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SEARCHES FOR GRAVITATIONAL WAVES FROM KNOWN PULSARS WITH SCIENCE RUN 5 LIGO DATA

Title:	SEARCHES FOR GRAVITATIONAL WAVES FROM KNOWN PULSARS WITH SCIENCE RUN 5 LIGO DATA
Authors:	ABBOTT BP; ABBOTT R; ACERNESE F; ADHIKARI R; AJITH P; ALLEN B; ALLEN G; ALSHOURBAGY M; AMIN RS; ANDERSON SB; ANDERSON WG; ANTONUCCI F; AOUDIA S; ARAIN MA; ARAYA M; ARMANDULA H; ARMOR P; ARUN KG; ASO Y; ASTON S; ASTONEA P; AUFMUTH P; AULBERT C; BABAK S; BAKER P; BALLARDIN G; BALLMER S; BARKER C; BARKER D; BARONE F; BARR B; BARRIGA P; BARSOTTI L; BARSUGLIA M; BARTON MA; BARTOS I; BASSIRI R; BASTARRIKA M; BAUER TS; BEHNKE B; BEKER M; BENACQUISTA M; BETZWIESER J; BEYERSDORF PT; BIGOTTA S; BILENKO IA; BILLINGSLEY G; BIRINDELLI S; BISWAS R; BIZOUARD MA; BLACK E; BLACKBURN JK; BLACKBURN L; BLAIR D; BLAND B; BOCCARA C; BODIYA TP; BOGUE L; BONDUB F; BONELLI L; BORK R; BOSCHI V; BOSE S; BOSI L; BRACCINIA S; BRADASCHIA C; BRADY PR; BRAGINSKY VB; BRAU JE; BRIDGES DO; BRILLET A; BRINKMANN M; BRISSON V; VAN DEN BROECK C; BROOKS AF; BROWN DA; BRUMMIT A; BRUNET G; BUDZYNSKI R; BULIK T; BULLINGTON A; BULTEN HJ; BUONANNO A; BURMEISTER O; BUSKULIC D; BYER RL; CADONATI L; CAGNOLI G; CALLONI E; CAMP JB; CAMPAGNA E; CANNIZZO J; CANNON KC; CANUEL B; CAO J; CARBOGNANI F; CARDENAS L; CARIDE S; CASTALDI G; CAUDILL S; CAVAGLIA M; CAVALIER F; CAVALIERI R; CELLA G; CEPEDA C; CESARINI E; CHALERMSONGSAK T; CHALKLEY E; CHARLTON P; CHASSANDE MOTTIN E; CHATTERJI S; CHELKOWSKI S; CHEN Y; CHINCARINI A; CHRISTENSEN N; CHUNG CTY; CLARK D; CLARK J; CLAYTON JH; CLEVA F; COCCIA E; COKELAER T; COLACINO CN; COLAS J; COLLA A; COLOMBINI M; CONTE R; COOK D; CORBITT TRC; CORDA C; CORNISH N; CORSI A; COULON JP; COWARD D; COYNE DC; CREIGHTON JDE; CREIGHTON TD; CRUISE AM; CULTER RM; CUMMING A; CUNNINGHAM L; CUOCO E; DANILISHIN SL; D'ANTONIO S; DANZMANN K; DARI A; DATTILO V; DAUDERT B; DAVIER M; DAVIES G; DAW EJ; DAY R; DE ROSA R; DEBRA D; DEGALLAIX J; DEL PRETE M; DERGACHEV V; DESAI S; DESALVO R; DHURANDHAR S; DI FIORE L; DI LIETO A; EMILIO MDP; DI VIRGILIO A; DIAZ M; DIETZ A; DONOVAN F; DOOLEY KL; DOOMES EE; DRAGO M; DREVER RWP; DUECK J; DUKE I; DUMAS JC; DWYER JG; ECHOLS C; EDGAR M; EFFLER A; EHRENS P; ESPINOZA E; ETZEL T; EVANS M; EVANS T; FAFONE V; FAIRHURST S; FALTAS Y; FAN Y; FAZI D; FEHRMANN H; FERRANTE I; FIDECARO F; FINN LS; FIORI I; FLAMINIO R; FLASCH K; FOLEY S; FORREST C; FOTOPOULOS N; FOURNIER JD; FRANC J; FRANZEN A; FRASCONI F; FREDE M; FREI M; FREI Z; FREISE A; FREY R; FRICKE T; FRITSCHEL P; FROLOV VV; FYFFE M; GALDI V; GAMMAITONI L; GAROFOLI JA; GARUFIAB F; GEMME G; GENIN E; GENNAI A; GHOLAMI I; GIAIME JA; GIAMPANIS S; GIARDINA KD; GIAZOTTO A; GODA K; GOETZ E; GOGGIN LM; GONZALEZ G; GORODETSKY ML; GOSSLER S; GOUATY R; GRANATA M; GRANATA V; GRANT A; GRAS S; GRAY C; GRAY M; GREENHALGH RJS; GRETARSSON AM; GREVERIE C; GRIMALDI F; GROSSO R; GROTE