Zobrazeno 1 - 10
of 233
pro vyhledávání: '"Brocco , L."'
Autor:
Beauville, F., Bizouard, M. -A., Blackburn, L., Bosi, L., Brocco, L., Brown, D., Buskulic, D., Cavalier, F., Chatterji, S., Christensen, N., Clapson, A. -C., Fairhurst, S., Grosjean, D., Guidi, G., Hello, P., Heng, S., Hewitson, M., Katsavounidis, E., Klimenko, S., Knight, M., Lazzarini, A., Leroy, N., Marion, F., Markowitz, J., Melachrinos, C., Mours, B., Ricci, F., Viceré, A., Yakushin, I., Zanolin, M.
Publikováno v:
Class.Quant.Grav.25:045001,2008
Presented in this paper is a detailed and direct comparison of the LIGO and Virgo binary neutron star detection pipelines. In order to test the search programs, numerous inspiral signals were added to 24 hours of simulated detector data. The efficien
Externí odkaz:
http://arxiv.org/abs/gr-qc/0701027
Autor:
Beauville, F., Bizouard, M. -A., Blackburn, L., Bosi, L., Brocco, L., Brown, D., Buskulic, D., Cavalier, F., Chatterji, S., Christensen, N., Clapson, A. -C., Fairhurst, S., Grosjean, D., Guidi, G., Hello, P., Heng, S., Hewitson, M., Katsavounidis, E., Klimenko, S., Knight, M., Lazzarini, A., Leroy, N., Marion, F., Markowitz, J., Melachrinos, C., Mours, B., Ricci, F., Viceré, A., Yakushin, I., Zanolin, M.
Publikováno v:
Class.Quant.Grav.25:045002,2008
The search procedure for burst gravitational waves has been studied using 24 hours of simulated data in a network of three interferometers (Hanford 4-km, Livingston 4-km and Virgo 3-km are the example interferometers). Several methods to detect burst
Externí odkaz:
http://arxiv.org/abs/gr-qc/0701026
Autor:
Beauville, F., Bizouard, M. -A., Blackburn, L., Bosi, L., Brady, P., Brocco, L., Brown, D., Buskulic, D., Cavalier, F., Chatterji, S., Christensen, N., Clapson, A. -C., Fairhurst, S., Grosjean, D., Guidi, G., Hello, P., Katsavounidis, E., Knight, M., Lazzarini, A., Leroy, N., Marion, F., Mours, B., Ricci, F., Vicere, A., Zanolin, M.
Publikováno v:
J.Phys.Conf.Ser. 32 (2006) 212
We examine the benefits of performing a joint LIGO--Virgo search for transient signals. We do this by adding burst and inspiral signals to 24 hours of simulated detector data. We find significant advantages to performing a joint coincidence analysis,
Externí odkaz:
http://arxiv.org/abs/gr-qc/0509041
Autor:
Blackburn, L., Beauville, F., Bizouard, M. -A., Bosi, L., Brady, P., Brocco, L., Brown, D., Buskulic, D., Chatterji, S., Christensen, N., Clapson, A. -C., Fairhurst, S., Grosjean, D., Guidi, G., Hello, P., Katsavounidis, E., Knight, M., Lazzarini, A., Marion, F., Mours, B., Ricci, F., Vicere, A., Zanolin, M.
Publikováno v:
Class.Quant.Grav. 22 (2005) S1293-S1302
We present a comparative study of 6 search methods for gravitational wave bursts using simulated LIGO and Virgo noise data. The data's spectra were chosen to follow the design sensitivity of the two 4km LIGO interferometers and the 3km Virgo interfer
Externí odkaz:
http://arxiv.org/abs/gr-qc/0504060
Autor:
Blackburn, L., Beauville, F., Bizouard, M. -A., Bosi, L., Brady, P., Brocco, L., Brown, D., Buskulic, D., Chatterji, S., Christensen, N., Clapson, A. -C., Fairhurst, S., Grosjean, D., Guidi, G., Hello, P., Katsavounidis, E., Knight, M., Lazzarini, A., Marion, F., Mours, B., Ricci, F., Vicere', A., Zanolin, M.
