Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts

We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We looked for millisecond-duration unmodeled gravitational-wave bursts in 473 hr of coincident data collected during early 2003. No candidate signals were found. We set an upper limit of 0.12 events per...

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Veröffentlicht in:Physical review. D, Particles and fields Particles and fields, 2005-12, Vol.72 (12), Article 122004
Hauptverfasser: Abbott, B., Abbott, R., Adhikari, R., Ageev, A., Agresti, J., Ajith, P., Allen, B., Allen, J., Amin, R., Anderson, S. B., Anderson, W. G., Araya, M., Armandula, H., Ashley, M., Asiri, F., Aufmuth, P., Aulbert, C., Babak, S., Balasubramanian, R., Ballmer, S., Barish, B. C., Barker, C., Barker, D., Barnes, M., Barr, B., Barton, M. A., Bayer, K., Beausoleil, R., Belczynski, K., Bennett, R., Berukoff, S. J., Betzwieser, J., Bhawal, B., Bilenko, I. A., Billingsley, G., Black, E., Blackburn, K., Blackburn, L., Bland, B., Bochner, B., Bogue, L., Bork, R., Bose, S., Brady, P. R., Braginsky, V. B., Brau, J. E., Brown, D. A., Bullington, A., Bunkowski, A., Buonanno, A., Burgess, R., Busby, D., Butler, W. E., Byer, R. L., Cadonati, L., Cagnoli, G., Camp, J. B., Cannizzo, J., Cannon, K., Cantley, C. A., Cao, J., Cardenas, L., Carter, K., Casey, M. M., Castiglione, J., Chandler, A., Chapsky, J., Charlton, P., Chatterji, S., Chelkowski, S., Chen, Y., Chickarmane, V., Chin, D., Christensen, N., Churches, D., Cokelaer, T., Colacino, C., Coldwell, R., Coles, M., Cook, D., Corbitt, T., Coyne, D., Creighton, J. D. E., Creighton, T. D., Crooks, D. R. M., Csatorday, P., Cusack, B. J., Cutler, C., Dalrymple, J., D’Ambrosio, E., Danzmann, K., Davies, G., Daw, E., DeBra, D., Delker, T., Dergachev, V., Desai, S., DeSalvo, R., Dhurandhar, S., Di Credico, A.
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container_issue 12
container_start_page
container_title Physical review. D, Particles and fields
container_volume 72
creator Abbott, B.
Abbott, R.
Adhikari, R.
Ageev, A.
Agresti, J.
Ajith, P.
Allen, B.
Allen, J.
Amin, R.
Anderson, S. B.
Anderson, W. G.
Araya, M.
Armandula, H.
Ashley, M.
Asiri, F.
Aufmuth, P.
Aulbert, C.
Babak, S.
Balasubramanian, R.
Ballmer, S.
Barish, B. C.
Barker, C.
Barker, D.
Barnes, M.
Barr, B.
Barton, M. A.
Bayer, K.
Beausoleil, R.
Belczynski, K.
Bennett, R.
Berukoff, S. J.
Betzwieser, J.
Bhawal, B.
Bilenko, I. A.
Billingsley, G.
Black, E.
Blackburn, K.
Blackburn, L.
Bland, B.
Bochner, B.
Bogue, L.
Bork, R.
Bose, S.
Brady, P. R.
Braginsky, V. B.
Brau, J. E.
Brown, D. A.
Bullington, A.
Bunkowski, A.
Buonanno, A.
Burgess, R.
Busby, D.
Butler, W. E.
Byer, R. L.
Cadonati, L.
Cagnoli, G.
Camp, J. B.
Cannizzo, J.
Cannon, K.
Cantley, C. A.
Cao, J.
Cardenas, L.
Carter, K.
Casey, M. M.
Castiglione, J.
Chandler, A.
Chapsky, J.
Charlton, P.
Chatterji, S.
Chelkowski, S.
Chen, Y.
Chickarmane, V.
Chin, D.
Christensen, N.
Churches, D.
Cokelaer, T.
Colacino, C.
Coldwell, R.
Coles, M.
Cook, D.
Corbitt, T.
Coyne, D.
Creighton, J. D. E.
Creighton, T. D.
Crooks, D. R. M.
Csatorday, P.
