Del Monte, E., Di Cocco, G., Evangelista, Y., Ferrari, A., Feroci, M., Fiorini, M., Fuschino, F., Galli, M., Gianotti, F., Labanti, C., Lapshov, I., Lazzarotto, F., Lipari, P., Marisaldi, M., Mereghetti, S., Morelli, E., Moretti, E., Morselli, A., Pellizzoni, A., Perotti, F., Piano, G., Picozza, P., Pilia, M., Prest, M., Rapisarda, M., Rappoldi, A., Rubini, A., Sabatini, S., Soffitta, P., Trifoglio, M., Trois, A., Vallazza, E., Zanello, D., Colafrancesco, S., Pittori, C., Verrecchia, F., Santolamazza, P., Lucarelli, F., Giommi, P., and Salotti, L.
- Subjects
Cosmology and Nongalactic Astrophysics (astro-ph.CO) ,Astrophysics::High Energy Astrophysical Phenomena ,FOS: Physical sciences ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics - Cosmology and Nongalactic Astrophysics - Abstract
During the month of December, 2009 the blazar 3C 454.3 became the brightest gamma-ray source in the sky, reaching a peak flux F ~2000E-8 ph/cm2/s for E > 100 MeV. Starting in November, 2009 intensive multifrequency campaigns monitored the 3C 454 gamma-ray outburst. Here we report the results of a 2-month campaign involving AGILE, INTEGRAL, Swift/XRT, Swift/BAT, RossiXTE for the high-energy observations, and Swift/UVOT, KANATA, GRT, REM for the near-IR/optical/UV data. The GASP/WEBT provided radio and additional optical data. We detected a long-term active emission phase lasting ~1 month at all wavelengths: in the gamma-ray band, peak emission was reached on December 2-3, 2009. Remarkably, this gamma-ray super-flare was not accompanied by correspondingly intense emission in the optical/UV band that reached a level substantially lower than the previous observations in 2007-2008. The lack of strong simultaneous optical brightening during the super-flare and the determination of the broad-band spectral evolution severely constrain the theoretical modelling. We find that the pre- and post-flare broad-band behavior can be explained by a one-zone model involving SSC plus external Compton emission from an accretion disk and a broad-line region. However, the spectra of the Dec. 2-3, 2009 super-flare and of the secondary peak emission on Dec. 9, 2009 cannot be satisfactorily modelled by a simple one-zone model. An additional particle component is most likely active during these states., 21 pages, 2 figures, ApJL accepted
- Published
- 2010
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21. AGILE and blazar studies
- Author
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Marisaldi, M., D Ammando, F., Vercellone, S., Donnarumma, I., Bulgarelli, A., Andrew Chen, Giuliani, A., Longo, F., Pacciani, L., Pucella, G., Tavani, M., and Vittorini, V.
- Subjects
High Energy Astrophysical Phenomena (astro-ph.HE) ,FOS: Physical sciences ,Astrophysics - High Energy Astrophysical Phenomena - Abstract
During the first two years of observation, AGILE detected several blazars at high significance: 3C 279, 3C 454.3, PKS 1510-089, S5 0716+714, 3C 273, W Comae, Mrk 421 and PKS 0537-441. We obtained long-term coverage of 3C 454.3, for a total of more than three months at energies above 100 MeV. 3C 273 was the first blazar detected simultaneously by the AGILE gamma-ray detector and by its hard X-ray monitor. S5 0716+714, an intermediate BL Lac object, exhibited a very fast and intense gamma-ray transient during an optical high-state phase, challenging the current theoretical models for energy extraction from a rotating black hole, while W Comae and Mkn 421 were detected during an AGILE Target of Opportunity (ToO) repointing, and were simultaneously detected by Cherenkov telescopes. Thanks to the rapid dissemination of our alerts, we were able to obtain multi-wavelength ToO data from other observatories such as Spitzer, Swift, RXTE, Suzaku, INTEGRAL, MAGIC, VERITAS, as well as radio-to-optical coverage by means of the WEBT Consortium and REM, allowing us to study truly simultaneous spectral energy distributions from the radio to the TeV energy band., Comment: 4 pages, 5 figures, conference proceedings of the ICRC 2009
- Published
- 2009
- Full Text
- View/download PDF
22. Formal specifications of concurrent systems: a structured approach
- Author
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MAZZEO A., MAZZOCCA N., RUSSO S., VITTORINI V., SAVY, CARLO, Mazzeo, A., Mazzocca, N., Russo, S., Savy, Carlo, and Vittorini, V.
- Abstract
Oxford University Press - British Computer Society, Oxford, UK
- Published
- 1998
23. AGILE detection of variable gamma-ray activity from the blazar S5 0716+714 during September-October 2007
- Author
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D'Ammando, F., Chen, A. W., Villata, M., Raiteri, C. M., Vittorini, V., Bulgarelli, A., Donnarumma, I., Giuliani, A., Longo, F., Pacciani, L., Pucella, G., Tavani, M., and Vercellone, S.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,FOS: Physical sciences ,Astrophysics - Abstract
We report the gamma-ray activity from the Intermediate BL Lac S5 0716+714 during 2007 September-October observations by the AGILE satellite, coincident with a period of intense optical activity of the source monitored by GASP-WEBT. AGILE observed the source with its two co-aligned imagers, the Gamma-Ray Imaging Detector (GRID) and the hard X-ray imager (Super-AGILE) sensitive in the energy range 30 MeV-50 GeV and 18-60 keV respectively, in two different periods: the first between 4 and 23 September 2007, the second between 24 October and 1 November 2007. Over the period 7-12 September, 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}, increasing by a factor of at least four within three days. No emission was detected by Super-AGILE in the energy range 18-60 keV, with a 3-sigma upper limit of 10 mCrab in 335 ksec. 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 Spectral Energy Distribution (SED) of mid-September seems to be consistent with the synchrotron self-Compton (SSC) emission model, but only by including two SSC components with different variability. 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. The gamma-ray flux during both AGILE pointings appears to be highly variable on timescales of 1 day., 8 pages, 4 figures, "Workshop on Blazar Variability across the Electromagnetic Spectrum", 2008 April 22-25, Palaiseau, France
- Published
- 2008
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- View/download PDF
24. A Systematic Approach to the Petri Net Based Specifications of Concurrent Systems
- Author
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MAZZEO, ANTONINO, MAZZOCCA N., RUSSO S., VITTORINI V., Mazzeo, A., Mazzocca, N., Russo, S., Vittorini, Valeria, Mazzeo, A, Mazzocca, Nicola, Vittorini, V., and Mazzeo, Antonino
- Published
- 1997
25. Formal methods integration for the specification of dependable distributed system
- Author
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MAZZOCCA, NICOLA, RUSSO S., VITTORINI V., Mazzocca, Nicola, Russo, S., and Vittorini, V.
