A joint search for gravitational wave bursts with AURIGA and LIGO
Creators
- Baggio, L.1
- Bignotto, M.2
- Bonaldi, M.3
- Cerdonio, M.2
- De Rosa, M.
- Falferi, P.3
- Fattori, S.2
- Fortini, P.4
- Giusfredi, G.5
- Inguscio, M.6
- Liguori, N.2
- Longo, S.7
- Marin, F.6
- Mezzena, R.1
- Mion, A.1
- Ortolan, A.7
- Poggi, S.
- Prodi, G. A.1
- Re, V.1
- Salemi, F.1
- Soranzo, G.8
- Taffarello, L.8
- Vedovato, G.8
- Vinante, A.3
- Vitale, S.1
- Zendri, J. P.8
- Abbott, B.9
- Abbott, R.9
-
Adhikari, Rana X.9
- Agresti, J.9
-
Ajith, P.10
- Allen, B.10, 11
- Amin, R.12
- Anderson, S. B.9
- Anderson, W. G.11
- Arain, M.13
-
Araya, M. C.9
- Armandula, H.9
- Ashley, M.14
- Aston, S.15
- Aufmuth, P.
- Aulbert, C.10
- Babak, S.10
- Ballmer, S.9
- Bantilan, H.16
- Barish, B. C.9
- Barker, C.9
- Barker, D.9
- Barr, B.17
- Barriga, P.18
- Barton, M. A.17
- Bayer, K.19
- Belczynski, K.20
- Betzwieser, J.19
- Beyersdorf, P. T.21
- Bhawal, B.9
- Bilenko, I. A.22
-
Billingsley, G.9
-
Biswas, R.11
- Black, E.9
- Blackburn, K.9
- Blackburn, L.19
- Blair, D.18
- Bland, B.9
- Bogenstahl, J.17
- Bogue, L.9
- Bork, R.9
- Boschi, V.9
-
Bose, S.23
-
Brady, P. R.11
- Braginsky, V. B.22
- Brau, J. E.24
- Brinkmann, M.10
- Brooks, A.
-
Brown, D. A.9
- Bullington, A.25
- Bunkowski, A.10
- Buonanno, A.26
- Burmeister, O.10
- Busby, D.9
- Butler, W. E.27
-
Byer, R. L.25
- Cadonati, L.19
- Cagnoli, G.17
- Camp, J. B.28
- Cannizzo, J.28
- Cannon, K.11
- Cantley, C. A.17
- Cao, J.19
- Cardenas, L.9
- Carter, K.9
- Casey, M. M.17
- Castaldi, G.29
- Cepeda, C.9
- Chalkley, E.17
- Charlton, P.30
- Chatterji, S.9
- Chelkowski, S.10
-
Chen, Yanbei10
- Chiadini, F.31
- Chin, D.32
- Chin, E.18
- Chow, J.14
- Christensen, N.16
- Clark, J.17
- Cochrane, P.10
- Cokelaer, T.33
- Colacino, C. N.15
- Coldwell, R.13
- Conte, R.31
- Cook, D.9
-
Corbitt, T.19
- Coward, D.18
-
Coyne, D.9
-
Creighton, J. D. E.11
- Creighton, T. D.9
- Croce, R. P.29
- Crooks, D. R. M.17
- Cruise, A. M.15
- Cumming, A.17
- Dalrymple, J.34
- D'Ambrosio, E.9
- Danzmann, K.10
- Davies, G.33
- DeBra, D.25
- Degallaix, J.18
- Degree, M.25
- Demma, T.29
- Dergachev, V.32
- Desai, S.35
- DeSalvo, R.9
- Dhurandhar, S.36
- Díaz, M.37
- Dickson, J.14
- Di Credico, A.34
- Diederichs, G.
- Dietz, A.33
- Doomes, E. E.38
- Drever, R. W. P.39
- Dumas, J. C.18
- Dupuis, R. J.9
- Dwyer, J. G.40
- Ehrens, P.9
- Espinoza, E.9
- Etzel, T.9
-
Evans, M.9
-
Evans, T.9
- Fairhurst, S.9, 33
- Fan, Y.18
- Fazi, D.9
-
Fejer, M. M.25
- Finn, L. S.35
- Fiumara, V.31
- Fotopoulos, N.11
- Franzen, A.
- Franzen, K. Y.13
-
Freise, A.15
- Frey, R.24
- Fricke, T.27
- Fritschel, P.19
- Frolov, V. V.9
- Fyffe, M.9
- Galdi, V.29
- Ganezer, K. S.41
- Garofoli, J.9
- Gholami, I.10
- Giaime, J. A.12, 9
- Giampanis, S.27
- Giardina, K. D.9
- Goda, K.19
- Goetz, E.32
- Goggin, L. M.9
- González, G.12
- Gossler, S.14
- Grant, A.17
- Gras, S.18
- Gray, C.9
- Gray, M.14
- Greenhalgh, J.42
- Gretarsson, A. M.43
- Grosso, R.37
- Grote, H.10
- Grunewald, S.10
- Guenther, M.9
- Gustafson, R.32
- Hage, B.