Cusack, B. J.
Cutler, C.
Dalrymple, J.
D’Ambrosio, E.
Danzmann, K.
Davies, G.
Daw, E.
DeBra, D.
Delker, T.
Dergachev, V.
Desai, S.
DeSalvo, R.
Dhurandhar, S.
Di Credico, A.
description We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We looked for millisecond-duration unmodeled gravitational-wave bursts in 473 hr of coincident data collected during early 2003. No candidate signals were found. We set an upper limit of 0.12 events per day on the rate of detectable gravitational-wave bursts, at 90% confidence level. From software simulations, we estimate that our detector network was sensitive to bursts with root-sum-square strain amplitude above approximately 1-3x10{sup -19} Hz{sup -1/2} in the frequency band 700-2000 Hz. We describe the details of this collaborative search, with particular emphasis on its advantages and disadvantages compared to searches by LIGO and TAMA separately using the same data. Benefits include a lower background and longer observation time, at some cost in sensitivity and bandwidth. We also demonstrate techniques for performing coincidence searches with a heterogeneous network of detectors with different noise spectra and orientations. These techniques include using coordinated software signal injections to estimate the network sensitivity, and tuning the analysis to maximize the sensitivity and the livetime, subject to constraints on the background.
doi_str_mv 10.1103/PhysRevD.72.122004
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A. ; Bayer, K. ; Beausoleil, R. ; Belczynski, K. ; Bennett, R. ; Berukoff, S. J. ; Betzwieser, J. ; Bhawal, B. ; Bilenko, I. A. ; Billingsley, G. ; Black, E. ; Blackburn, K. ; Blackburn, L. ; Bland, B. ; Bochner, B. ; Bogue, L. ; Bork, R. ; Bose, S. ; Brady, P. R. ; Braginsky, V. B. ; Brau, J. E. ; Brown, D. A. ; Bullington, A. ; Bunkowski, A. ; Buonanno, A. ; Burgess, R. ; Busby, D. ; Butler, W. E. ; Byer, R. L. ; Cadonati, L. ; Cagnoli, G. ; Camp, J. B. ; Cannizzo, J. ; Cannon, K. ; Cantley, C. A. ; Cao, J. ; Cardenas, L. ; Carter, K. ; Casey, M. M. ; Castiglione, J. ; Chandler, A. ; Chapsky, J. ; Charlton, P. ; Chatterji, S. ; Chelkowski, S. ; Chen, Y. ; Chickarmane, V. ; Chin, D. ; Christensen, N. ; Churches, D. ; Cokelaer, T. ; Colacino, C. ; Coldwell, R. ; Coles, M. ; Cook, D. ; Corbitt, T. ; Coyne, D. ; Creighton, J. D. E. ; Creighton, T. D. ; Crooks, D. R. M. ; Csatorday, P. ; Cusack, B. J. ; Cutler, C. ; Dalrymple, J. ; D’Ambrosio, E. ; Danzmann, K. ; Davies, G. ; Daw, E. ; DeBra, D. ; Delker, T. ; Dergachev, V. ; Desai, S. ; DeSalvo, R. ; Dhurandhar, S. ; Di Credico, A.</creatorcontrib><description>We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We looked for millisecond-duration unmodeled gravitational-wave bursts in 473 hr of coincident data collected during early 2003. No candidate signals were found. We set an upper limit of 0.12 events per day on the rate of detectable gravitational-wave bursts, at 90% confidence level. From software simulations, we estimate that our detector network was sensitive to bursts with root-sum-square strain amplitude above approximately 1-3x10{sup -19} Hz{sup -1/2} in the frequency band 700-2000 Hz. We describe the details of this collaborative search, with particular emphasis on its advantages and disadvantages compared to searches by LIGO and TAMA separately using the same data. Benefits include a lower background and longer observation time, at some cost in sensitivity and bandwidth. We also demonstrate techniques for performing coincidence searches with a heterogeneous network of detectors with different noise spectra and orientations. These techniques include using coordinated software signal injections to estimate the network sensitivity, and tuning the analysis to maximize the sensitivity and the livetime, subject to constraints on the background.