- Published
- 1997
26. A systematic approach to the Petri net based specification of concurrent systems
- Author
-
MAZZEO A., MAZZOCCA N., VITTORINI V., RUSSO, STEFANO, Mazzeo, A., Mazzocca, N., Russo, Stefano, and Vittorini, V.
- Published
- 1997
27. A method for predictive performance evaluation of distributed programs
- Author
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MAZZEO A., RUSSO S., VITTORINI V., MAZZOCCA, NICOLA, Mazzeo, A., Mazzocca, N., Russo, Stefano, Vittorini, V., Mazzocca, Nicola, and Russo, S.
- Published
- 1997
28. A parallel graph-traversing procedure for multicomputer architectures
- Author
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MAZZEO A., MAZZOCCA N., VITTORINI V., SFORZA, ANTONIO, VALERO M., ONATE E., JANE M., LARRIBA J.L., SUAREZ B., Mazzeo, A., Mazzocca, N., Sforza, Antonio, and Vittorini, V.
- Published
- 1992
29. The Rise and Fall of the Quasars
- Author
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Cavaliere, A. and Vittorini, V.
- Subjects
Astrophysics::High Energy Astrophysical Phenomena ,Astrophysics (astro-ph) ,Astrophysics::Solar and Stellar Astrophysics ,FOS: Physical sciences ,Astrophysics::Earth and Planetary Astrophysics ,Astrophysics::Cosmology and Extragalactic Astrophysics ,Astrophysics ,Astrophysics::Galaxy Astrophysics - Abstract
The coherent rise and fall of the quasar population is discussed in terms of gas accretion onto massive black holes, governed by the hierarchically growing environment. The rise is related to plentiful accretion during the assemblage of the host galaxies; the fall to intermittent accretion when these interact with companions in a group. The LFs are computed out to z=6, and are related to the mass distribution of relict BH found in local galaxies. The histories of the QS and of the star light are compared., Comment: 8 pages latex, paspconf.sty. To be published in ``The Young Universe'' Eds. S. D'Odorico, A. Fontana & E. Giallongo ASP Conf. Series 1998. With corrected references and figure captions
- Published
- 1998
- Full Text
- View/download PDF
30. Evaluating the Hazardous Failure Rate of majority voting computer architectures by means of Bayesian Network models
- Author
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Flammini, F., Stefano Marrone, Mazzocca, N., Vittorini, V., Flammini, F, Marrone, Stefano, Mazzocca, N, Vittorini, V., T. Aven, J. E. Vinnem, F., Flammini, S., Marrone, Mazzocca, Nicola, and Vittorini, Valeria
- Subjects
Voting system ,TMR ,Bayesian Network ,Safety analysis - Abstract
Safety-critical control systems are usually based on majority voters. In order to assess the compliance of these architectures with international safety standards, the probability of the occurrence of unsafe events should be evaluated by developing and analyzing proper formal models. In this paper we demonstrate that a Bayesian Network (BN) model can be used to evaluate the Mean Time Between Hazardous Events (MTBHE) of voting architectures. The proposed modeling approach is applied to a “2 out of 2” (2oo2) voter consisting of independent computing units. The results obtained from the analysis of the BN model of the 2oo2 voter can be easily extended to evaluate the hazardous failure rate of more complex voting architectures (e.g. Triple Modular Redundant architectures, based on a 2oo3 voting).
31. Building formal models of concurrent and distributed systems: An experience in applicability with two different Petri nets approaches
- Author
-
Nicola Mazzocca, Russo, S., Vittorini, V., Mazzocca, N, Russo, Stefano, and Vittorini, V.
- Subjects
Formal methods, Railway interlocking - Abstract
This paper presents an experience in building formal models for the specification and design of concurrent and distributed systems. In particular our work is oriented to state the real applicability of formal methods in industrial settings, where practical engineering means are needed in modeling and evaluating complex systems. Here a standard voting system is used to compare a SAN-based and an event driven GSPN based approach.
32. Modeling system reliability aspects of ERTMS/ETCS by fault trees and Bayesian networks
- Author
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Flammini, F., Marrone, S., Nicola Mazzocca, Vittorini, V., Flammini, F, Marrone, Stefano, Mazzocca, N, and Vittorini, V.
