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          Document History for Document ID 119694

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Document Version Version Comment Date Status
119694.0 [No comment] 06.04.2009 13:48 Released

ID: 119694.0, MPI für Gravitationsphysik / Laser Interferometry & Gravitational Wave Astronomy
Upper limits on the strength of periodic gravitational waves from PSR J1939+2134
Authors:Woan, G.; Allen, Bruce; Abbott, B.; Abbott, F.; Adhikari, R.; Amin, R.; Anderson, S. B.; Anderson, W. G.; Araya, M.; Armandula, H.; Asiri, F.; Aufmuth, Peter; Aulbert, Carsten; Babak, Stanislav; Balasubramanian, R.; Ballmer, S.; Barish, B. C.; Barker, D.; Barker-Patton, C.; Barnes, M.; Barr, B. W.; Barton, M. A.; Bayer, K.; Beausoleil, R.; Belczynski, K.; Bennett, R.; Berukoff, Steven J.; Betzwieser, J.; Bhawal, B.; Billingsley, G.; Black, E.; Blackburn, K.; Bland-Weaver, B.; Bochner, B.; Bogue, L.; Bork, Rolf; Bose, Sukanta; Brady, Patrick R.; Braginsky, V. B.; Brau, J. E.; Brown, Duncan A.; Brozek, Oliver Sascha; Bullington, A.; Buonanno, Alessandra; Burgess, R.; Busby, D.; Butler, W. E.; Byer, R. L.; Cadonati, L.; Cagnoli, G.; Camp, J. B.; Cantley, C. A.; Cardenas, L.; Carter, K.; Casey, Morag M.; Castiglione, J.; Chandler, A.; Chapsky, J.; Charlton, P.; Chatterji, S.; Chen, Yanbei; Chickarmane, V.; Chin, D.; Christensen, Nelson; Churches, D.; Colacino, Carlo Nicola; Coldwell, R.; Coles, M.; Cook, D.; Corbitt, Thomas; Coyne, D.; Creighton, Jolien D. E.; Creighton, Teviet D.; Crooks, D. R. M.; Csatorday, P.; Cusack, B. J.; Cutler, Curt; D'Ambrosio, Erika; Danzmann, Karsten; Davies, R.; Daw, Edward J.; DeBra, D.; Delker, T.; DeSalvo, R.; Dhurandhar, Sanjeev; Diaz, M.; Ding, H.; Drever, R. W. P.; Dupuis, R. J.; Ebeling, C.; Edlund, J. A.; Ehrens, P.; Elliffe, E. J.; Etzel, T.; Evans, M.; Evans, T.; Fallnich, Carsten; Farnham, D.; Fejer, M. M.; Fine, M.; Finn, Lee S.; Flanagan, Eanna E.; Freise, Andreas; Frey, R.; Fritschel, P.; Frolov, V. V.; Ganezer, K. S.; Giaime, J. A.; Gillespie, A.; Goda, Keisuke; Gonzalez, Gabriela; Gossler, Stefan; Grandclement, P.; Grant, A.; Gray, C.; Gretarsson, A. M.; Grimmett, D.; Grote, Hartmut; Grunewald, Steffen; Guenther, Mathias; Gustafson, E. K.; Gustafson, R.; Hamilton, W. O.; Hammond, M.; Hanson, J.; Hardham, C.; Harry, G.; Hartunian, A.; Heefner, J.; Hefetz, Y.; Heinzel, Gerhard; Heng, Ik Siong; Hennessy, M.; Hepler, N.; Heptonstall, A.; Heurs, Michele; Hewitson, Martin; Hindman, N.; Hoang, P.; Hough, Jim; Hrynevych, M.; Hua, W.; Ingley, R.; Ito, M.; Itoh, Yousuke; Ivanov, A.; Jennrich, Oliver; Johnson, W. W.; Johnston, W. R.; Jones, L.; Jungwirth, D.; Kalogera, V.; Katsavounidis, E.; Kawabe, Keita; Kawamura, Seiji; Kells, W.; Kern, J.; Khan, A.; Killbourn, S.; Killow, Christian J.; Kim, C.; King, C.; King, Peter; Klimenko, S.; Kloevekorn, P.; Koranda, S.; Kötter, Karsten; Kovalik, J.; Kozak, D.; Krishnan, Badri; Landry, Michael; Langdale, J.; Lantz, B.; Lawrence, R.; Lazzarini, Albert; Lei, M.; Leonhardt, Volker; Leonor, I.; Libbrecht, K.; Lindquist, P.; Liu, S.; Logan, J. E.; Lormand, M.; Lubinski, M.; Lück, Harald; Lyons, T. T.; Machenschalk, Bernd; MacInnis, M.; Mageswaran, M.; Mailand, K.; Majid, W.; Malec, Michaela; Mann, F.; Marin, A.; Marka, S.; Maros, E.; Mason, J.; Matherny, O.; Mason, K.; Matone, L.; Mavalvala, N.; McCarthy, R.; McClelland, D. E.; McHugh, Martin; McNamara, P. W.; Mendell, Gregory; Meshkov, S.; Messenger, Christopher; Mitrofanov, V. P.; Mitselmakher, G.; Mittleman, R.; Miyakawa, O.; Miyoki, Shinji; Mohanty, Soumya; Moreno, G.; Mossavi, Kasem; Mours, B.; Müller, G.; Mukherjee, Soma; Myers, J.; Naganov, S.; Nash, T.; Naundorf, Holger; Nayak, R.; Newton, G.; Nocera, F.; Nutzman, P.; Olson, T.; O'Reilly, B.; Ottaway, D. J.; Ottewill, A.; Ouimette, D.; Overmier, H.; Owen, Benjamin