- Hammer, D.11
- Hanna, C.12
- Hanson, J.9
-
Harms, J.10
- Harry, G.19
- Harstad, E.24
- Hayler, T.42
- Heefner, J.9
- Heng, I. S.17
- Heptonstall, A.17
- Heurs, M.10
- Hewitson, M.10
- Hild, S.
- Hirose, E.34
- Hoak, D.9
- Hosken, D.
- Hough, J.17
- Howell, E.18
- Hoyland, D.15
- Huttner, S. H.17
- Ingram, D.9
- Innerhofer, E.19
- Ito, M.24
- Itoh, Y.11
- Ivanov, A.9
- Jackrel, D.25
- Johnson, B.9
- Johnson, W. W.12
- Jones, D. I.44
- Jones, G.33
- Jones, R.17
- Ju, L.18
- Kalmus, P.40
-
Kalogera, V.20
- Kasprzyk, D.15
- Katsavounidis, E.19
- Kawabe, K.9
- Kawamura, S.45
- Kawazoe, F.45
- Kells, W.9
- Keppel, D. G.9
- Khalili, F. Ya.22
- Kim, C.20
- King, P.9
-
Kissel, J. S.12
- Klimenko, S.13
- Kokeyama, K.45
- Kondrashov, V.9
- Kopparapu, R. K.12
-
Kozak, D.9
- Krishnan, B.10
- Kwee, P.
- Lam, P. K.14
- Landry, M.9
- Lantz, B.25
- Lazzarini, A.9
- Lee, B.18
- Lei, M.9
- Leiner, J.23
- Leonhardt, V.45
- Leonor, I.24
-
Libbrecht, K.9
- Lindquist, P.9
- Lockerbie, N. A.46
- Longo, M.31
- Lormand, M.9
- Lubinski, M.9
- Lück, H.10
- Machenschalk, B.10
- MacInnis, M.19
- Mageswaran, M.9
- Mailand, K.9
- Malec, M.
- Mandic, V.9
- Marano, S.31
- Márka, S.40
- Markowitz, J.19
- Maros, E.9
- Martin, I.17
- Marx, J. N.9
- Mason, K.19
- Matone, L.40
- Matta, V.31
- Mavalvala, N.19
- McCarthy, R.9
- McClelland, D. E.14
- McGuire, S. C.38
- McHugh, M.47
- McKenzie, K.14
- McNabb, J. W. C.35
- McWilliams, S.28
- Meier, T.
- Melissinos, A.27
- Mendell, G.9
- Mercer, R. A.13
- Meshkov, S.9
- Messenger, C. J.17
- Meyers, D.9
- Mikhailov, E.19
- Mitra, S.36
- Mitrofanov, V. P.22
- Mitselmakher, G.13
- Mittleman, R.19
- Miyakawa, O.9
- Mohanty, S.37
- Moreno, G.9
- Mossavi, K.10
- MowLowry, C.14
- Moylan, A.14
- Mudge, D.
-
Mueller, G.13
- Mukherjee, S.37
- Müller-Ebhardt, H.10
- Munch, J.
