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

B Allen ,D Farnham ,H Lück ,R Davies ,Keisuke Goda ,J H Romie ,C J Killow ,B S Sathyaprakash ,Vijay Chickarmane ,C Kim ,V V Frolov ,M Guenther ,Dieter Jungwirth ,S Brozek ,R J Dupuis ,Y Hefetz ,J Worden ,S Wise ,C Barker-Patton ,K Mossavi ,F Nocera ,S Márka ,M Lormand ,H Armandula ,Jeffrey A Edlund ,A M Sintes ,Duncan Brown ,Adrian C Ottewill ,T Delker ,L Wen ,Richard Ingley ,D J Ottaway ,P W Mcnamara ,J Heefner ,R Mittleman ,R L Coldwell ,B Bochner ,M Łubiński ,P Kloevekorn ,J Hanson ,G Mueller ,D C Coyne ,S Tilav ,C Hardham ,S Babak ,E Maros ,Brent Ware ,G H Sanders ,F.m Mann ,Masahiro Ito ,K Carter ,Kip S Thorne ,K Reithmaier ,M Macinnis ,Kenneth G Libbrecht ,Éanna É Flanagan ,D De Bra ,D R M Crooks ,C N Colacino ,D Churches ,R D Williams ,William E Butler ,J Logan ,M Schrempel ,D B Tanner ,H Walther ,P Lindquist ,K Kötter ,N Zotov ,Soma Mukherjee ,M Evans ,Ian Taylor ,G Mitselmakher ,L Jones ,Carsten Fallnich ,W Hua ,S M Scott ,S Roddy ,M Coles ,Raymond G Beausoleil ,S Seel ,V Schmidt ,A Chandler ,D Cook ,R Mccarthy ,H Ward ,I Zawischa ,R Wooley ,M A Papa ,S D Mohanty ,V Parameswariah ,S Traeger ,P R Brady ,G Billingsley ,J Hough ,M Hrynevych ,M Hennessy ,B P Abbott ,R Lawrence ,David C Redding ,K Watts ,John Langdale ,J T Whelan ,M E Zucker ,A Rizzi ,S Grünewald ,James Mason ,D Ouimette ,M Hewitson ,K Belczyński ,R Bork ,L Sievers ,A C Searle ,J Kovalik ,M C Díaz ,G Mendell ,W G Anderson ,V Sannibale ,M Van Putten ,U Weiland ,S Liu ,B F Whiting ,I Leonor ,Kevin C Schlaufman ,R W P Drever ,H Ding ,R K Nayak ,D E Mcclelland ,R Amin ,D B Kozak ,A M Gretarsson ,Shanti Rao ,S Klimenko ,O Miyakawa ,V Kalogera ,B Barish ,M Lei ,V Leonhardt ,D Barker ,M Rakhmanov ,M Fine ,S Nagano ,C Vorvick ,David Webber ,Andrew Wilson ,E J Daw ,B Bland-Weaver ,G M Harry ,Robert L Byer ,T T Lyons ,M Pitkin ,C I Torrie ,H Grote ,M Heurs ,G Newton ,J E Brau ,L Wallace ,Haisheng Rong ,J Castiglione ,M W Regehr ,M Pedraza ,Robert Spero ,Peter Williams ,E D’ambrosio ,A Sazonov ,M Tibbits ,S Chatterji ,D Rose ,J G Rollins ,W Winkler ,W O Hamilton ,D Sigg ,P J King ,D Ugolini ,William R Johnston ,D Grimmett ,L Zhang ,J D Romano ,Rolf Riesen ,R Burgess ,A Weidner ,C Messenger ,F J Raab ,K D Skeldon ,V Quetschke ,M Mchugh ,A Hartunian ,R X Adhikari ,T M Evans ,J B Camp ,C Gray ,G Woan ,E Katsavounidis ,B Sears ,K Bayer ,G Traylor ,B F Schutz ,C Parameswariah ,R Gustafson ,T R Corbitt ,P Fritschel ,K Mailand ,H Tariq ,B Krishnan ,K S Ganezer ,A Takamori ,K Kawabe ,S Bose ,K Danzmann ,T Regimbau ,J Myers ,P Ehrens ,Holger Naundorf ,K Blackburn ,M C Sumner ,Julien Sylvestre ,L S Finn ,A Grant ,A Ivanov ,L Cardenas ,A Bullington ,S E Whitcomb ,Massimo Tinto ,M Landry ,A Khan ,S Killbourn ,A Heptonstall ,C King ,K Mason ,K T Reilly ,S Vass ,R Rahkola ,D Busby ,B J Winjum ,I Yakushin ,A S Sengupta ,B Barr ,H Yamamoto ,D I Robertson ,X Siemens ,Philippe