33. AGILE detection of a possible rebrightening of the gamma-ray source AGL J2021+4032 in the Cygnus Region
- Author
-
Tavani, M., Piano, G., Chen, A., Giuliani, A., Bulgarelli, A., D Ammando, F., Pucella, G., Vittorini, V., Costa, E., Feroci, M., Donnarumma, I., Pacciani, L., Del Monte, E., Lazzarotto, F., Soffitta, P., Evangelista, Y., Lapshov, I., Rapisarda, M., Argan, A., Trois, A., Paris, G., Marisaldi, M., Gianotti, F., Trifoglio, M., Di Cocco, G., Labanti, C., Fuschino, F., Galli, M., Caraveo, P., Mereghetti, S., Alberto Paolo Pellizzoni, Vercellone, S., Perotti, F., Fiorini, M., Zambra, A., Barbiellini, G., Longo, F., Vallazza, E., Picozza, P., Morselli, A., Sabatini, S., Prest, M., Lipari, P., Zanello, D., Cattaneo, P., Gasparrini, D., Pittori, C., Verrecchia, F., Preger, B., Santolamazza, P., Colafrancesco, S., Giommi, P., and Salotti, L.
34. AGILE detection of a gamma-ray flare from the blazar 3C 273
- Author
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Pacciani, L., Verrecchia, F., Donnarumma, I., Pittori, C., Tavani, M., Bulgarelli, A., Gianotti, F., Trifoglio, M., Striani, E., Vercellone, S., D Ammando, F., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Argan, A., Piano, G., Pucella, G., Sabatini, S., Trois, A., Vittorini, V., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Di Cocco, G., Chen, A., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Alberto Paolo Pellizzoni, Pilia, M., Barbiellini, G., Longo, F., Moretti, E., Vallazza, E., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Lucarelli, F., Santolamazza, P., Colafrancesco, S., Giommi, P., and Salotti, L.
35. AGILE detection of enhanced gamma-ray emission from the blazar PKS 1510-089
- Author
-
Striani, E., Verrecchia, F., Tavani, M., Vercellone, S., D Ammando, F., Del Monte, E., Donnarumma, I., Evangelista, Y., Feroci, M., Lazzarotto, F., Pacciani, L., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Argan, A., Piano, G., Pucella, G., Sabatini, S., Trois, A., Vittorini, V., Andrea Bulgarelli, Gianotti, F., Trifoglio, M., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Di Cocco, G., Chen, A., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Pellizzoni, A., Pilia, M., Barbiellini, G., Longo, F., Moretti, E., Vallazza, E., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Pittori, C., Lucarelli, F., Santolamazza, P., Colafrancesco, S., Giommi, P., and Salotti, L.
36. GRB 090910: SuperAGILE localization of a long GRB
- Author
-
Donnarumma, I., Evangelista, Y., Del Monte, E., Feroci, M., Lazzarotto, F., Pacciani, L., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Giuliani, A., Chen, A., Mereghetti, S., Perotti, F., Caraveo, P., Pellizzoni, A., Pilia, M., Vercellone, S., Andrea Bulgarelli, Gianotti, F., Trifoglio, M., Di Cocco, G., Labanti, C., Fuschino, F., Marisaldi, M., Galli, M., Tavani, M., Pucella, G., D Ammando, F., Striani, E., Vittorini, V., Argan, A., Trois, A., Piano, G., Sabatini, S., Barbiellini, G., Longo, F., Moretti, E., Picozza, P., Morselli, A., Prest, M., Vallazza, E., Lipari, P., Zanello, D., Giommi, P., Pittori, C., Santolamazza, P., Verrecchia, F., and Salotti, L.
37. AGILE detects enhanced gamma-ray emission from the blazar PKS 2142-758
- Author
-
Verrecchia, F., Striani, E., Pittori, C., Lucarelli, F., Vercellone, S., Tavani, M., Bulgarelli, A., D Ammando, F., Donnarumma, I., Vittorini, V., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Pacciani, L., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Argan, A., Piano, G., Pucella, G., Sabatini, S., Trois, A., Fuschino, F., Galli, M., Gianotti, F., Labanti, C., Marisaldi, M., Trifoglio, M., Di Cocco, G., Chen, A., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Alberto Paolo Pellizzoni, Pilia, M., Barbiellini, G., Longo, F., Moretti, E., Vallazza, E., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Santolamazza, P., Colafrancesco, S., Giommi, P., and Salotti, L.
38. A gamma-ray flare from 3C 454.3 detected by AGILE
- Author
-
Munar-Adrover, P., Piano, G., Pittori, C., Verrecchia, F., Lucarelli, F., Bulgarelli, A., Parmiggiani, N., Valentina Fioretti, Zoli, A., Vercellone, S., Tavani, M., Donnarumma, I., Striani, E., Minervini, G., Cardillo, M., Gianotti, F., Trifoglio, M., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Chen, A., Argan, A., Costa, E., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Lapshov, I., Pacciani, L., Soffitta, P., Sabatini, S., Vittorini, V., Pucella, G., Rapisarda, M., Di Cocco, G., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Pellizzoni, A., Pilia, M., Trois, A., Barbiellini, G., Vallazza, E., Longo, F., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Colafrancesco, S., Ferrari, A., Antonelli, A., Giommi, P., Salotti, L., Valentini, G., and D Amico, F.
39. AGILE/GRID detection of increased gamma-ray emission from 3C 454.3
- Author
-
Vercellone, S., Verrecchia, F., Donnarumma, I., Tavani, M., Striani, E., Lucarelli, F., Pittori, C., Bulgarelli, A., Gianotti, F., Trifoglio, M., D Ammando, F., Chen, A., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Pacciani, L., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Argan, A., Piano, G., Pucella, G., Sabatini, S., Trois, A., Vittorini, V., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Di Cocco, G., Alberto Paolo Pellizzoni, Pilia, M., Barbiellini, G., Longo, F., Vallazza, E., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Santolamazza, P., Colafrancesco, S., Giommi, P., and Salotti, L.