</description><identifier>ISSN: 1550-7998</identifier><identifier>ISSN: 0556-2821</identifier><identifier>EISSN: 1550-2368</identifier><identifier>EISSN: 1089-4918</identifier><identifier>DOI: 10.1103/PhysRevD.72.122004</identifier><language>eng</language><publisher>United States</publisher><subject>AMPLITUDES ; COMPUTER CODES ; COMPUTERIZED SIMULATION ; COSMOLOGY ; GRAVITATIONAL WAVE DETECTORS ; GRAVITATIONAL WAVES ; INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY ; INTERFEROMETRY ; ORIENTATION ; PHYSICS OF ELEMENTARY PARTICLES AND FIELDS ; SENSITIVITY ; VISIBLE RADIATION</subject><ispartof>Physical review. 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M.</creatorcontrib><creatorcontrib>Csatorday, P.</creatorcontrib><creatorcontrib>Cusack, B. J.</creatorcontrib><creatorcontrib>Cutler, C.</creatorcontrib><creatorcontrib>Dalrymple, J.</creatorcontrib><creatorcontrib>D’Ambrosio, E.</creatorcontrib><creatorcontrib>Danzmann, K.</creatorcontrib><creatorcontrib>Davies, G.</creatorcontrib><creatorcontrib>Daw, E.</creatorcontrib><creatorcontrib>DeBra, D.</creatorcontrib><creatorcontrib>Delker, T.</creatorcontrib><creatorcontrib>Dergachev, V.</creatorcontrib><creatorcontrib>Desai, S.</creatorcontrib><creatorcontrib>DeSalvo, R.</creatorcontrib><creatorcontrib>Dhurandhar, S.</creatorcontrib><creatorcontrib>Di Credico, A.</creatorcontrib><title>Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts</title><title>Physical review. D, Particles and fields</title><description>We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We looked for millisecond-duration unmodeled gravitational-wave bursts in 473 hr of coincident data collected during early 2003. No candidate signals were found. We set an upper limit of 0.12 events per day on the rate of detectable gravitational-wave bursts, at 90% confidence level. From software simulations, we estimate that our detector network was sensitive to bursts with root-sum-square strain amplitude above approximately 1-3x10{sup -19} Hz{sup -1/2} in the frequency band 700-2000 Hz. We describe the details of this collaborative search, with particular emphasis on its advantages and disadvantages compared to searches by LIGO and TAMA separately using the same data. Benefits include a lower background and longer observation time, at some cost in sensitivity and bandwidth. We also demonstrate techniques for performing coincidence searches with a heterogeneous network of detectors with different noise spectra and orientations. 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J.</creator><creator>Cutler, C.</creator><creator>Dalrymple, J.</creator><creator>D’Ambrosio, E.</creator><creator>Danzmann, K.</creator><creator>Davies, G.</creator><creator>Daw, E.</creator><creator>DeBra, D.</creator><creator>Delker, T.</creator><creator>Dergachev, V.</creator><creator>Desai, S.</creator><creator>DeSalvo, R.</creator><creator>Dhurandhar, S.</creator><creator>Di Credico, A.