- Murray, P.17
- Myers, E.9
- Myers, J.9
- Nash, T.9
- Newton, G.17
-
Nishizawa, A.45
- Nocera, F.9
- Numata, K.28
- O'Reilly, B.9
-
O'Shaughnessy, R.20
-
Ottaway, D. J.19
- Overmier, H.9
- Owen, B. J.35
- Pan, Y.26
- Papa, M. A.11
- Parameshwaraiah, V.9
- Parameshwaraiah, C.9
- Patel, P.9
- Pedraza, M.9
- Penn, S.48
- Pierro, V.29
- Pinto, I. M.29
- Pitkin, M.17
- Pletsch, H.10
- Plissi, M. V.17
- Postiglione, F.31
- Prix, R.10
-
Quetschke, V.13
- Raab, F.9
- Rabeling, D.14
- Radkins, H.9
- Rahkola, R.24
- Rainer, N.10
- Rakhmanov, M.35
- Ramsunder, M.35
- Rawlins, K.19
- Ray-Majumder, S.11
- Regimbau, T.33
- Rehbein, H.10
- Reid, S.17
-
Reitze, D. H.13
- Ribichini, L.10
- Riesen, R.9
- Riles, K.32
- Rivera, B.9
- Robertson, N. A.9, 17
- Robinson, C.33
- Robinson, E. L.15
- Roddy, S.9
- Rodriguez, A.12
- Rogan, A. M.23
- Rollins, J.40
- Romano, J. D.33
- Romie, J.9
- Route, R.25
- Rowan, S.17
- Rüdiger, A.10
- Ruet, L.19
- Russell, P.9
- Ryan, K.9
- Sakata, S.45
- Samidi, M.9
- Sancho de la Jordana, L.49
- Sandberg, V.9
-
Sanders, G. H.9
- Sannibale, V.9
- Saraf, S.50
- Sarin, P.19
- Sathyaprakash, B. S.33
- Sato, S.45
- Saulson, P. R.34
- Savage, R.9
- Savov, P.39
- Sazonov, A.13
- Schediwy, S.18
- Schilling, R.10
-
Schnabel, R.10
- Schofield, R.24
- Schutz, B. F.10, 33
- Schwinberg, P.9
- Scott, S. M.14
- Searle, A. C.14
- Sears, B.9
- Seifert, F.10
- Sellers, D.9
- Sengupta, A. S.33
- Shawhan, P.26
- Shoemaker, D. H.19
- Sibley, A.9
-
Siemens, X.9, 39
-
Sigg, D.9
- Sinha, S.25
- Sintes, A. M.10, 49
-
Slagmolen, B. J. J.14
- Slutsky, J.12
- Smith, J. R.10
- Smith, M. R.9
- Somiya, K.10
- Strain, K. A.17
- Strom, D. M.24
- Stuver, A.35
- Summerscales, T. Z.51
- Sun, K. X.25
- Sung, M.12
- Sutton, P. J.9
- Takahashi, H.10
-
Tanner, D. B.13
- Tarallo, M.9
- Taylor, R.9
- Taylor, R.17
- Thacker, J.9
- Thorne, K. A.35
- Thorne, K. S.39
- Thüring, A.
-
Tinto, M.9
- Tokmakov, K. V.17
- Torres, C.37
- Torrie, C.17
- Traylor, G.9
- Trias, M.49
- Tyler, W.9
- Ugolini, D.52
- Ungarelli, C.15
- Urbanek, K.25
- Vahlbruch, H.
-
Vallisneri, M.39
- Van Den Broeck, C.33
-
van Putten, M.19
- Varvella, M.9
- Vass, S.9
-
Vecchio, A.15
- Veitch, J.17
- Veitch, P.
- Villar, A.9
- Vorvick, C.9
- Vyachanin, S. P.22
- Waldman, S. J.9
- Wallace, L.9
- Ward, H.17
- Ward, R.9
- Watts, K.9
- Webber, D.9
- Weidner, A.10
- Weinert, M.10
- Weiss, R.9
- Wen, S.19
- Wette, K.12
- Whelan, J. T.14
- Whitbeck, D. M.10
- Whitcomb, S. E.35
-
Whiting, B. F.9
- Wiley, S.13
- Wilkinson, C.41
- Willems, P. A.9
- Williams, L.9
- Willke, B.13
- Wilmut, I.10
- Winkler, W.42
- Wipf, C. C.10
- Wise, S.19
- Wiseman, A. G.13
- Woan, G.11
- Woods, D.17
- Wooley, R.11
-
Worden, J.9
- Wu, W.9
- Yakushin, I.13
- Yamamoto, H.9
- Yan, Z.9
- Yoshida, S.18
-
Yunes, N.53
- Zanolin, M.35
- Zhang, J.19
-
Zhang, L.32
-
Zhao, C.9
- Zotov, N.18
-
Zucker, M.54
- zur Mühlen, H.19
-
Zweizig, J.
-
Weinstein, Alan J.9
-
1.
University of Trento
-
2.
University of Padua
-
3.
Istituto di Fotonica e Nanotecnologie
-
4.
University of Ferrara
-
5.
National Research Council
-
6.
University of Florence
-
7.
Legnaro National Laboratories
-
8.
INFN Sezione di Padova
-
9.
Laser Interferometer Gravitational Wave Observatory
-
10.
Max Planck Institute for Gravitational Physics
-
11.
University of Wisconsin–Milwaukee
-
12.
Louisiana State University
-
13.
University of Florida
-
14.
Australian National University
-
15.
University of Birmingham
-
16.
Carleton College
-
17.
University of Glasgow
-
18.
University of Western Australia
-
19.
Massachusetts Institute of Technology
-
20.
Northwestern University
-
21.
San Jose State University
-
22.
Lomonosov Moscow State University
-
23.
Washington State University
-
24.
University of Oregon
-
25.
Stanford University
-
26.
University of Maryland, College Park
-
27.
University of Rochester
-
28.
Goddard Space Flight Center
-
29.
University of Sannio
-
30.
Charles Sturt University
-
31.
University of Salerno
-
32.
University of Michigan–Ann Arbor
-
33.
Cardiff University
-
34.
Syracuse University
-
35.
