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2. THE INTERPLANETARY NETWORK

Author

Hurley, K., primary, Mitrofanov, I. G., additional, Golovin, D., additional, Litvak, M. L., additional, Sanin, A. B., additional, Boynton, W., additional, Fellows, C., additional, Harshman, K., additional, Starr, R., additional, Golenetskii, S., additional, Aptekar, R., additional, Mazets, E., additional, Palshin, V., additional, Frederiks, D., additional, Svinkin, D., additional, Smith, D. M., additional, Hajdas, W., additional, Kienlin, A. von, additional, Zhang, X., additional, Rau, A., additional, Yamaoka, K., additional, Takahashi, T., additional, Ohno, M., additional, Hanabata, Y., additional, Fukazawa, Y., additional, Tashiro, M., additional, Terada, Y., additional, Murakami, T., additional, Makishima, K., additional, Cline, T., additional, Barthelmy, S., additional, Cummings, J., additional, Gehrels, N., additional, Krimm, H., additional, Palmer, D., additional, Goldsten, J., additional, Del Monte, E., additional, Feroci, M., additional, Marisaldi, M., additional, Connaughton, V., additional, Briggs, M. S., additional, and Meegan, C., additional

Published
2020
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3. OBSERVING GRBS WITH THE LOFT WIDE FIELD MONITOR

Author

Brandt, S., primary, Hernanz, M., additional, Feroci, M., additional, Amati, L., additional, Azzarello, Alvarez P., additional, Barret, D., additional, Bozzo, E., additional, Budtz-Jørgensen, C., additional, Campana, R., additional, Castro-Tirado, A., additional, Cros, A., additional, Del Monte, E., additional, Donnarumma, I., additional, Evangelista, Y., additional, Galvez Sanchez, J. L., additional, Gotz, D., additional, Herder, J. W. den, additional, Hornstrup, A., additional, Hudec, R., additional, Karelin, D., additional, Klis, M. van der, additional, Korpela, S., additional, Kuvvetli, I., additional, Lund, N., additional, Orleanski, P., additional, Pohl, M., additional, Rachevski, A., additional, Santangelo, A., additional, Schanne, S., additional, Schmid, C., additional, Stella, L., additional, Suchy, S., additional, Tenzer, C., additional, Vacchi, A., additional, Wilms, J., additional, Zampa, N., additional, Zand, J. J. M. in’t, additional, and Zdziarski, A., additional

Published
2020
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5. 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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6. The IPN I: From the Past to the Future

Author

Cline, T. L., primary, Hurley, K. C., additional, Barthelmy, S., additional, Butterworth, P., additional, Feroci, M., additional, Frontera, F., additional, Golenetskii, S., additional, Mazets, E., additional, and Trombka, J., additional

Published
2003
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8. 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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9. 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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11. 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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14. Programs of X-ray polarimetry in Italy

Author

Costa, E., primary, Argan, A., additional, Cosimo, S. Di, additional, Fabiani, S., additional, Feroci, M., additional, Lazzarotto, F., additional, Muleri, F., additional, Rubini, A., additional, Soffitta, P., additional, Trois, A., additional, Bellazzini, R., additional, Brez, A., additional, Minuti, M., additional, Pinchera, M., additional, Spandre, G., additional, Tagliaferri, G., additional, Basso, S., additional, Citterio, O., additional, Cotroneo, V., additional, Pareschi, G., additional, and Matt, G., additional

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15. GRB000615 in X-Rays

Author

Nicastro, Luciano, primary, Cusumano, G., additional, Antonelli, A., additional, Amati, L., additional, Frontera, F., additional, Palazzi, E., additional, Pian, E., additional, Costa, E., additional, Feroci, M., additional, Piro, L., additional, Zand, J. in’t, additional, and Heise, J., additional

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16. GAMMA-RAY ASTROPHYSICS WITH AGILE.

Author

SIDHARTH, B.G., HONSELL, F., DE ANGELIS, A., LONGO, F., ARGAN, A., BARBIELLINI, G., BASSET, M., BOFFELLI, F., BULGARELLI, A., CARAVEO, P., CATTANEO, P. W., CELESTI, E., CHEN, A., COCCO, V., COSTA, E., MONTE, E. DEL, COCCO, G. DI, PERSIO, G. DI, DONNARUMMA, I., and FEROCI, M.