</creator><scope>AAYXX</scope><scope>CITATION</scope><scope>OTOTI</scope></search><sort><creationdate>20051201</creationdate><title>Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts</title><author>Abbott, B. ; Abbott, R. ; Adhikari, R. ; Ageev, A. ; Agresti, J. ; Ajith, P. ; Allen, B. ; Allen, J. ; Amin, R. ; Anderson, S. B. ; Anderson, W. G. ; Araya, M. ; Armandula, H. ; Ashley, M. ; Asiri, F. ; Aufmuth, P. ; Aulbert, C. ; Babak, S. ; Balasubramanian, R. ; Ballmer, S. ; Barish, B. C. ; Barker, C. ; Barker, D. ; Barnes, M. ; Barr, B. ; Barton, M. A. ; Bayer, K. ; Beausoleil, R. ; Belczynski, K. ; Bennett, R. ; Berukoff, S. J. ; Betzwieser, J. ; Bhawal, B. ; Bilenko, I. A. ; Billingsley, G. ; Black, E. ; Blackburn, K. ; Blackburn, L. ; Bland, B. ; Bochner, B. ; Bogue, L. ; Bork, R. ; Bose, S. ; Brady, P. R. ; Braginsky, V. B. ; Brau, J. E. ; Brown, D. A. ; Bullington, A. ; Bunkowski, A. ; Buonanno, A. ; Burgess, R. ; Busby, D. ; Butler, W. E. ; Byer, R. L. ; Cadonati, L. ; Cagnoli, G. ; Camp, J. B. ; Cannizzo, J. ; Cannon, K. ; Cantley, C. A. ; Cao, J. ; Cardenas, L. ; Carter, K. ; Casey, M. M. ; Castiglione, J. ; Chandler, A. ; Chapsky, J. ; Charlton, P. ; Chatterji, S. ; Chelkowski, S. ; Chen, Y. ; Chickarmane, V. ; Chin, D. ; Christensen, N. ; Churches, D. ; Cokelaer, T. ; Colacino, C. ; Coldwell, R. ; Coles, M. ; Cook, D. ; Corbitt, T. ; Coyne, D. ; Creighton, J. D. E. ; Creighton, T. D. ; Crooks, D. R. M. ; Csatorday, P. ; Cusack, B. J. ; Cutler, C. ; Dalrymple, J. ; D’Ambrosio, E. ; Danzmann, K. ; Davies, G. ; Daw, E. ; DeBra, D. ; Delker, T. ; Dergachev, V. ; Desai, S. ; DeSalvo, R. ; Dhurandhar, S. ; Di Credico, A.</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-LOGICAL-c429t-381f85968e3afb2936f6c8a1d43d59a791b85ab52e14281eb4ada579e1f0d46a3</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2005</creationdate><topic>AMPLITUDES</topic><topic>COMPUTER CODES</topic><topic>COMPUTERIZED SIMULATION</topic><topic>COSMOLOGY</topic><topic>GRAVITATIONAL WAVE DETECTORS</topic><topic>GRAVITATIONAL WAVES</topic><topic>INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY</topic><topic>INTERFEROMETRY</topic><topic>ORIENTATION</topic><topic>PHYSICS OF ELEMENTARY PARTICLES AND FIELDS</topic><topic>SENSITIVITY</topic><topic>VISIBLE RADIATION</topic><toplevel>peer_reviewed</toplevel><toplevel>online_resources</toplevel><creatorcontrib>Abbott, B.</creatorcontrib><creatorcontrib>Abbott, R.</creatorcontrib><creatorcontrib>Adhikari, R.</creatorcontrib><creatorcontrib>Ageev, A.</creatorcontrib><creatorcontrib>Agresti, J.</creatorcontrib><creatorcontrib>Ajith, P.</creatorcontrib><creatorcontrib>Allen, B.</creatorcontrib><creatorcontrib>Allen, J.</creatorcontrib><creatorcontrib>Amin, R.</creatorcontrib><creatorcontrib>Anderson, S. B.</creatorcontrib><creatorcontrib>Anderson, W. G.</creatorcontrib><creatorcontrib>Araya, M.</creatorcontrib><creatorcontrib>Armandula, H.</creatorcontrib><creatorcontrib>Ashley, M.</creatorcontrib><creatorcontrib>Asiri, F.</creatorcontrib><creatorcontrib>Aufmuth, P.</creatorcontrib><creatorcontrib>Aulbert, C.</creatorcontrib><creatorcontrib>Babak, S.</creatorcontrib><creatorcontrib>Balasubramanian, R.</creatorcontrib><creatorcontrib>Ballmer, S.</creatorcontrib><creatorcontrib>Barish, B. C.</creatorcontrib><creatorcontrib>Barker, C.</creatorcontrib><creatorcontrib>Barker, D.</creatorcontrib><creatorcontrib>Barnes, M.</creatorcontrib><creatorcontrib>Barr, B.</creatorcontrib><creatorcontrib>Barton, M. A.</creatorcontrib><creatorcontrib>Bayer, K.</creatorcontrib><creatorcontrib>Beausoleil, R.</creatorcontrib><creatorcontrib>Belczynski, K.</creatorcontrib><creatorcontrib>Bennett, R.