40. AGILE detection of AGL J2206+6203, a new unidentified gamma-ray source
- Author
-
Andrea Bulgarelli, Gianotti, F., Trifoglio, M., Lucarelli, F., Pittori, C., Verrecchia, F., Tavani, M., Striani, E., Chen, A., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Vercellone, S., Donnarumma, I., D Ammando, F., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Pacciani, L., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Argan, A., Piano, G., Pucella, G., Sabatini, S., Trois, A., Vittorini, V., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Di Cocco, G., Pellizzoni, A., Pilia, M., Barbiellini, G., Longo, F., Moretti, E., Vallazza, E., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Santolamazza, P., Colafrancesco, S., Giommi, P., and Salotti, L.
41. Gamma-ray flaring emission from Cygnus X-3 detected by AGILE
- Author
-
Bulgarelli, A., Pittori, C., Striani, E., Tavani, M., Gianotti, F., Trifoglio, M., Pooley, G., Mccollough, M., Trushkin, Sergei A., Piano, G., Verrecchia, F., Lucarelli, F., Cardillo, M., Argan, A., Trois, A., Paris, G., Vittorini, V., Costa, E., Donnarumma, I., Feroci, M., Pacciani, L., Del Monte, E., Lazzarotto, F., Soffitta, P., Evangelista, Y., Lapshov, I., Sabatini, S., Chen, A., Giuliani, A., Marisaldi, M., Di Cocco, G., Labanti, C., Fuschino, F., Galli, M., Caraveo, P., Mereghetti, S., Perotti, F., Pucella, G., Rapisarda, M., D Ammando, F., Vercellone, S., Alberto Paolo Pellizzoni, Pilia, M., Barbiellini, G., Longo, F., Picozza, P., Morselli, A., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Giommi, P., Santolamazza, P., Salotti, L., and Valentini, G.
42. AGILE detection of enhanced gamma-ray activity from the CTA 102 region
- Author
-
Bulgarelli, A., Tavani, M., Pittori, C., Verrecchia, F., Lucarelli, F., Donnarumma, Â I., Vercellone, S., Fioretti, V., Piano, G., Striani, E., Cardillo, M., Gianotti, F., Trifoglio, M., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Chen, A., Argan, A., Costa, E., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Lapshov, I., Pacciani, L., Soffitta, P., Sabatini, S., Vittorini, V., Pucella, G., Rapisarda, M., Di Cocco, G., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Pellizzoni, A., Pilia, M., Trois, A., Barbiellini, G., Vallazza, E., Longo, F., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Colafrancesco, S., Parmiggiani, N., Ferrari, A., Lucio Angelo Antonelli, Giommi, P., Salotti, L., Valentini, G., and D Amico, F.
43. AGILE detects enhanced gamma-ray emission from the FSRQ PKS 1510-089
- Author
-
Verrecchia, F., Pittori, C., Cardillo, M., Striani, E., Donnarumma, I., Vercellone, S., Tavani, M., Andrea Bulgarelli, Gianotti, F., Trifoglio, M., Chen, A., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., D Ammando, F., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Pacciani, L., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Argan, A., Piano, G., Sabatini, S., Trois, A., Vittorini, V., Pucella, G., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Di Cocco, G., Pellizzoni, A., Pilia, M., Barbiellini, G., Longo, F., Moretti, E., Vallazza, E., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Lucarelli, F., Santolamazza, P., Giommi, P., Salotti, L., and Valentini, G.
44. AGILE detection of Cygnus X-3 above 400 MeV
- Author
-
Bulgarelli, A., Striani, E., Piano, G., Tavani, M., Gianotti, F., Trifoglio, M., Mccollough, M., Savolainen, P., Argan, A., Trois, A., Paris, G., Vittorini, V., Costa, E., Donnarumma, I., Feroci, M., Pacciani, L., Del Monte, E., Lazzarotto, F., Soffitta, P., Evangelista, Y., Lapshov, I., Sabatini, S., Cardillo, M., Chen, A., Giuliani, A., Mereghetti, S., Perotti, F., Marisaldi, M., Di Cocco, G., Labanti, C., Fuschino, F., Galli, M., Pucella, G., Rapisarda, M., D Ammando, F., Vercellone, S., Alberto Paolo Pellizzoni, Pilia, M., Barbiellini, G., Longo, F., Picozza, P., Morselli, A., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Pittori, C., Verrecchia, F., Lucarelli, F., Giommi, P., Santolamazza, P., Salotti, L., and Valentini, G.
45. Compositional modeling of complex systems: contact center scenarios in osmosys
- Author
-
Franceschinis, G., Gribaudo, M., Mauro Iacono, Marrone, S., Mazzocca, N., and Vittorini, V.
46. A new gamma-ray transient, AGL J1835-6040, detected by AGILE
- Author
-
Pittori, C., Verrecchia, F., Lucarelli, F., Bulgarelli, A., Fioretti, V., Zoli, A., Tavani, M., Vercellone, S., Piano, G., Striani, E., Donnarumma, I., Cardillo, M., Gianotti, F., Trifoglio, M., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Chen, A., Argan, A., Costa, E., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Lapshov, I., Pacciani, L., Soffitta, P., Sabatini, S., Vittorini, V., Pucella, G., Rapisarda, M., Di Cocco, G., Fuschino, F., Galli, M., Labanti, C., Marisaldi, M., Pellizzoni, A., Pilia, M., Trois, A., Barbiellini, G., Vallazza, E., Longo, F., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Sergio Colafrancesco, Parmiggiani, N., Ferrari, A., Antonelli, A., Giommi, P., Salotti, L., Valentini, G., and D Amico, F.