J.; Papa, Maria Alessandra; Parameswariah, C.; Parameswariah, V.; Pedraza, M.; Penn, S.; Pitkin, Matthew; Plissi, M. V.; Pratt, M.; Quetschke, Volker; Raab, F.; Radkins, H.; Rahkola, R.; Rakhmanov, M.; Rao, S. R.; Redding, D.; Regehr, M. W.; Regimbau, T.; Reilly, K. T.; Reithmaier, K.; Reitze, D. H.; Richman, S.; Riesen, R.; Riles, K.; Rizzi, A.; Robertson, D. I.; Robertson, N. A.; Robison, L.; Roddy, S.; Rollins, J.; Romano, J. D.; Romie, J.; Rong, H.; Rose, D.; Rotthoff, E.; Rowan, S.; Rüdiger, Albrecht; Russell, P.; Ryan, K.; Salzman, I.; Sanders, G. H.; Sannibale, V.; Sathyaprakash, B.; Saulson, P. R.; Savage, R.; Sazonov, A.; Schilling, Roland; Schlaufman, K.; Schmidt, V.; Schofield, R.; Schrempel, M.; Schutz, Bernard F.; Schwinberg, P.; Scott, S. M.; Searle, A. C.; Sears, B.; Seel, S.; Sengupta, A. S.; Shapiro, C. A.; Shawhan, P.; Shoemaker, D. H.; Shu, Q. Z.; Sibley, A.; Siemens, X.; Sievers, L.; Sigg, D.; Sintes, Alicia M.; Skeldon, K. D.; Smith, J. R.; Smith, M.; Smith, M. R.; Sneddon, P.; Spero, R.; Stapfer, G.; Strain, Kenneth A.; Strom, D.; Stuver, A.; Summerscales, T.; Sumner, M. C.; Sutton, Patrick J.; Sylvestre, J.; Takamori, A.; Tanner, D. B.; Tariq, H.; Taylor, I.; Taylor, R.; Thorne, Kip S.; Tibbits, M.; Tilav, S.; Tinto, Massimo; Fyffe, M.; Torres, C.; Torrie, C.; Traeger, S.; Traylor, G.; Tyler, W.; Ugolini, D.; Vallisneri, M.; van Putten, M.; Vass, S.; Vecchio, Alberto; Vorvick, C.; Vyatchanin, S. P.; Wallace, L.; Walther, H.; Ward, H.; Ware, B.; Watts, K.; Webber, D.; Weidner, Andreas; Weiland, Uta; Weinstein, A.; Weiss, R.; Welling, Herbert; Wen, L.; Wen, S.; Whelan, John T.; Whitcomb, S. E.; Whiting, B. F.; Willems, P. A.; Williams, P. R.; Williams, R.; Willke, Benno; Wilson, A.; Winjum, B. J.; Winkler, Walter; Wise, S.; Wiseman, A. G.; Wooley, R.; Worden, J.; Yakushin, I.; Yamamoto, H.; Yoshida, S.; Zawischa, Ivo; Zhang, L.; Zotov, N.; Zucker, M.; Zweizig, J.
Language:English
Date of Publication (YYYY-MM-DD):2004
Title of Journal:Classical and Quantum Gravity
Volume:21
Issue / Number:5
Start Page:S671
End Page:S676
Review Status:not specified
Audience:Not Specified
Abstract / Description:The first science run of the LIGO and GEO gravitational wave detectors presented the opportunity to test methods of searching for gravitational waves from known pulsars. Here we present new direct upper limits on the strength of waves from the pulsar PSR J1939+2134 using two independent analysis methods, one in the frequency domain using frequentist statistics and one in the time domain using Bayesian inference. Both methods show that the strain amplitude at Earth from this pulsar is less than a few times 10-22.
External Publication Status:published
Document Type:Article
Communicated by:Karsten Danzmann
Affiliations:MPI für Gravitationsphysik/Teilinstitut Hannover
MPI für Gravitationsphysik/GEO 600
MPI für Gravitationsphysik/Laser Interferometry & Gravitational Wave Astronomy
MPI für Gravitationsphysik/Observational Relativity and Cosmology
MPI für Gravitationsphysik/Astrophysical Relativity
Identifiers:ISSN:0264-9381
DOI:10.1088/0264-9381/21/5/042
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