</creatorcontrib><creatorcontrib>Berukoff, S. 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E.</creatorcontrib><creatorcontrib>Byer, R. L.</creatorcontrib><creatorcontrib>Cadonati, L.</creatorcontrib><creatorcontrib>Cagnoli, G.</creatorcontrib><creatorcontrib>Camp, J. B.</creatorcontrib><creatorcontrib>Cannizzo, J.</creatorcontrib><creatorcontrib>Cannon, K.</creatorcontrib><creatorcontrib>Cantley, C. A.</creatorcontrib><creatorcontrib>Cao, J.</creatorcontrib><creatorcontrib>Cardenas, L.</creatorcontrib><creatorcontrib>Carter, K.</creatorcontrib><creatorcontrib>Casey, M. M.</creatorcontrib><creatorcontrib>Castiglione, J.</creatorcontrib><creatorcontrib>Chandler, A.</creatorcontrib><creatorcontrib>Chapsky, J.</creatorcontrib><creatorcontrib>Charlton, P.</creatorcontrib><creatorcontrib>Chatterji, S.</creatorcontrib><creatorcontrib>Chelkowski, S.</creatorcontrib><creatorcontrib>Chen, Y.</creatorcontrib><creatorcontrib>Chickarmane, V.</creatorcontrib><creatorcontrib>Chin, D.</creatorcontrib><creatorcontrib>Christensen, N.</creatorcontrib><creatorcontrib>Churches, D.</creatorcontrib><creatorcontrib>Cokelaer, T.</creatorcontrib><creatorcontrib>Colacino, C.</creatorcontrib><creatorcontrib>Coldwell, R.</creatorcontrib><creatorcontrib>Coles, M.</creatorcontrib><creatorcontrib>Cook, D.</creatorcontrib><creatorcontrib>Corbitt, T.</creatorcontrib><creatorcontrib>Coyne, D.</creatorcontrib><creatorcontrib>Creighton, J. D. E.</creatorcontrib><creatorcontrib>Creighton, T. D.</creatorcontrib><creatorcontrib>Crooks, D. R. M.</creatorcontrib><creatorcontrib>Csatorday, P.</creatorcontrib><creatorcontrib>Cusack, B. J.</creatorcontrib><creatorcontrib>Cutler, C.</creatorcontrib><creatorcontrib>Dalrymple, J.</creatorcontrib><creatorcontrib>D’Ambrosio, E.</creatorcontrib><creatorcontrib>Danzmann, K.</creatorcontrib><creatorcontrib>Davies, G.</creatorcontrib><creatorcontrib>Daw, E.</creatorcontrib><creatorcontrib>DeBra, D.</creatorcontrib><creatorcontrib>Delker, T.</creatorcontrib><creatorcontrib>Dergachev, V.</creatorcontrib><creatorcontrib>Desai, S.</creatorcontrib><creatorcontrib>DeSalvo, R.</creatorcontrib><creatorcontrib>Dhurandhar, S.</creatorcontrib><creatorcontrib>Di Credico, A.</creatorcontrib><collection>CrossRef</collection><collection>OSTI.GOV</collection><jtitle>Physical review. D, Particles and fields</jtitle></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Abbott, B.</au><au>Abbott, R.</au><au>Adhikari, R.</au><au>Ageev, A.</au><au>Agresti, J.</au><au>Ajith, P.</au><au>Allen, B.</au><au>Allen, J.</au><au>Amin, R.</au><au>Anderson, S. B.</au><au>Anderson, W. G.</au><au>Araya, M.</au><au>Armandula, H.</au><au>Ashley, M.</au><au>Asiri, F.</au><au>Aufmuth, P.</au><au>Aulbert, C.</au><au>Babak, S.</au><au>Balasubramanian, R.</au><au>Ballmer, S.</au><au>Barish, B. C.</au><au>Barker, C.</au><au>Barker, D.</au><au>Barnes, M.</au><au>Barr, B.</au><au>Barton, M. A.</au><au>Bayer, K.</au><au>Beausoleil, R.</au><au>Belczynski, K.</au><au>Bennett, R.</au><au>Berukoff, S. J.</au><au>Betzwieser, J.</au><au>Bhawal, B.</au><au>Bilenko, I. A.</au><au>Billingsley, G.</au><au>Black, E.</au><au>Blackburn, K.</au><au>Blackburn, L.</au><au>Bland, B.</au><au>Bochner, B.</au><au>Bogue, L.</au><au>Bork, R.</au><au>Bose, S.</au><au>Brady, P. R.</au><au>Braginsky, V. B.</au><au>Brau, J. E.</au><au>Brown, D. A.</au><au>Bullington, A.</au><au>Bunkowski, A.</au><au>Buonanno, A.</au><au>Burgess, R.</au><au>Busby, D.</au><au>Butler, W. E.