Publikováno v:
Class.Quant.Grav. 22 (2005) S1149-S1158
This article reports on a project that is the first step the LIGO Scientific Collaboration and the Virgo Collaboration have taken to prepare for the mutual search for inspiral signals. The project involved comparing the analysis pipelines of the two
Externí odkaz:
http://arxiv.org/abs/gr-qc/0504050
Preliminary results on the flux of non strongly-interacting, fractionally charged particles in primary cosmic rays at 400 Km above sea level are given. Cosmic ray data collected by AMS-01 in June 1998 have been analysed on the hypotheses of 2/3 charg
Externí odkaz:
http://arxiv.org/abs/astro-ph/0304192
Autor:
Brocco, L., Casadei, D., Cindolo, F., Contin, A., Laurenti, G., Levi, G., Montanari, A., Palmonari, F., Patuelli, L., Sbarra, C., Zichichi, A.
The Time-of-Flight (TOF) system of the AMS detector gives the fast trigger to the read out electronics and measures velocity, direction and charge of the crossing particles. The new version of the detector (called AMS-02) will be installed on the Int
Externí odkaz:
http://arxiv.org/abs/hep-ex/0111096
Autor:
Baldini, L., Brocco, L., Casadei, D., Cindolo, F., Contin, A., Laurenti, G., Levi, G., Margotti, A., Montanari, A., Palmonari, F., Patuelli, L., Sbarra, C., Zichichi, A.
The Time-of-Flight (TOF) system of the AMS detector gives the fast trigger to the read out electronics and measures velocity, direction and charge of the crossing particles. The first version of the detector (called AMS-01) has flown in 1998 aboard o
Externí odkaz:
http://arxiv.org/abs/astro-ph/0111480
Autor:
Baldini, L., Brocco, L., Casadei, D., Castellini, G., Cindolo, F., Contin, A., Laurenti, G., Levi, G., Palmonari, F., Zichichi, A.
The Time of Flight (TOF) system of the AMS experiment provides the fast trigger to the detector and measures the crossing particle direction, velocity and charge. AMS was operated aboard of the shuttle Discovery on June 1998 (NASA STS-91 mission) and
Externí odkaz:
http://arxiv.org/abs/hep-ex/0108042
Autor:
Acernese, F., Amico, P., Al-Shourbagy, M., Aoudia, S., Avino, S., Babusci, D., Ballardin, G., Barillé, R., Barone, F., Barsotti, L., Barsuglia, M., Beauville, F., Bizouard, M.A., Boccara, C., Bondu, F., Bosi, L., Bradaschia, C., Braccini, S., Brillet, A., Brisson, V., Brocco, L., Buskulic, D., Calloni, E., Campagna, E., Cavalier, F., Cavalieri, R., Cella, G., Chassande-Mottin, E., Clapson, A.C., Cleva, F., Corda, C., Coulon, J.-P., Cuoco, E., Dattilo, V., Davier, M., De Rosa, R., Di Fiore, L., Di Virgilio, A., Dujardin, B., Eleuteri, A., Enard, D., Ferrante, I., Fidecaro, F., Fiori, I., Flaminio, R., Fournier, J.-D., Frasca, S., Frasconi, F., Freise, A., Gammaitoni, L., Gennai, A., Giazotto, A., Giordano, G., Gouaty, R., Grosjean, D., Guidi, G., Hebri, S., Heitmann, H., Hello, P., Holloway, L., Kreckelberg, S., La Penna, P., Loriette, V., Loupias, M., Losurdo, G., Mackowski, J.-M., Majorana, E., Man, C.N., Mantovani, M., Marion, F., Marque, J., Martelli, F., Masserot, A., Massonnet, L., Mazzoni, M., Milano, L., Moins, C., Moreau, J., Moreau, F., Morgado, N., Mornet, F., Mours, B., Pacheco, J., Pai, A., Palomba, C., Paoletti, F., Pardi, S., Pasqualetti, A., Passaquieti, R., Passuello, D., Perniola, B., Piergiovanni, F., Pinard, L., Poggiani, R., Punturo, M., Puppo, P., Qipiani, K., Rapagnani, P., Reita, V., Remillieux, A., Ricci, F., Ricciardi, I., Ruggi, P., Russo, G., Solimeno, S., Spallicci, A., Stanga, R., Taddei, R., Tombolato, D., Toncelli, A., Tonelli, M., Tournefier, E., Travasso, F., Trinquet, H., Varvella, M., Verkindt, D., Vetrano, F., Viceré, A., Vinet, J.-Y., Vocca, H., Yvert, M., Zhou, Z.
Publikováno v:
In Optics and Lasers in Engineering 2007 45(4):478-487
