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Search for gravitational waves from binary black hole inspirals in LIGO data

Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Agresti, J., Ajith, P., Allen, B., Allen, J., Amin, R., Anderson, S., Anderson, W., Araya, M., Armandula, H., Ashley, M., Asiri, F., Aufmuth, P., Aulbert, C., Babak, Stanislav, Balasubramanian, Ramachandran, Ballmer, S., Barish, B., Barker, C., Barker, D., Barnes, M., Barr, B., Barton, M., Bayer, K., Beausoleil, R., Belczynski, K., Bennett, R., Berukoff, S., Betzwieser, J., Bhawal, B., Bilenko, I., Billingsley, G., Black, E., Blackburn, K., Blackburn, L., Bland, B., Bochner, B., Bogue, L., Bork, R., Bose, S., Brady, P., Braginsky, V., Brau, J., Brown, D., Bullington, A., Bunkowski, A., Buonanno, A., Burgess, R., Busby, D., Butler, W., Byer, R., Cadonati, L., Cagnoli, G., Camp, J., Cannizzo, J., Cannon, K., Cantley, C., Cao, J., Cardenas, L., Carter, K., Casey, M., Castiglione, J., Chandler, A., Chapsky, J., Charlton, P., Chatterji, S., Chelkowski, S., Chen, Y., Chickarmane, V., Chin, D., Christensen, N., Churches, David K., Cokelaer, 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Vyachanin, S., Wallace, L., Walther, H., Ward, H., Ward, R., Ware, B., Watts, K., Webber, D., Weidner, A., Weiland, U., Weinstein, A., Weiss, R., Welling, H., Wen, L., Wen, S., Wette, K., Whelan, J., Whitcomb, S., Whiting, B., Wiley, S., Wilkinson, C., Willems, P., Williams, P., Williams, R., Willke, B., Wilson, A., Winjum, B., Winkler, W., Wise, S., Wiseman, A., Woan, G., Woods, D., Wooley, R., Worden, J., Wu, W., Yakushin, I., Yamamoto, H., Yoshida, S., Zaleski, K., Zanolin, M., Zawischa, I., Zhang, L., Zhu, R., Zotov, N., Zucker, M. and Zweizig, J. 2006. Search for gravitational waves from binary black hole inspirals in LIGO data. Physical Review D 73 (6) , 062001. 10.1103/PhysRevD.73.062001

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Abstract

We report on a search for gravitational waves from binary black hole inspirals in the data from the second science run of the LIGO interferometers. The search focused on binary systems with component masses between 3 and 20M⊙. Optimally oriented binaries with distances up to 1 Mpc could be detected with efficiency of at least 90%. We found no events that could be identified as gravitational waves in the 385.6 hours of data that we searched.

Item Type: Article
Date Type: Publication
Status: Published
Schools: Cardiff University Brain Research Imaging Centre (CUBRIC)
Medicine
Physics and Astronomy
Psychology
Subjects: Q Science > QB Astronomy
Publisher: American Physical Society
ISSN: 1550-7998
Last Modified: 09 Jul 2020 14:42
URI: http://orca.cf.ac.uk/id/eprint/35924

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