47. AGILE detects enhanced gamma-ray emission from the blazar PKS 0402-362
- Author
-
Striani, E., Verrecchia, F., Pittori, C., Lucarelli, F., Vercellone, S., Tavani, M., Bulgarelli, A., D Ammando, F., Donnarumma, I., Vittorini, V., Del Monte, E., Evangelista, Y., Feroci, M., Lazzarotto, F., Pacciani, L., Soffitta, P., Costa, E., Lapshov, I., Rapisarda, M., Argan, A., Piano, G., Pucella, G., Sabatini, S., Trois, A., Fuschino, F., Galli, M., Gianotti, F., Labanti, C., Marisaldi, M., Trifoglio, M., Di Cocco, G., Chen, A., Giuliani, A., Mereghetti, S., Caraveo, P., Perotti, F., Alberto Paolo Pellizzoni, Pilia, M., Barbiellini, G., Longo, F., Moretti, E., Vallazza, E., Morselli, A., Picozza, P., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Santolamazza, P., Colafrancesco, S., Giommi, P., and Salotti, L.
48. Searching for very-high-energy electromagnetic counterparts to gravitational-wave events with the Cherenkov Telescope Array
- Author
-
Patricelli, B., Carosi, A., Nava, L., Seglar-Arroyo, M., Schüssler, F., Stamerra, A., Adelfio, A., Ashkar, H., Bulgarelli, A., Di Girolamo, T., Di Piano, A., Gasparetto, T., Green, J., Longo, F., Agudo, I., Berti, A., Bissaldi, E., Cella, G., Circiello, A., Covino, S., Ghirlanda, G., Humensky, B., Inoue, S., Lefaucheur, J., Filipovic, M., Razzano, M., Ribeiro, D., Sergijenko, O., Stratta, G., Vergani, S., Abdalla, H., Abe, H., Abe, S., Abusleme, A., Acero, F., Acharyya, A., Acín Portella, V., Ackley, K., Adam, R., Adams, C., Adhikari, S. S., Aguado-Ruesga, I., Aguilera, R., Aguirre-Santaella, A., Aharonian, F., Alberdi, A., Alfaro, R., Alfaro, J., Alispach, C., Aloisio, R., Alves Batista, R., Amans, J. -P, Amati, L., Amato, E., Ambrogi, L., Ambrosi, G., Ambrosio, M., Ammendola, R., Anderson, J., Anduze, M., Angüner, E. O., Antonelli, L. A., Antonuccio, V., Antoranz, P., Anutarawiramkul, R., Aragunde Gutierrez, J., Aramo, C., Araudo, A., Araya, M., Arbet-Engels, A., Arcaro, C., Arendt, V., Armand, C., Armstrong, T., Arqueros, F., Arrabito, L., Arsioli, B., Artero, M., Asano, K., Ascasíbar, Y., Aschersleben, J., Ashley, M., Attinà, P., Aubert, P., Singh, C. B., Baack, D., Babic, A., Backes, M., Baena, V., Bajtlik, S., Baktash, A., Balazs, C., Balbo, M., Ballester, O., Ballet, J., Balmaverde, B., Bamba, A., Bandiera, R., Baquero Larriva, A., Barai, P., Barbier, C., Barbosa Martins, V., Barcelo, M., Barkov, M., Barnard, M., Baroncelli, L., Almeida, U. B., Barrio, J. A., Bastieri, D., Batista, P. I., Batkovic, I., Bauer, C., Bautista-González, R., Baxter, J., Becciani, U., Becerra González, J., Becherini, Y., Beck, G., Becker Tjus, J., Bednarek, W., Belfiore, A., Bellizzi, L., Belmont, R., Benbow, W., Berge, D., Bernardini, E., Bernardos, M. I., Bernlöhr, K., Berton, M., Bertucci, B., Beshley, V., Bhatt, N., Bhattacharyya, S., Bhattacharyya, W., Bi, B., Bicknell, G., Biederbeck, N., Bigongiari, C., Biland, A., Bird, R., Biteau, J., Bitossi, M., Blanch, O., Blank, M., Blazek, J., Bobin, J., Boccato, C., Bocchino, F., Boehm, C., Bohacova, M., Boisson, C., Boix, J., Bolle, J. -P, Bolmont, J., Bonanno, G., Bonavolontà, C., Bonneau Arbeletche, L., Bonnoli, G., Bordas, P., Borkowski, J., Bórquez, S., Bose, R., Bose, D., Bosnjak, Z., Bottacini, E., Böttcher, M., Botticella, M. T., Boutonnet, C., Bouyjou, F., Bozhilov, V., Bozzo, E., Brahimi, L., Braiding, C., Brau-Nogué, S., Breen, S., Bregeon, J., Breuhaus, M., Brill, A., Brisken, W., Brocato, E., Brown, A. M., Brügge, K., Brun, P., Brun, F., Brunetti, L., Brunetti, G., Bruno, P., Bruno, A., Bruzzese, A., Bucciantini, N., Buckley, J., Bühler, R., Bulik, T., Bünning, M., Bunse, M., Burton, M., Burtovoi, A., Buscemi, M., Buschjäger, S., Busetto, G., Buss, J., Byrum, K., Caccianiga, A., Cadoux, F., Calanducci, A., Calderón, C., Calvo Tovar, J., Cameron, R., Campaña, P., Canestrari, R., Cangemi, F., Cantlay, B., Capalbi, M., Capasso, M., Cappi, M., Caproni, A., Capuzzo-Dolcetta, R., Caraveo, P., Cárdenas, V., Cardiel, L., Cardillo, M., Carlile, C., Caroff, S., Carosi, R., Carquín, E., Carrère, M., Casandjian, J. -M, Casanova, S., Cascone, E., Cassol, F., Castro-Tirado, A. J., Catalani, F., Catalano, O., Cauz, D., Ceccanti, A., Celestino