Pennsylvania State University
-
36.
Inter-University Centre for Astronomy and Astrophysics
-
37.
The University of Texas Rio Grande Valley
-
38.
Southern University and Agricultural and Mechanical College
-
39.
California Institute of Technology
-
40.
Columbia University
-
41.
California State University, Dominguez Hills
-
42.
Rutherford Appleton Laboratory
-
43.
Embry–Riddle Aeronautical University
-
44.
University of Southampton
-
45.
National Astronomical Observatory of Japan
-
46.
University of Strathclyde
-
47.
Loyola University New Orleans
-
48.
Hobart and William Smith Colleges
-
49.
University of the Balearic Islands
-
50.
Rochester Institute of Technology
-
51.
Andrews University
-
52.
Trinity University
-
53.
Southeastern Louisiana University
-
54.
Louisiana Tech University
Abstract
The first simultaneous operation of the AURIGA detector and the LIGO observatory was an opportunity to explore real data, joint analysis methods between two very different types of gravitational wave detectors: resonant bars and interferometers. This paper describes a coincident gravitational wave burst search, where data from the LIGO interferometers are cross-correlated at the time of AURIGA candidate events to identify coincident transients. The analysis pipeline is tuned with two thresholds, on the signal-to-noise ratio of AURIGA candidate events and on the significance of the cross-correlation test in LIGO. The false alarm rate is estimated by introducing time shifts between data sets and the network detection efficiency is measured by adding simulated gravitational wave signals to the detector output. The simulated waveforms have a significant fraction of power in the narrower AURIGA band. In the absence of a detection, we discuss how to set an upper limit on the rate of gravitational waves and to interpret it according to different source models. Due to the short amount of analyzed data and to the high rate of non-Gaussian transients in the detectors' noise at the time, the relevance of this study is methodological: this was the first joint search for gravitational wave bursts among detectors with such different spectral sensitivity and the first opportunity for the resonant and interferometric communities to unify languages and techniques in the pursuit of their common goal.
Additional Information
© 2008 IOP Publishing Ltd. Received 18 October 2007, in final form 25 January 2008 Published 15 April 2008. http://stacks.iop.org/ CQG/25/095004 The LIGO Scientific Collaboration (LSC) gratefully acknowledge the support of the United States National Science Foundation for the construction and operation of the LIGO Laboratory and the Science and Technology Facilities Council of the United Kingdom, the Max-Planck- Society, and the State of Niedersachsen/Germany for support of the construction and operation of theGEO600 detector. The authors also gratefully acknowledge the support of the research by these agencies and by the Australian Research Council, the Council of Scientific and Industrial Research of India, the Istituto Nazionale di Fisica Nucleare of Italy, the Spanish Ministerio de Educaciόn y Ciencia, the Conselleria d'Economia, Hisenda i Innovaciό of the Govern de les Illes Balears, the Scottish Funding Council, the Scottish Universities Physics Alliance, The National Aeronautics and Space Administration, the Carnegie Trust, the Leverhulme Trust, the David and Lucile Packard Foundation, the Research Corporation, and the Alfred P Sloan Foundation. The AURIGA Collaboration acknowledges the support of the research by the Istituto Nazionale di Fisica Nucleare (INFN), the Universities of Ferrara, Firenze, Padova and Trento, the Center of Trento of the Istituto di Fotonica e Nanotecnologie - Istituto Trentino di Cultura and the Consorzio Criospazio Ricerche of Trento. This paper was assigned LIGO document number P070086-04.Additional details
Identifiers
- Eprint ID
- 14467
- Resolver ID
- CaltechAUTHORS:20090630-134133512
Funding
- NSF
- Science and Technology Facilities Council (STFC)
- State of Niedersachsen/Germany
- Australian Research Council
- Council of Scientific and Industrial Research (India)
- Istituto Nazionale di Fisica Nucleare (INFN)
- Ministerio de Educaciόn y Ciencia (MEC)
- Scottish Funding Council
- Scottish Universities Physics Alliance
- NASA
- Carnegie Trust
- Leverhulme Trust
- David and Lucile Packard Foundation
- Alfred P. Sloan Foundation
- Universities of Ferrara, Firenze, Padova and Trento
- Center of Trento of the Istituto di Fotonica e Nanotecnologie- Istituto Trentino di Cultura and the Consorzio Criospazio Ricerche of Trento
- Max-Planck-Society
- Conselleria d'Economia, Hisenda i Innovaciό of the Govern de les Illes Balears
Dates
- Created
-
2009-08-29Created from EPrint's datestamp field
- Updated
-
2023-03-16Created from EPrint's last_modified field
Caltech Custom Metadata
- Caltech groups
- TAPIR , LIGO , Physics Department
- Other Numbering System Name
- LIGO Document
- Other Numbering System Identifier
- P070086-04