Search for gravitational wave bursts in LIGO's third science run

Autor: Abbott, B., Abbott, R., Adhikari, R., Agresti, J., Allen, B., Amin, R., Anderson, S., Anderson, W., Araya, M., Armandula, H., Ashley, M., Ajith, P., Aulbert, C., Babak, S., Balasubramanian, R., Ballmer, S., Barish, B., Barker, D., Barker, C., Allen, J., Bantilan, H., Barton, M., Bayer, K., Belczynski, K., Betzwieser, J., Bhawal, B., Bilenko, I., Billingsley, G., Black, E., Blackburn, K., Blackburn, L., Bland, B., Bogue, L., Bork, R., Bose, S., Brady, P., Braginsky, V., Brau, J., Brown, D., Buonanno, A., Cannon, K., Busby, D., Butler, W., Cao, J., Cadonati, L., Cagnoli, G., Camp, J., Cannizzo, J., Cardenas, L., Carter, K., Casey, M., Charlton, P., Chatterji, S., Chen, Y., Chin, D., Christensen, N., Cokelaer, T., Colacino, C., Coldwell, R., Cook, D., Corbitt, T., Coyne, D., Creighton, J., Creighton, T., Dalrymple, J., D'Ambrosio, E., Danzmann, K., Davies, G., Desai, S., DeBra, D., Dergachev, V., DeSalvo, R., Dhurandhar, S., Diaz, M., Di Credico, A., Drever, R., Dupuis, R., Ehrens, P., Etzel, T., Evans, M., Evans, T., Fairhurst, S., Garofoli, J., Gholami, I., Finn, L., Franzen, K., Fyffe, M., Frey, R., Fritschel, P., Frolov, V., Ganezer, K., Giaime, J., Goggin, L., Goda, K., Gonzalez, G., Gray, C., Gretarsson, A., Grimmett, D., Grote, H., Grunewald, S., Guenther, M., Gustafson, R., Hamilton, W., Hanna, C., Hanson, J., Hardham, C., Harry, G., Heefner, J., Heng, I., Hewitson, M., Hindman, N., Hoang, P., Hough, J., Hua, W., Ito, M., Itoh, Y., Ivanov, A., Jones, D., Johnson, W., Johnson, B., Jones, G., Kalogera, V., Katsavounidis, E., Kawabe, K., Kawamura, S., Kells, W., Khan, A., Kim, C., King, P., Klimenko, S., Koranda, S., Kozak, D., Krishnan, B., Landry, M., Lantz, B., Lazzarini, A., Lei, M., Leonor, I., Libbrecht, K., Lindquist, P., Liu, S., Mitra, S., Lormand, M., Lubinski, M., Lück, H., Luna, M., Machenschalk, B., MacInnis, M., Mageswaran, M., Mailand, K., Mikhailov, E., Malec, M., Mandic, V., Messaritaki, E., Marka, S., Maros, E., Mason, J., Mercer, R., Melissinos, A., Matone, L., Mavalvala, N., McCarthy, R., McClelland, D., McHugh, M., McNabb, J., Mendell, G., Meshkov, S., Messenger, C., Mitrofanov, V., Mitselmakher, G., Mittleman, R., Miyakawa, O., Mohanty, S., Moreno, G., Mossavi, K., Myers, E., Müller, G., Mukherjee, S., Myers, J., Nash, T., Noel, J., Nocera, F., O'Shaughnessy, R., O'Reilly, B., Ottaway, D., Pan, Y., Overmier, H., Owen, B., Papa, M., Parameswariah, C., Parameswariah, V., Pedraza, M., Penn, S., Pitkin, M., Prix, R., Quetschke, V., Raab, F., Radkins, H., Rahkola, R., Rakhmanov, M., Rawlins, K., Ray-Majumder, S., Re, T., Regimbau, T., Reitze, D., Rivera, B., Riles, K., Rodriguez, A., Robertson, D., Robertson, N., Robinson, C., Roddy, S., Rollins, J., Romano, J., Romie, J., Sarin, P., Ruet, L., Rowan, S., Rüdiger, A., Russell, P., Ryan, K., Sandberg, V., Sanders, G., Sannibale, V., Sathyaprakash, B., Saulson, P., Savage, R., Sazonov, A., Schilling, R., Schofield, R., Seader, S., Schutz, B., Schwinberg, P., Scott, S., Searle, A., Sears, B., Sellers, D., Sengupta, A., Shawhan, P., Shoemaker, D., Sibley, A., Siemens, X., Sigg, D., Sintes, A., Smith, J., Smith, M., Spjeld, O., Strain, K., Strom, D., Stuver, A., Summerscales, T., Sung, M., Sutton, P., Tanner, D., Tarallo, M., Thorne, K., Taylor, R., Veitch, J., Tokmakov, K., Torres, C., Torrie, C., Ungarelli, C., Traylor, G., Tyler, W., Ugolini, D., Vallisneri, M., van Putten, M., Vass, S., Vecchio, A., Vorvick, C., Vyachanin, S., Wallace, L., Walther, H., Ward, H., Ward, R., Watts, K., Webber, D., Weiland, U., Weinstein, A., Weiss, R., Wiley, S., Wette, K., Wen, S., Whelan, J., Whitcomb, S., Whiting, B., Willems, P., Wilkinson, C., Willke, B., Wilson, A., Woods, D., Winkler, W., Wise, S., Wiseman, A., Woan, G., Wooley, R., Worden, J., Yakushin, I., Yamamoto, H., Yoshida, S., Zanolin, M., Zhang, L., Zotov, N., Zucker, M., Zweizig, J.
Přispěvatelé: The LIGO Scientific Collaboration
Rok vydání: 2005
Předmět:
Zdroj: Classical and Quantum Gravity
DOI: 10.48550/arxiv.gr-qc/0511146
Popis: We report on a search for gravitational wave bursts in data from the three LIGO interferometric detectors during their third science run. The search targets subsecond bursts in the frequency range 100-1100 Hz for which no waveform model is assumed, and has a sensitivity in terms of the root-sum-square (rss) strain amplitude of hrss ~ 10^{-20} / sqrt(Hz). No gravitational wave signals were detected in the 8 days of analyzed data.
Comment: 12 pages, 6 figures. Amaldi-6 conference proceedings to be published in Classical and Quantum Gravity
Databáze: OpenAIRE