Grandclément ,J R Smith ,B Mours ,M Fyffe ,I Salzman ,A J Weinstein ,C Aulbert ,P R Saulson ,L Matone ,M Malec ,Timothy S Olson ,R M S Schofield ,A Marin ,D Chin ,P Aufmuth ,S Goßler ,D H Reitze ,P Csatorday ,L Robison ,G Stapfer ,B J Owen ,H Radkins ,R L Savage ,S Koranda ,M M Fejer ,W Tyler ,Robert W Taylor ,A G Wiseman ,L Bogue ,F Asiri ,M Mageswaran ,Y Itoh ,H Overmier ,C A Cantley ,N A Robertson ,Neil Hindman ,K Ryan ,K A Strain ,J Betzwieser ,R Abbott ,B Willke ,N Mavalvala ,P Schwinberg ,S Yoshida ,M A Barton ,J Chapsky ,K Riles ,M V Plissi ,Mónica Barnes ,A Vecchio ,S Richman ,M Hammond ,A L Stuver ,S W Ballmer ,N Hepler ,R Weiss ,S Meshkov ,A Lazzarini ,P Shawhan ,I S Heng ,W Kells ,P A Willems ,R Balasubramanian ,D H Shoemaker ,M C Araya ,E Rotthoff ,M M Casey ,G Cagnoli ,Q Z Shu ,R Schilling ,D Strom ,A Sibley ,P Sneddon ,A Buonanno ,Curt Cutler ,L Cadonati ,T Nash ,J A Giaime ,C Ebeling ,S Dhurandar ,S Penn ,P J Sutton ,R Frey ,T D Creighton ,C Torres ,P Nutzman ,P Russell ,P Charlton ,T Etzel ,Michele Vallisneri ,J D E Creighton ,S B Anderson ,Gerhard Heinzel ,Charles A Shapiro ,W W Johnson ,B Lantz ,O Matherny ,T Z Summerscales ,P Hoang ,J Kern ,N Christensen ,R De Salvo ,M R Pratt ,Gabriela González ,S J Berukoff ,Walid A Majid ,E Black ,S Rowan ,O Jennrich ,S Wen ,M R Smith ,A Gillespie ,B Machenschalk ,A Rüdiger ,E K Gustafson ,R Bennett ,S Miyoki ,B Bhawal ,H Welling ,Y Chen ,B O’reilly ,E J Elliffe ,B J Cusack ,Seiji Kawamura ,G Moreno ,A Freise ,J Zweizig

doi:10.1088/0264-9381/21/5/042

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

B Allen , D Farnham + Show 365 more

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https://doi.org/10.1088/0264-9381/21/5/042

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Journal: Classical and Quantum Gravity	Publication Date: Feb 9, 2004
Citations: 4

Affiliation: California Institute of Technology, Louisiana State University, National Science Foundation, Leibniz University Hannover, Massachusetts Institute of Technology, University of the Balearic Islands, University of Wisconsin–Milwaukee, University of Florida, University of Birmingham, Stanford University, Cardiff University, University of Rochester, Louisiana Tech University, University of Glasgow, Australian National University, The University of Texas at Austin, University of Oregon, Pennsylvania State University, Inter-University Centre for Astronomy and Astrophysics, Trinity University, University of Michigan–Ann Arbor, California State University, Dominguez Hills, Max Planck Society, Northwestern University, Southeastern Louisiana University, Hobart and William Smith Colleges, National Institutes of Natural Sciences

#Strength Of Waves #PSR J1939 + Show 8 more

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Abstract

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.

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