H; GRUNEWALD S; GUENTHER M; GUIDI G; GUSTAFSON EK; GUSTAFSON R; HAGE B; HALLAM JM; HAMMER D; HAMMOND GD; HANNA C; HANSON J; HARMS J; HARRY GM; HARRY IW; HARSTAD ED; HAUGHIAN K; HAYAMA K; HEEFNER J; HEITMANN H; HELLO P; HENG IS; HEPTONSTALL A; HEWITSON M; HILD S; HIROSE E; HOAK D; HODGE KA; HOLT K; HOSKEN DJ; HOUGH J; HOYLAND D; HUET D; HUGHEY B; HUTTNER SH; INGRAM DR; ISOGAI T; ITO M; IVANOV A; JARANOWSKI P; JOHNSON B; JOHNSON WW; JONES DI; JONES G; JONES R; DE LA JORDANA LS; JU L; KALMUS P; KALOGERA V; KANDHASAMY S; KANNER J; KASPRZYK D; KATSAVOUNIDIS E; KAWABE K; KAWAMURA S; KAWAZOE F; KELLS W; KEPPEL DG; KHALAIDOVSKI A; KHALILI FY; KHAN R; KHAZANOV E; KING P; KISSEL JS; KLIMENKO S; KOKEYAMA K; KONDRASHOV V; KOPPARAPU R; KORANDA S; KOWALSKA I; KOZAK D; KRISHNAN B; KROLAK A; KUMAR R; KWEE P; LA PENNA P; LAM PK; LANDRY M; LANTZ B; LAZZARINI A; LEI H; LEI M; LEINDECKER N; LEONOR I; LEROY N; LETENDRE N; LI C; LIN H; LINDQUIST PE; LITTENBERG TB; LOCKERBIE NA; LODHIA D; LONGO M; LORENZINI M; LORIETTE V; LORMAND M; LOSURDO G; LU P; LUBINSKI M; LUCIANETTI A; LUCK H; MACHENSCHALK B; MACINNIS M; MACKOWSKI JM; MAGESWARAN M; MAILAND K; MAJORANA E; MANA N; MANDEL I; MANDIC V; MANTOVANI M; MARCHESONI F; MARION F; MARKA S; MARKA Z; MARKOSYAN A; MARKOWITZ J; MAROS E; MARQUE J; MARTELLI F; MARTIN IW; MARTIN RM; MARX JN; MASON K; MASSEROT A; MATICHARD F; MATONE L; MATZNER RA; MAVALVALA N; MCCARTHY R; MCCLELLAND DE; MCGUIRE SC; MCHUGH M; MCINTYRE G; MCKECHAN DJA; MCKENZIE K; MEHMET M; MELATOS A; MELISSINOS AC; MENDELL G; MENENDEZ DF; MENZINGER F; MERCER RA; MESHKOV S; MESSENGER C; MEYER MS; MICHEL C; MILANO L; MILLER J; MINELLI J; MINENKOVA Y; MINO Y; MITROFANOV VP; MITSELMAKHER G; MITTLEMAN R; MIYAKAWA O; MOE B; MOHAN M; MOHANTY SD; MOHAPATRA SRP; MOREAU J; MORENO G; MORGADO N; MORGIA A; MORIOKA T; MORS K; MOSCA S; MOSCATELLI V; MOSSAVI K; MOURS B; MOWLOWRY C; MUELLER G; MUHAMMAD D; ZUR MUHLEN H; MUKHERJEE S; MUKHOPADHYAY H; MULLAVEY A; MULLER EBHARDT H; MUNCH J; MURRAY PG; MYERS E; MYERS J; NASH T; NELSON J; NERI I; NEWTON G; NISHIZAWA A; NOCERA F; NUMATA K; OCHSNER E; O'DELL J; OGIN GH; O'REILLY B; O'SHAUGHNESSY R; OTTAWAY DJ; OTTENS RS; OVERMIER H; OWEN BJ; PAGLIAROLI G; PALOMBA C; PAN Y; PANKOW C; PAOLETTI F; PAPA MA; PARAMESHWARAIAH V; PARDI S; PASQUALETTI A; PASSAQUIETI R; PASSUELLO D; PATEL P; PEDRAZA M; PENN S; PERRECA A; PERSICHETTI G; PICHOT M; PIERGIOVANNI F; PIERRO V; PIETKA M; PINARD L; PINTO IM; PITKIN M; PLETSCH HJ; PLISSI MV; POGGIANI R; POSTIGLIONE F; PRATO M; PRINCIPE M; PRIX R; PRODI GA; PROKHOROV L; PUNCKEN O; PUNTURO M; PUPPO P; QUETSCHKE V; RAAB FJ; RABASTE O; RABELING DS; RADKINS H; RAFFAI P; RAICS Z; RAINER N; RAKHMANOV M; RAYMOND V; RE V; REED CM; REED T; REGIMBAU T; REHBEIN H; REID S; REITZE DH; RIESEN R; RILES K; RIVERA B; ROBERTS P; ROBERTSON NA; ROBINET F; ROBINSON C; ROBINSON EL; ROCCHI A; RODDY S; ROLLAND L; ROLLINS