B Allen et al 2004 Class. Quantum Grav. 21 S671 doi:10.1088/0264-9381/21/5/042
B Allen39, G Woan35, (for the LIGO Scientific Collaboration), B Abbott13, R Abbott13, R Adhikari14, B Allen39, R Amin34, S B Anderson13, W G Anderson29, M Araya13, H Armandula13, F Asiri13, P Aufmuth31, C Aulbert1, S Babak7, R Balasubramanian7, S Ballmer14, B C Barish13, D Barker15, C Barker-Patton15, M Barnes13, B Barr35, M A Barton13, K Bayer14, R Beausoleil26, K Belczynski23, R Bennett35, S J Berukoff1, J Betzwieser14, B Bhawal13, G Billingsley13, E Black13, K Blackburn13, B Bland-Weaver15, B Bochner14, L Bogue13, R Bork13, S Bose40, P R Brady39, J E Brau37, D A Brown39, S Brozek31, A Bullington26, A Buonanno6, R Burgess14, D Busby13, W E Butler38, R L Byer26, L Cadonati14, G Cagnoli35, J B Camp21, C A Cantley35, L Cardenas13, K Carter16, M M Casey35, J Castiglione34, A Chandler13, J Chapsky13, P Charlton13, S Chatterji14, Y Chen6, V Chickarmane17, D Chin36, N Christensen8, D Churches7, C Colacino31,2, R Coldwell34, M Coles16, D Cook15, T Corbitt14, D Coyne13, J D E Creighton39, T D Creighton13, D R M Crooks35, P Csatorday14, B J Cusack3, C Cutler1, E D'Ambrosio13, K Danzmann31,2,20, R Davies7, E Daw17, D DeBra26, T Delker34, R DeSalvo13, S Dhurandar12, M Díaz29, H Ding13, R W P Drever4, R J Dupuis35, C Ebeling8, J Edlund13, P Ehrens13, E J Elliffe35, T Etzel13, M Evans13, T Evans16, C Fallnich31, D Farnham13, M M Fejer26, M Fine13, L S Finn28, É Flanagan9, A Freise2, R Frey37, P Fritschel14, V Frolov16, M Fyffe16, K S Ganezer5, J A Giaime17, A Gillespie13, K Goda14, G González17, S Goßler31, P Grandclément23, A Grant35, C Gray15, A M Gretarsson16, D Grimmett13, H Grote2, S Grunewald1, M Guenther15, E Gustafson26, R Gustafson36, W O Hamilton17, M Hammond16, J Hanson16, C Hardham26, G Harry14, A Hartunian13, J Heefner13, Y Hefetz14, G Heinzel2, I S Heng31, M Hennessy26, N Hepler28, A Heptonstall35, M Heurs31, M Hewitson35, N Hindman15, P Hoang13, J Hough35, M Hrynevych13, W Hua26, R Ingley33, M Ito37, Y Itoh1, A Ivanov13, O Jennrich35, W W Johnson17, W Johnston29, L Jones13, D Jungwirth13, V Kalogera23, E Katsavounidis14, K Kawabe20,2, S Kawamura22, W Kells13, J Kern16, A Khan16, S Killbourn35, C J Killow35, C Kim23, C King13, P King13, S Klimenko34, P Kloevekorn2, S Koranda39, K Kötter31, J Kovalik16, D Kozak13, B Krishnan1, M Landry15, J Langdale16, B Lantz26, R Lawrence14, A Lazzarini13, M Lei13, V Leonhardt31, I Leonor37, K Libbrecht13, P Lindquist13, S Liu13, J Logan13, M Lormand16, M Lubinski15, H Lück31,2, T T Lyons13, B Machenschalk1, M MacInnis14, M Mageswaran13, K Mailand13, W Majid13, M Malec31, F Mann13, A Marin14, S Márka13, E Maros13, J Mason13, K Mason14, O Matherny15, L Matone15, N Mavalvala14, R McCarthy15, D E McClelland3, M McHugh19, P McNamara35, G Mendell15, S Meshkov13, C Messenger33, G Mitselmakher34, R Mittleman14, O Miyakawa13, S Miyoki13, S Mohanty1, G Moreno15, K Mossavi2, B Mours13, G Mueller34, S Mukherjee1, J Myers15, S Nagano2, T Nash10, H Naundorf1, R Nayak12, G Newton35, F Nocera13, P Nutzman23, T Olson24, B O'Reilly16, D J Ottaway14, A Ottewill39, D Ouimette13, H Overmier16, B J Owen28, M A Papa1, C Parameswariah16, V Parameswariah15, M Pedraza13, S Penn11, M Pitkin35, M Plissi35, M Pratt14, V Quetschke31, F Raab15, H Radkins15, R Rahkola37, M Rakhmanov34, S R Rao13, D Redding13, M W Regehr13, T Regimbau14, K T Reilly13, K Reithmaier13, D H Reitze34, S Richman14, R Riesen16, K Riles36, A Rizzi16, D I Robertson35, N A Robertson35,26, L Robison13, S Roddy16, J Rollins14, J D Romano29, J Romie13, H Rong34, D Rose13, E Rotthoff28, S Rowan35, A Rüdiger20,2, P Russell13, K Ryan15, I Salzman13, G H Sanders13, V Sannibale13, B Sathyaprakash7, P R Saulson27, R Savage15, A Sazonov34, R Schilling20,2, K Schlaufman28, V Schmidt13, R Schofield37, M Schrempel31, B F Schutz1,7, P Schwinberg15, S M Scott3, A C Searle3, B Sears13, S Seel13, A S Sengupta12, C A Shapiro28, P Shawhan13, D H Shoemaker14, Q Z Shu34, A Sibley16, X Siemens39, L Sievers13, D Sigg15, A M Sintes1,32, K Skeldon35, J R Smith2, M Smith14, M R Smith13, P Sneddon35, R Spero13, G Stapfer16, K A Strain35, D Strom37, A Stuver28, T Summerscales28, M C Sumner13, P J Sutton28, J Sylvestre13, A Takamori13, D B Tanner34, H Tariq13, I Taylor7, R Taylor13, K S Thorne6, M Tibbits28, S Tilav13, M Tinto4, C Torres29, C Torrie13,35, S Traeger31, G Traylor16, W Tyler13, D Ugolini30, M Vallisneri6, M van Putten14, S Vass13, A Vecchio33, C Vorvick15, L Wallace13, H Walther20, H Ward35, B Ware13, K Watts16, D Webber13, A Weidner20,2, U Weiland31, A Weinstein13, R Weiss14, H Welling31, L Wen13, S Wen17, J T Whelan19, S E Whitcomb13, B F Whiting34, P A Willems13, P R Williams1, R Williams4, B Willke31,2, A Wilson13, B J Winjum28, W Winkler20,2, S Wise34, A G Wiseman39, G Woan35, R Wooley16, J Worden15, I Yakushin16, H Yamamoto13, S Yoshida25, I Zawischa31, L Zhang13, N Zotov18, M Zucker16 and J Zweizig13
Show affiliationsThe 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.
04.80.Nn Gravitational wave detectors and experiments
Issue 5 (7 March 2004)
Received 2 October 2003
Published 9 February 2004
B Allen et al 2004 Class. Quantum Grav. 21 S671
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