</au><au>Byer, R. L.</au><au>Cadonati, L.</au><au>Cagnoli, G.</au><au>Camp, J. B.</au><au>Cannizzo, J.</au><au>Cannon, K.</au><au>Cantley, C. A.</au><au>Cao, J.</au><au>Cardenas, L.</au><au>Carter, K.</au><au>Casey, M. M.</au><au>Castiglione, J.</au><au>Chandler, A.</au><au>Chapsky, J.</au><au>Charlton, P.</au><au>Chatterji, S.</au><au>Chelkowski, S.</au><au>Chen, Y.</au><au>Chickarmane, V.</au><au>Chin, D.</au><au>Christensen, N.</au><au>Churches, D.</au><au>Cokelaer, T.</au><au>Colacino, C.</au><au>Coldwell, R.</au><au>Coles, M.</au><au>Cook, D.</au><au>Corbitt, T.</au><au>Coyne, D.</au><au>Creighton, J. D. E.</au><au>Creighton, T. D.</au><au>Crooks, D. R. M.</au><au>Csatorday, P.</au><au>Cusack, B. J.</au><au>Cutler, C.</au><au>Dalrymple, J.</au><au>D’Ambrosio, E.</au><au>Danzmann, K.</au><au>Davies, G.</au><au>Daw, E.</au><au>DeBra, D.</au><au>Delker, T.</au><au>Dergachev, V.</au><au>Desai, S.</au><au>DeSalvo, R.</au><au>Dhurandhar, S.</au><au>Di Credico, A.</au><format>journal</format><genre>article</genre><ristype>JOUR</ristype><atitle>Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts</atitle><jtitle>Physical review. D, Particles and fields</jtitle><date>2005-12-01</date><risdate>2005</risdate><volume>72</volume><issue>12</issue><artnum>122004</artnum><issn>1550-7998</issn><issn>0556-2821</issn><eissn>1550-2368</eissn><eissn>1089-4918</eissn><abstract>We report on the first joint search for gravitational waves by the TAMA and LIGO collaborations. We looked for millisecond-duration unmodeled gravitational-wave bursts in 473 hr of coincident data collected during early 2003. No candidate signals were found. We set an upper limit of 0.12 events per day on the rate of detectable gravitational-wave bursts, at 90% confidence level. From software simulations, we estimate that our detector network was sensitive to bursts with root-sum-square strain amplitude above approximately 1-3x10{sup -19} Hz{sup -1/2} in the frequency band 700-2000 Hz. We describe the details of this collaborative search, with particular emphasis on its advantages and disadvantages compared to searches by LIGO and TAMA separately using the same data. Benefits include a lower background and longer observation time, at some cost in sensitivity and bandwidth. We also demonstrate techniques for performing coincidence searches with a heterogeneous network of detectors with different noise spectra and orientations. These techniques include using coordinated software signal injections to estimate the network sensitivity, and tuning the analysis to maximize the sensitivity and the livetime, subject to constraints on the background.</abstract><cop>United States</cop><doi>10.1103/PhysRevD.72.122004</doi><oa>free_for_read</oa></addata></record>
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identifier ISSN: 1550-7998
ispartof Physical review. D, Particles and fields, 2005-12, Vol.72 (12), Article 122004
issn 1550-7998
0556-2821
1550-2368
1089-4918
language eng
recordid cdi_osti_scitechconnect_20774492
source American Physical Society Journals
subjects AMPLITUDES
COMPUTER CODES
COMPUTERIZED SIMULATION
COSMOLOGY
GRAVITATIONAL WAVE DETECTORS
GRAVITATIONAL WAVES
INSTRUMENTATION RELATED TO NUCLEAR SCIENCE AND TECHNOLOGY
INTERFEROMETRY
ORIENTATION
PHYSICS OF ELEMENTARY PARTICLES AND FIELDS
SENSITIVITY
VISIBLE RADIATION
title Upper limits from the LIGO and TAMA detectors on the rate of gravitational-wave bursts
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