J; ROMANO JD; ROMANOAC R; ROMIE JH; ROSINSKA D; ROVER C; ROWAN S; RUDIGER A; RUGGI P; RUSSELL P; RYAN K; SAKATA S; SALEMI F; SANDBERG V; SANNIBALE V; SANTAMARIA L; SARAF S; SARIN P; SASSOLAS B; SATHYAPRAKASH BS; SATO S; SATTERTHWAITE M; SAULSON PR; SAVAGE R; SAVOV P; SCANLAN M; SCHILLING R; SCHNABEL R; SCHOFIELD R; SCHULZ B; SCHUTZ BF; SCHWINBERG P; SCOTT J; SCOTT SM; SEARLE AC; SEARS B; SEIFERT F; SELLERS D; SENGUPTA AS; SENTENAC D; SERGEEV A; SHAPIRO B; SHAWHAN P; SHOEMAKER DH; SIBLEY A; SIEMENS X; SIGG D; SINHA S; SINTES AM; SLAGMOLEN BJJ; SLUTSKY J; VAN DER SLUYS MV; SMITH JR; SMITH MR; SMITH ND; SOMIYA K; SORAZU B; STEIN A; STEIN LC; STEPLEWSKI S; STOCHINO A; STONE R; STRAIN KA; STRIGIN S; STROEER A; STURANI R; STUVER AL; SUMMERSCALES TZ; SUN KX; SUNG M; SUTTON PJ; SWINKELS B; SZOKOLY GP; TALUKDER D; TANG L; TANNER DB; TARABRIN SP; TAYLOR JR; TAYLOR R; TERENZI R; THACKER J; THORNE KA; THORNE KS; URING ATR; TOKMAKOV KV; TONCELLI A; TONELLI M; TORRES C; TORRIE C; TOURNEFIER E; TRAVASSO F; TRAYLOR G; TRIAS M; TRUMMER J; UGOLINI D; ULMEN J; URBANEK K; VAHLBRUCH H; VAJENTE G; VALLISNERI M; VAN DEN BRAND JFJ; VAN DER PUTTEN S; VASS S; VAULIN R; VAVOULIDIS M; VECCHIO A; VEDOVATO G; VAN VEGGEL AA; VEITCH J; VEITCH P; VELTKAMP C; VERKINDT D; VETRANO F; VICERE A; VILLAR A; VINETA JY; VOCCA H; VORVICK C; VYACHANIN SP; WALDMAN SJ; WALLACE L; WARD RL; WAS M; WEIDNER A; WEINERT M; WEINSTEIN AJ; WEISS R; WEN L; WEN S; WETTE K; WHELAN JT; WHITCOMB SE; WHITING BF; WILKINSON C; WILLEMS PA; WILLIAMS HR; WILLIAMS L; WILLKE B; WILMUT I; WINKELMANN L; WINKLER W; WIPF CC; WISEMAN AG; WOAN G; WOOLEY R; WORDEN J; WU W; YAKUSHIN I; YAMAMOTO H; YAN Z; YOSHIDA S; YVERT M; ZANOLIN M; ZHANG J; ZHANG L; ZHAO C; ZOTOV N; ZUCKER ME; ZWEIZIG J; BEGIN S; CORONGIU A; D'AMICO N; FREIRE PCC; HESSELS JWT; HOBBS GB; KRAMER M; LYNE AG; MANCHESTER RN; MARSHALL FE; MIDDLEDITCH J; POSSENTI A; RANSOM SM; STAIRS IH; STAPPERS B.; FRASCA, Sergio; RAPAGNANI, Piero; RICCI, Fulvio
Contributors:	Abbott, Bp; Abbott, R; Acernese, F; Adhikari, R; Ajith, P; Allen, B; Allen, G; Alshourbagy, M; Amin, R; Anderson, Sb; Anderson, Wg; Antonucci, F; Aoudia, S; Arain, Ma; Araya, M; Armandula, H; Armor, P; Arun, Kg; Aso, Y; Aston, S; Astonea, P; Aufmuth, P; Aulbert, C; Babak, S; Baker, P; Ballardin, G; Ballmer, S; Barker, C; Barker, D; Barone, F; Barr, B; Barriga, P; Barsotti, L; Barsuglia, M; Barton, Ma; Bartos, I; Bassiri, R; Bastarrika, M; Bauer, T; Behnke, B; Beker, M; Benacquista, M; Betzwieser, J; Beyersdorf, Pt; Bigotta, S; Bilenko, Ia; Billingsley, G; Birindelli, S; Biswas, R; Bizouard, Ma; Black, E; Blackburn, Jk; Blackburn, L; Blair, D; Bland, B; Boccara, C; Bodiya, Tp; Bogue, L; Bondub, F; Bonelli, L; Bork, R; Boschi, V; Bose, S; Bosi, L; Braccinia, S; Bradaschia, C; Brady, Pr; Braginsky, Vb; Brau, Je; Bridges, Do; Brillet, A; Brinkmann, M; Brisson, V; VAN DEN BROECK, C; Brooks, Af; Brown, Da; Brummit, A; Brunet, G; Budzynski, R; Bulik, T; Bullington, A; Bulten, Hj; Buonanno, A; Burmeister, O; Buskulic, D; Byer, Rl; Cadonati, L; Cagnoli, G; Calloni, E; Camp, Jb; Campagna, E; Cannizzo, J; Cannon, Kc; Canuel, B; Cao, J; Carbognani, F; Cardenas, L; Caride, S; Castaldi, G; Caudill, S
