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Upper limits on the strength of periodic gravitational waves from PSR J1939+2134

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

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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.


PACS

04.80.Nn Gravitational wave detectors and experiments

95.55.Ym Gravitational radiation detectors; mass spectrometers; and other instrumentation and techniques

97.60.Gb Pulsars

95.75.Wx Time series analysis, time variability

95.75.Pq Mathematical procedures and computer techniques

MSC

83C35 Gravitational waves

85A35 Statistical astronomy

Subjects

Instrumentation and measurement

Gravitation and cosmology

Astrophysics and astroparticles

Dates

Issue 5 (7 March 2004)

Received 2 October 2003

Published 9 February 2004



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