Silva, C., Celli, S., Cerny, K., Cerruti, M., Chabanne, E., Chadwick, P., Chai, Y., Chambery, P., Champion, C., Chandra, S., Chaty, S., Chen, A., Cheng, K., Chernyakova, M., Chiaro, G., Chiavassa, A., Chikawa, M., Chitnis, V. R., Chudoba, J., Chytka, L., Cikota, S., Clark, P., Çolak, M., Colombo, E., Colome, J., Colonges, S., Comastri, A., Compagnino, A., Conforti, V., Congiu, E., Coniglione, R., Conrad, J., Conte, F., Contreras, J. L., Coppi, P., Cornat, R., Coronado-Blazquez, J., Cortina, J., Costa, A., Costantini, H., Cotter, G., Courty, B., Crestan, S., Cristofari, P., Crocker, R., Croston, J., Cubuk, K., Cuevas, O., Cui, X., Cusumano, G., Cutini, S., D’aì, A., D’amico, G., D’ammando, F., D’avanzo, P., Da Vela, P., Dadina, M., Dai, S., Dalchenko, M., Dall’ Ora, M., Daniel, M. K., Dauguet, J., Davids, I., Davies, J., Dawson, B., Angelis, A., Araújo Carvalho, A. E., Bony Lavergne, M., Caprio, V., Cesare, G., Frondat, F., Gouveia Dal Pino, E. M., La Calle, I., Lotto, B., Luca, A., Martino, D., Menezes, R. M., Naurois, M., Oña Wilhelmi, E., Palma, F., Persio, F., Simone, N., Souza, V., Del Santo, M., Del Valle, M. V., Delagnes, E., Deleglise, G., Delfino Reznicek, M., Delgado, C., Delgado Giler, A. G., Delgado Mengual, J., Della Ceca, R., Della Valle, M., Della Volpe, D., Depaoli, D., Depouez, D., Devin, J., Di Giulio, C., Di Pierro, F., Di Venere, L., Díaz, C., Díaz-Bahamondes, C., Dib, C., Diebold, S., Digel, S., Dima, R., Djannati-Ataï, A., Djuvsland, J., Dmytriiev, A., Docher, K., Domínguez, A., Dominis Prester, D., Donath, A., Donini, A., Dorner, D., Doro, M., Dos Anjos, R. D. C., Dournaux, J. -L, Downes, T., Drake, G., Drass, H., Dravins, D., Duangchan, C., Duara, A., Dubus, G., Ducci, L., Duffy, C., Dumora, D., Dundas Morå, K., Durkalec, A., Dwarkadas, V. V., Ebr, J., Eckner, C., Eder, J., Ederoclite, A., Edy, E., Egberts, K., Einecke, S., Eisch, J., Eleftheriadis, C., Elsässer, D., Emery, G., Emmanoulopoulos, D., Ernenwein, J. -P, Errando, M., Escarate, P., Escudero, J., Espinoza, C., Ettori, S., Eungwanichayapant, A., Evans, P., Evoli, C., Fairbairn, M., Falceta-Goncalves, D., Falcone, A., Fallah Ramazani, V., Falomo, R., Farakos, K., Fasola, G., Fattorini, A., Favre, Y., Fedora, R., Fedorova, E., Fegan, S., Feijen, K., Feng, Q., Ferrand, G., Ferrara, G., Ferreira, O., Fesquet, M., Fiandrini, E., Fiasson, A., Fink, D., Finley, J. P., Fioretti, V., Fiorillo, D. F. G., Fiorini, M., Flis, S., Flores, H., Foffano, L., Föhr, C., Fonseca, M. V., Font, L., Fontaine, G., Fornieri, O., Fortin, P., Fortson, L., Fouque, N., Fournier, A., Fraga, B., Franceschini, A., Franco, F. J., Franco Ordovas, A., Freixas Coromina, L., Fresnillo, L., Fruck, C., Fugazza, D., Fujikawa, Y., Fujita, Y., Fukami, S., Fukazawa, Y., Fukui, Y., Fulla, D., Funk, S., Furniss, A., Gabella, O., Gabici, S., Gaggero, D., Galanti, G., Galaz, G., Galdemard, P., Gallant, Y., Galloway, D., Gallozzi, S., Gammaldi, V., Garcia, R., Garcia, E., García, E., Garcia López, R., Garczarczyk, M., Gargano, F., Gargano, C., Garozzo, S., Gascon, D., Gasparrini, D., Gasparyan, H., Gaug, M., Geffroy, N., Gent, A., Germani, S., Gesa, L., Ghalumyan, A., Ghedina, A., Gianotti, F., Giarrusso, S., Giarrusso, M., Giavitto, G., Giebels, B., Giglietto, N., Gika, V., Gillardo, F., Gimenes, R., Giordano, F., Giovannini, G., Giro, E., Giroletti, M., Giuliani, A., Giunti, L., Gjaja, M., Glicenstein, J. -F, Gliwny, P., Godinovic, N., Göksu, H., Goldoni, P., Gómez, J. L., Gómez-Vargas, G., González, M. M., González, J. M., Gothe, K. S., Götz, D., Goulart Coelho, J., Gourgouliatos, K., Grabarczyk, T., Graciani, R., Grandi, P., Grasseau, G., Grasso, D., Green, A. J., Green, D., Greenshaw, T., Grenier, I., Grespan, P., Grillo, A., Grondin, M. -H, Grube, J., Guarino, V., Guest, B., Gueta, O., Gündüz, M., Gunji, S., Gusdorf, A., Gyuk, G., Hackfeld, J., Hadasch, D., Haga, J., Hagge, L., Hahn, A., Hajlaoui, J. E., Hakobyan, H., Halim, A., Hamal, P., Hanlon, W., Hara, S., Harada, Y., Hardcastle, M. J., Harvey, M., Hashiyama, K., Hassan