Publisher Information:	IOP PUBLISHING LTD
Publication Year:	2010
Collection:	Sapienza Università di Roma: CINECA IRIS
Subject Terms:	gravitational wave; pulsars: general
Description:	We present a search for gravitational waves from 116 known millisecond and young pulsars using data from the fifth science run of the LIGO detectors. For this search, ephemerides overlapping the run period were obtained for all pulsars using radio and X-ray observations. We demonstrate an updated search method that allows for small uncertainties in the pulsar phase parameters to be included in the search. We report no signal detection from any of the targets and therefore interpret our results as upper limits on the gravitational wave signal strength. The most interesting limits are those for young pulsars. We present updated limits on gravitational radiation from the Crab pulsar, where the measured limit is now a factor of 7 below the spin-down limit. This limits the power radiated via gravitational waves to be less than similar to 2% of the available spin-down power. For the X-ray pulsar J0537-6910 we reach the spin-down limit under the assumption that any gravitational wave signal from it stays phase locked to the X-ray pulses over timing glitches, and for pulsars J1913+1011 and J1952+3252 we are only a factor of a few above the spin-down limit. Of the recycled millisecond pulsars, several of themeasured upper limits are only about an order of magnitude above their spin-down limits. For these our best (lowest) upper limit on gravitational wave amplitude is 2.3 x 10(-26) for J1603-7202 and our best (lowest) limit on the inferred pulsar ellipticity is 7.0 x 10(-8) for J2124-3358.
Document Type:	article in journal/newspaper
Language:	English
Relation:	info:eu-repo/semantics/altIdentifier/wos/WOS:000275918500060; volume:713; issue:1; firstpage:671; lastpage:685; numberofpages:15; journal:THE ASTROPHYSICAL JOURNAL; http://hdl.handle.net/11573/225295; http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000275918500060&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a
DOI:	10.1088/0004-637x/713/1/671
Availability:	http://hdl.handle.net/11573/225295; https://doi.org/10.1088/0004-637x/713/1/671; http://gateway.webofknowledge.com/gateway/Gateway.cgi?GWVersion=2&SrcApp=PARTNER_APP&SrcAuth=LinksAMR&KeyUT=000275918500060&DestLinkType=FullRecord&DestApp=ALL_WOS&UsrCustomerID=0c7ff228ccbaaa74236f48834a34396a; http://www.scopus.com/inward/record.url?eid=2-s2.0-77950283283&partnerID=65&md5=3551de0ace9a0b0d2233cd7a8a29bda9
Accession Number:	edsbas.3DF0BDFE
Database:	BASE