Abstract

A brief description of the new generation high-energy gamma-ray astrophysics experiment AGILE and its main science objectives are presented. [ABSTRACT FROM AUTHOR]

Published
2006
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17. One Year of Rapid, Precise Gamma-Ray Burst Localizations by the Interplanetary Network.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Hurley, Kevin, Cline, T. L., Barthelmy, S., Butterworth, P., Feroci, M., Frontera, F., Montanari, E., Guidorzi, C., Golenetskii, S., Mazets, E., and Trombka, J.

Abstract

We review the performance of the interplanetary network over the past year, emphasizing the GRB detection rate, and the speed and accuracy of the localizations. Two scientific highlights, the burst with the highest redshift to date, and the first rapid, precise localizations of short bursts, are outlined. [ABSTRACT FROM AUTHOR]

Published
2001
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18. The IPN I: From the Past to the Future.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Cline, T. L., Hurley, K. C., Barthelmy, S., Butterworth, P., Feroci, M., Frontera, F., Golenetskii, S., Mazets, E., and Trombka, J.

Abstract

Interplanetary spacecraft have been used with orbiting satellites for over 25 years to precisely localize gamma ray transients by the measurement of their timedelay geometry. The first interplanetary network (IPN) made both discoveries and controversies, and the latest is making possible a significant number of GRB counterpart observations. The IPN technique was pursued with dedicated payloads, with piggy-back experiments, and by the creative modifications of other experiments. The achievement of the NEAR in-flight software revision added a distant vertex to the array of Ulysses and the near-Earth group of GGS-Wind Konus, Beppo-Sax and Rossi-XTE. This 3-way long-baseline network culminated IPN history by, in the year 2000 alone, enabling over one-third of the afterglow searches and 5 redshift measurements. Future IPN possibilities are also outlined. [ABSTRACT FROM AUTHOR]

Published
2001
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19. 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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20. GRB000615 in X-Rays.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Nicastro, Luciano, Cusumano, G., Antonelli, A., Amati, L., Frontera, F., Palazzi, E., Pian, E., Costa, E., Feroci, M., Piro, L., Zand, J. in't, and Heise, J.

Abstract

GRB000615 was detected simultaneously by the BeppoSAX GRBM and WFC 1 with a localization uncertainty of $2^\prime$ (error circle radius). X-ray emission was detected only in the 0.1-4 keV range during a NFI observation started $\simeq 10$ hours after the trigger time. The positional and temporal analysis shows the presence of two sources, one of which may be related to the GRB. [ABSTRACT FROM AUTHOR]

Published
2001
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21. BeppoSAX Observation of GRB990806: From the Prompt Emission to the X-Ray Afterglow.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Montanari, E., Amati, L., Frontera, F., Guidorzi, C., Capalbi, M., Costa, E., Feroci, M., Piro, L., Heise, J., Zand, J. J. M. in't, Pian, E., Palazzi, E., Masetti, N., and Nicastro, L.

Abstract

We present preliminary results of the analysis of BeppoSAX data of GRB 990806. The high energy spectrum of the prompt event is fitted by a single powerlaw whose spectral index does not vary significantly. In the error box of the GRB, determined by the WFC, the BSAX NFI have detected a previously unknown X-ray source. Based on the power-law temporal decay of its flux in the 2-10 keV range, $f(t) \sim t^{-1.15}$, the source has been identified with the GRB afterglow. [ABSTRACT FROM AUTHOR]

Published
2001
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22. Discovery of a Redshifted Iron K-Line in the X-Ray Afterglow of GRB 000214.

Author

Costa, Enrico, Frontera, Filippo, Hjorth, Jens, Antonelli1, L. A., Vietri, M., Piro, L., Costa, E., Sofftta, P., Feroci, M., Amati, L., Frontera, F., Pian, E., Zand, J. in 't., Stella, L., and Perola, G. C.

Abstract

We report on the BeppoSAX observation of the X-ray afterglow of GRB 000214 ("Valentine's Day Burst"). A strong emission line is detected (3$\sigma$ significance level) in the X-ray spectrum with a centroid energy of $4.7 \pm 0.2$ keV. This feature, if interpreted as Ka emission from hydrogen-like iron, corresponds to a redshift of z = 0.47. The intensity (EW$\sim 2$ keV) and duration (tens of hours) of the line give information on the distance of the emitting material ( $R \ge 3 \times 10^{15}$ cm) and its mass ( $M \ge 1.4M_\odot$). These results are not easily reconciled with the binary merger and hypernova models for gamma ray bursts, and rather point to a SupraNova scenario. [ABSTRACT FROM AUTHOR]

Published
2001
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23. 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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