Collado, T., Haubold, T., Haupt, A., Hautmann, U. A., Havelka, M., Hayashi, K., Hayashida, M., He, H., Heckmann, L., Heller, M., Helo, J. C., Henault, F., Henri, G., Hermann, G., Hermel, R., Hernández Cadena, S., Herrera Llorente, J., Herrero, A., Hervet, O., Hinton, J., Hiramatsu, A., Hiroshima, N., Hirotani, K., Hnatyk, B., Hnatyk, R., Hoang, J. K., Hoffmann, D., Hofmann, W., Hoischen, C., Holder, J., Holler, M., Hona, B., Horan, D., Hörandel, J., Horns, D., Horvath, P., Houles, J., Hovatta, T., Hrabovsky, M., Hrupec, D., Huang, Y., Huet, J. -M, Hughes, G., Hui, D., Hull, G., Humensky, T. B., Hütten, M., Iaria, R., Iarlori, M., Illa, J. M., Imazawa, R., Impiombato, D., Inada, T., Incardona, F., Ingallinera, A., Inome, Y., Inoue, T., Inoue, Y., Insolia, A., Iocco, F., Ioka, K., Ionica, M., Iori, M., Iovenitti, S., Iriarte, A., Ishio, K., Ishizaki, W., Iwamura, Y., Jablonski, C., Jacquemier, J., Jacquemont, M., Jamrozy, M., Janecek, P., Jankowsky, F., Jardin-Blicq, A., Jarnot, C., Jean, P., Jiménez Martínez, I., Jin, W., Jocou, L., Jordana, N., Josselin, M., Jouvin, L., Jung-Richardt, I., Junqueira, F. J. P. A., Juramy-Gilles, C., Jurysek, J., Kaaret, P., Kadowaki, L. H. S., Kagaya, M., Kalekin, O., Kankanyan, R., Kantzas, D., Karas, V., Karastergiou, A., Karkar, S., Kasai, E., Kasperek, J., Katagiri, H., Kataoka, J., Katarzyński, K., Katsuda, S., Katz, U., Kawanaka, N., Kazanas, D., Kerszberg, D., Khélifi, B., Kherlakian, M. C., Kian, T. P., Kieda, D. B., Kihm, T., Kim, S., Kimeswenger, S., Kisaka, S., Kissmann, R., Kleijwegt, R., Kleiner, T., Kluge, G., Kluźniak, W., Knapp, J., Knödlseder, J., Kobakhidze, A., Kobayashi, Y., Koch, B., Kocot, J., Kohri, K., Kokkotas, K., Komin, N., Kong, A., Kosack, K., Kowal, G., Krack, F., Krause, M., Krennrich, F., Krumholz, M., Kubo, H., Kudryavtsev, V., Kunwar, S., Kuroda, Y., Kushida, J., Kushwaha, P., La Barbera, A., La Palombara, N., La Parola, V., La Rosa, G., Lahmann, R., Lamanna, G., Lamastra, A., Landoni, M., Landriu, D., Lang, R. G., Lapington, J., Laporte, P., Lason, P., Lasuik, J., Lazendic-Galloway, J., Le Flour, T., Le Sidaner, P., Leach, S., Leckngam, A., Lee, S. -H, Lee, W. H., Lee, S., Oliveira, M. A. L., Lemière, A., Lemoine-Goumard, M., Lenain, J. -P, Leone, F., Leray, V., Leto, G., Leuschner, F., Levy, C., Lindemann, R., Lindfors, E., Linhoff, L., Liodakis, I., Lipniacka, A., Lloyd, S., Lobo, M., Lohse, T., Lombardi, S., Lopez, A., López, M., López-Coto, R., Loporchio, S., Louis, F., Louys, M., Lucarelli, F., Lucchesi, D., Ludwig Boudi, H., Luque-Escamilla, P. L., Lyard, E., Maccarone, M. C., Maccarone, T., Mach, E., Maciejewski, A. J., Mackey, J., Madejski, G. M., Maeght, P., Maggio, C., Maier, G., Majczyna, A., Majumdar, P., Makariev, M., Mallamaci, M., Almeida, R. M. N., Maltezos, S., Malyshev, D., Mandat, D., Maneva, G., Manganaro, M., Manicò, G., Manigot, P., Mannheim, K., Maragos, N., Marano, D., Marconi, M., Marcowith, A., Marculewicz, M., Marčun, B., Marín, J., Marinello, N., Marinos, P., Mariotti, M., Markoff, S., Marquez, P., Marsella, G., Martí, J., Martin, J. -M, Martin, P., Martinez, O., Martínez, M., Martínez, G., Martínez, O., Martínez-Huerta, H., Marty, C., Marx, R., Masetti, N., Massimino, P., Mastichiadis, A., Matsumoto, H., Matthews, N., Maurin, G., Max-Moerbeck, W., Maxted, N., Mazin, D., Mazziotta, M. N., Mazzola, S. M., Mbarubucyeye, J. D., Mc Comb, L., Mchardy, I., Mckeague, S., Mcmuldroch, S., Medina, E., Medina Miranda, D., Melandri, A., Melioli, C., Melkumyan, D., Menchiari, S., Mender, S., Mereghetti, S., Merino Arévalo, G., Mestre, E., Meunier, J. -L, Meures, T., Meyer, M., Micanovic, S., Miceli, M., Michailidis, M., Michałowski, J., Miener, T., Mievre, I., Miller, J., Minaya, I. A., Mineo, T., Minev, M., Miranda, J. M., Mirzoyan, R., Mitchell, A., Mizuno, T., Mode, B., Moderski, R., Mohrmann, L., Molina, E., Molinari, E., Montaruli, T., Monteiro, I., Moore, C., Moralejo, A., Morcuende-Parrilla, D., Moretti, E., Morganti, L., Mori, K., Moriarty, P., Morik, K., Morlino, G., Morris, P., Morselli, A., Mosshammer, K., Moya, P., Mukherjee, R., Muller, J., Mundell, C., Mundet, J., Murach, T., Muraczewski, A., Muraishi, H., Murase, K., Musella, I., Musumarra, A., Nagai, A., Nagar, N., Nagataki, S., Naito, T., Nakamori, T., Nakashima, K., Nakayama, K., Nakhjiri, N., Naletto, G., Naumann, D., Navarro, R., Nawaz, M. A., Ndiyavala, H., Neise, D., Nellen, L., Nemmen, R., Newbold, M., Neyroud, N., Ngernphat, K., Nguyen