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2. GAMMA-RAY ASTROPHYSICS WITH AGILE

Author

LONGO, F., primary, ARGAN, A., additional, BARBIELLINI, G., additional, BASSET, M., additional, BOFFELLI, F., additional, BULGARELLI, A., additional, CARAVEO, P., additional, CATTANEO, P. W., additional, CELESTI, E., additional, CHEN, A., additional, COCCO, V., additional, COSTA, E., additional, MONTE, E. DEL, additional, COCCO, G. DI, additional, PERSIO, G. DI, additional, DONNARUMMA, I., additional, FEROCI, M., additional, FIORINI, M., additional, FROYSLAND, T., additional, FRUTTI, M., additional, GALLI, M., additional, GIANOTTI, F., additional, GIULIANI, A., additional, LABANTI, C., additional, LAPSHOV, I., additional, LAZZAROTTO, F., additional, LIELLO, F., additional, LIPARI, P., additional, MARISALDI, M., additional, MASTROPIETRO, M., additional, MAURI, A., additional, MAURI, F., additional, MEREGHETTI, S., additional, MORELLI, E., additional, MORSELLI, A., additional, PACCIANI, L., additional, PELLIZZONI, A., additional, PEROTTI, F., additional, PICOZZA, P., additional, PITTORI, F., additional, PONTONI, C., additional, PORROVECCHIO, G., additional, PREST, M., additional, RAPISARDA, M., additional, ROSSI, E., additional, RUBINI, A., additional, SOFFITTA, P., additional, TAVANI, M., additional, TRACI, A., additional, TRIFOGLIO, M., additional, VALLAZZA, E., additional, VERCELLONE, S., additional, and ZANELLO, D., additional

Published
2006
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3. The Agile Gamma-Ray Astronomy Satellite

Author

Mereghetti, S., primary, Tavani, M., additional, Argan, A., additional, Chen, A., additional, Caraveo, P., additional, Perotti, F., additional, Vercellone, S., additional, Barbiellini, G., additional, Prest, M., additional, Vallazza, E., additional, Di Cocco, G., additional, Labanti, C., additional, Trifoglio, M., additional, Costa, E., additional, Feroci, M., additional, Lapshov, I., additional, Rubini, A., additional, Soffitta, P., additional, Picozza, P., additional, Morselli, A., additional, Cocco, V., additional, Pittori, C., additional, Zanello, D., additional, Lipari, P., additional, and Longo, F., additional

Published
2001
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4. Bepposax Observations of GRS 1915+105

Author

Feroci, M., primary, Casella, P., additional, Costa, E., additional, Massaro, E., additional, Soffitta, P., additional, Matt, G., additional, Belloni, T., additional, Castro-Tirado, A. J., additional, Dhawan, V., additional, Frontera, F., additional, Harmon, A., additional, Mirabel, F., additional, Pooley, G., additional, and Tavani, M., additional

Published
2001
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5. Evn Observations of GRS 1915+105

Author

Giovannini, G., primary, Feretti, L., additional, Tordi, M., additional, Venturi, T., additional, Massaglia, S., additional, Bodo, G., additional, Trussoni, E., additional, Gliozzi, M., additional, Tavani, M., additional, Conway, J., additional, Foley, A., additional, Graham, D., additional, Kus, A., additional, Spencer, R., additional, and Trigilio, C., additional

Published
2001
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6. ASCA Observations of the Superluminal Jet Source GRS1915+105

Author

Ebisawa, Ken, primary, Takeshima, T., additional, White, N. E., additional, Kotani, T., additional, Dotani, T., additional, Ueda, Y., additional, Harmon, B. A., additional, Robinson, C. R., additional, Zhang, S. N., additional, Paciesas, W. S., additional, Tavani, M., additional, and Foster, R., additional

Published
1998
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13. AGILE and Gamma-Ray Bursts

Author

Tavani, M., primary, Barbiellini, G., additional, Argan, A., additional, Auricchio, N., additional, Caraveo, P., additional, Chen, A., additional, Cocco, V., additional, Costa, E., additional, Cocco, G. Di, additional, Fedel, G., additional, Feroci, M., additional, Fiorini, M., additional, Galli, M., additional, Giuliani, A., additional, Labanti, C., additional, Lapshov, I., additional, Lipari, P., additional, Longo, F., additional, Mereghetti, S., additional, Morelli, E., additional, Morselli, A., additional, Pellizzoni, A., additional, Perotti, F., additional, Picozza, P., additional, Pittori, C., additional, Pontoni, C., additional, Prest, M., additional, Rapisarda, M., additional, Rossi, E., additional, Rubini, A., additional, Soffitta, P., additional, Trifoglio, M., additional, Vallazza, E., additional, Vercellone, S., additional, and Zanello, D., additional

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15. Gamma-Ray Bursts with SuperAGILE.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Feroci, M., Costa, E., Monte, E. Del, Lapshov, I., Rapisarda, M., Soffitta, P., Barbiellini, G., Prest, M., Vallazza, E., Mereghetti, S., Tavani, M., Vercellone, S., Morselli, A., and Longo, F.

Abstract

We present the capabilities for Gamma Ray Bursts of SuperAGILE, the hard X-ray (10-40 keV) monitor of the gamma-ray mission AGILE. SuperAGILE has a wide field of view ($\sim 1.8$ sr), coded by one-dimensional coded masks in two orthogonal directions, read-out by single-sided silicon microstrip detectors. Based on our simulations, we expect to detect and localize $\sim 1-2$ GRBs/month to better than 6 arcmin. [ABSTRACT FROM AUTHOR]

Published
2001
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16. Testing the Optically Thin Synchrotron Shock Model for Gamma-Ray Bursts Spectra from 2 to 700 keV with BeppoSAX.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Amati, L., Frontera, F., Tavani, M., Zand, J. J. M. in 't., Costa, E., Guidorzi, C., Montanari, E., and Soffitta, P.

Abstract

We present preliminary results of the fits with the Optically Thin Synchrotron Shock Modelof GRB time-averaged spectra from 2 to 700 keV basing on BeppoSAX data. This model gives a satisfactory description of the majority of the data. Nevertheless, $\sim$ 30% need of accounting for substantial radiative cooling of the emitting electrons during the event. [ABSTRACT FROM AUTHOR]

Published
2001
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17. AGILE and Gamma-Ray Bursts.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Tavani, M., Barbiellini, G., Argan, A., Auricchio, N., Caraveo, P., Chen, A., Cocco, V., Costa, E., Cocco, G. Di, Fedel, G., Feroci, M., Fiorini, M., Galli, M., Giuliani, A., Labanti, C., Lapshov, I., and Lipari, P.

Abstract

The AGILE astrophysics mission planned to be operational in 2003 will significantly contribute to the study of Gamma-Ray Bursts. AGILE is equipped with state-of-the-art imaging Silicon detectors in the 10-40 keV and 30 MeV-50 GeV ranges. In addition, also a CsI Mini-Calorimeter can independently detect transient events. Among the instrument characteristics most useful to GRB science we mention: (1) the excellent positioning and sensitivity at large off-axis angles; (2) the very small instrumental deadtimes ($\sim 100 \mu$s above 30 MeV, and $\sim 5 \mu$s below 10 MeV); (3) the on-board capability to trigger sky map acquisition in the 10-40 keV range and to transmit burst coordinates within a few seconds from the event. A special GRB search procedure will be implemented on-board for a broad range of trigger timescales from 1 millisecond to 100 seconds. AGILE will be the only Mission dedicated to astrophysics above 30 MeV and operating during the years 2003-2006. [ABSTRACT FROM AUTHOR]

Published
2001
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