Trung, T., Nicastro, L., Nickel, L., Niemiec, J., Nieto, D., Nievas, M., Nigro, C., Nikołajuk, M., Ninci, D., Nishijima, K., Noda, K., Nogami, Y., Nolan, S., Nomura, R., Norris, R., Nosek, D., Nöthe, M., Novosyadlyj, B., Novotny, V., Nozaki, S., Nunio, F., O’brien, P., Obara, K., Oger, R., Ohira, Y., Ohishi, M., Ohm, S., Ohtani, Y., Oka, T., Okazaki, N., Okumura, A., Olive, J. -F, Oliver, C., Olivera, G., Olmi, B., Ong, R. A., Orienti, M., Orito, R., Orlandini, M., Orlando, S., Orlando, E., Osborne, J. P., Ostrowski, M., Otte, N., Evgeni Ovcharov, Owen, E., Oya, I., Ozieblo, A., Padovani, M., Pagano, I., Pagliaro, A., Paizis, A., Palatiello, M., Palatka, M., Palazzi, E., Panazol, J. -L, Paneque, D., Panes, B., Panny, S., Pantaleo, F. R., Panter, M., Paoletti, R., Paolillo, M., Papitto, A., Paravac, A., Paredes, J. M., Pareschi, G., Park, N., Parmiggiani, N., Parsons, R. D., Paśko, P., Patel, S., Pauletta, G., Pavletić, L., Pavy, S., Pe’er, A., Pech, M., Pecimotika, M., Pellegriti, M. G., Del Campo, P. P., Penno, M., Pepato, A., Perard, S., Perennes, C., Peres, G., Peresano, M., Pérez-Aguilera, A., Pérez-Romero, J., Pérez-Torres, M. A., Perri, M., Persic, M., Petrera, S., Petrucci, P. -O, Petruk, O., Peyaud, B., Pfrang, K., Pian, E., Piano, G., Piatteli, P., Pietropaolo, E., Pillera, R., Pilszyk, B., Pimentel, D., Pintore, F., Pio García, C., Pirola, G., Piron, F., Pisarski, A., Pita, S., Pohl, M., Poireau, V., Poledrelli, P., Pollo, A., Polo, M., Pongkitivanichkul, C., Porthault, J., Powell, J., Pozo, D., Prado, R. R., Prandini, E., Prasit, P., Prast, J., Pressard, K., Principe, G., Priyadarshi, C., Produit, N., Prokhorov, D., Prokoph, H., Prouza, M., Przybilski, H., Pueschel, E., Pühlhofer, G., Puljak, I., Pumo, M. L., Punch, M., Queiroz, F., Quinn, J., Quirrenbach, A., Rainò, S., Rajda, P. 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I., Ziętara, K., Zink, A., Ziółkowski, J., Zitelli, V., Živec, M., and Zmija, A.
49. AGILE monitoring of the enhanced gamma-ray emission from the Crab Nebula region
- Author
-
Tavani, M., Andrea Bulgarelli, Striani, E., Piano, G., Vittorini, V., Gianotti, F., Trifoglio, M., Pittori, C., Verrecchia, F., Argan, A., Trois, A., Paris, G., Sabatini, S., Costa, E., Donnarumma, I., Feroci, M., Pacciani, L., Del Monte, E., Lazzarotto, F., Soffitta, P., Evangelista, Y., Lapshov, I., Caraveo, P., Chen, A., Giuliani, A., Mereghetti, S., Perotti, F., Marisaldi, M., Di Cocco, G., Labanti, C., Fuschino, F., Galli, M., Pucella, G., Rapisarda, M., Vercellone, S., D Ammando, F., Pellizzoni, A., Pilia, M., Barbiellini, G., Longo, F., Picozza, P., Morselli, A., Prest, M., Lipari, P., Zanello, D., Cattaneo, P. W., Rappoldi, A., Giommi, P., Santolamazza, P., Lucarelli, F., Valentini, G., and Salotti, L.
50. AGILE detection of gamma-ray transients
- Author
-
Tavani, Marco, Chen, Andrew, Argan, A., Barbiellini, G., Bulgarelli, A., Caraveo, P., Cattaneo, P. W., D Ammando, F., Costa, E., Paris, G., Pasquale, F., Del Monte, E., Di Cocco, G., Don-Narumma, I., Evangelista, Y., Feroci, M., Ferrari, A., Fiorini, M., Fuschino, F., Galli, M., Gianotti, F., Giuliani, A., Giusti, M., Labanti, C., Lazzarotto, F., Lipari, P., Longo, F., Lucarelli, F., Marisaldi, M., Mereghetti, S., Morelli, E., Moretti, E., Morselli, A., Pacciani, L., Pellizzoni, A., Perotti, F., Piano, G., Picozza, P., Pilia, M., Pucella, G., Prest, M., Rapisarda, M., Rappoldi, A., Rubini, A., Sabatini, S., Scalise, E., Soffitta, P., Striani, E., Trifoglio, M., alessio trois, Vallazza, E., Vercellone, S., Vittorini, V., Zambra, A., Zanello, D., Pittori, C., Verrecchia, F., Santolamazza, P., Giommi, P., Colafrancesco, S., Antonelli, L. A., and Salotti, L.
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