J/ApJ/713/671ivo://CDS.VizieR/J/ApJ/713/671doi:10.26093/cds/vizier.17130671CDSAbbott B.P.Abbott R.Acernese F.Adhikari R.Ajith P.Allen B.,Allen G.Alshourbagy M.Amin R.S.Anderson S.B.Anderson W.G.,Antonucci F.Aoudia S.Arain M.A.Araya M.Armandula H.Armor P.,Arun K.G.Aso Y.Aston S.Astone 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 M.A.Bartos I.,Bassiri R.Bastarrika M.Bauer TH.S.Behnke B.Beker M.,Benacquista M.Betzwieser J.Beyersdorf P.T.Bigotta S.Bilenko I.A.,Billingsley G.Birindelli S.Biswas R.Bizouard M.A.Black E.,Blackburn J.K.Blackburn L.Blair D.Bland B.Boccara C.Bodiya T.P.,Bogue L.Bondu F.Bonelli L.Bork R.Boschi V.Bose S.Bosi L.,Braccini S.Bradaschia C.Brady P.R.Braginsky V.B.Brau J.E.,Bridges D.O.Brillet A.Brinkmann M.Brisson V.Van Den Broeck C.,Brooks A.F.Brown D.A.Brummit A.Brunet G.Budzynski R.Bulik T.,Bullington A.Bulten H.J.Buonanno A.Burmeister O.Buskulic D.,Byer R.L.Cadonati L.Cagnoli G.Calloni E.Camp J.B.Campagna E.,Cannizzo J.Cannon K.C.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 C.T.Y.Clark D.Clark J.,Clayton J.H.Cleva F.Coccia E.Cokelaer T.Colacino C.N.Colas J.,Colla A.Colombini M.Conte R.Cook D.Corbitt T.R.C.Corda C.,Cornish N.Corsi A.Coulon J.-P.Coward D.Coyne D.C.,Creighton J.D.E.Creighton T.D.Cruise A.M.Culter R.M.Cumming A.,Cunningham L.Cuoco E.Danilishin S.L.D'Antonio S.Danzmann K.,Dari A.Dattilo V.Daudert B.Davier M.Davies G.Daw E.J.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.Di Paolo Emilio M.,Di Virgilio A.Diaz M.Dietz A.Donovan F.Dooley K.L.Doomes E.E.,Drago M.Drever R.W.P.Dueck J.Duke I.Dumas J.-C.Dwyer J.G.,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 L.S.Fiori I.Flaminio R.Flasch K.,Foley S.Forrest C.Fotopoulos N.Fournier J.-D.Franc J.Franzen A.,Frasca S.Frasconi F.Frede M.Frei M.Frei Z.Freise A.Frey R.,Fricke T.Fritschel P.Frolov V.V.Fyffe M.Galdi V.Gammaitoni L.,Garofoli J.A.Garufi F.Gemme G.Genin E.Gennai A.Gholami I.,Giaime J.A.Giampanis S.Giardina K.D.Giazotto A.Goda K.Goetz E.,Goggin L.M.Gonzalez G.Gorodetsky M.L.Gossler S.Gouaty R.,Granata M.Granata V.Grant A.Gras S.Gray C.Gray M.,Greenhalgh R.J.S.Gretarsson A.M.Greverie C.Grimaldi F.Grosso R.,Grote H.Grunewald S.Guenther M.Guidi G.Gustafson E.K.,Gustafson R.Hage B.Hallam J.M.Hammer D.Hammond G.D.Hanna C.,Hanson J.Harms J.Harry G.M.Harry I.W.Harstad E.D.Haughian K.,Hayama K.Heefner J.Heitmann H.Hello P.Heng I.S.Heptonstall A.,Hewitson M.Hild S.Hirose E.Hoak D.Hodge K.A.Holt K.Hosken D.J.,Hough J.Hoyland D.Huet D.Hughey B.Huttner S.H.Ingram D.R.,Isogai T.Ito M.Ivanov A.Jaranowski P.Johnson B.Johnson W.W.,Jones D.I.Jones G.Jones R.Sancho de la Jordana L.Ju L.Kalmus P.,Kalogera V.Kandhasamy S.Kanner J.Kasprzyk D.Katsavounidis E.,Kawabe K.Kawamura S.Kawazoe F.Kells W.Keppel D.G.Khalaidovski A.,Khalili F.Y.Khan R.Khazanov E.King P.Kissel J.S.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 P.K.,Landry M.Lantz B.Lazzarini A.Lei H.Lei M.Leindecker N.,Leonor I.Leroy N.Letendre N.Li C.Lin H.Lindquist P.E.,Littenberg T.B.Lockerbie N.A.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 J.-M.Mageswaran M.,Mailand K.Majorana E.Man 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 I.W.Martin R.M.Marx J.N.,Mason K.Masserot A.Matichard F.Matone L.Matzner R.A.Mavalvala N.,McCarthy R.McClelland D.E.McGuire S.C.McHugh M.McIntyre G.,McKechan D.J.A.McKenzie K.Mehmet M.Melatos A.Melissinos A.C.,Mendell G.Menendez D.F.Menzinger F.Mercer R.A.Meshkov S.,Messenger C.Meyer M.S.Michel C.Milano L.Miller J.Minelli J.,Minenkov Y.Mino Y.Mitrofanov V.P.Mitselmakher G.Mittleman R.,Miyakawa O.Moe B.Mohan M.Mohanty S.D.Mohapatra S.R.P.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 P.G.Myers E.Myers J.Nash T.,Nelson J.Neri I.Newton G.Nishizawa A.Nocera F.Numata K.,Ochsner E.O'Dell J.Ogin G.H.O'Reilly B.O'Shaughnessy R.,Ottaway D.J.Ottens R.S.Overmier H.Owen B.J.Pagliaroli G.,Palomba C.Pan Y.Pankow C.Paoletti F.Papa M.A.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 I.M.Pitkin M.,Pletsch H.J.Plissi M.V.Poggiani R.Postiglione F.Prato M.,Principe M.Prix R.Prodi G.A.Prokhorov L.Puncken O.Punturo M.,Puppo P.Quetschke V.Raab F.J.Rabaste O.Rabeling D.S.Radkins H.,Raffai P.Raics Z.Rainer N.Rakhmanov M.Rapagnani P.Raymond V.,Re V.Reed C.M.Reed T.Regimbau T.Rehbein H.Reid S.Reitze D.H.,Ricci F.Riesen R.Riles K.Rivera B.Roberts P.Robertson N.A.,Robinet F.Robinson C.Robinson E.L.Rocchi A.Roddy S.Rolland L.,Rollins J.Romano J.D.Romano R.Romie J.H.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 B.S.Sato S.Satterthwaite M.Saulson P.R.Savage R.,Savov P.Scanlan M.Schilling R.Schnabel R.Schofield R.Schulz B.,Schutz B.F.Schwinberg P.Scott J.Scott S.M.Searle A.C.Sears B.,Seifert F.Sellers D.Sengupta A.S.Sentenac D.Sergeev A.Shapiro B.,Shawhan P.Shoemaker D.H.Sibley A.Siemens X.Sigg D.Sinha S.,Sintes A.M.Slagmolen B.J.J.Slutsky J.van der Sluys M.V.Smith J.R.,Smith M.R.Smith N.D.Somiya K.Sorazu B.Stein A.Stein L.C.,Steplewski S.Stochino A.Stone R.Strain K.A.Strigin S.Stroeer A.,Sturani R.Stuver A.L.Summerscales T.Z.Sun K.-X.Sung M.,Sutton P.J.Swinkels B.Szokoly G.P.Talukder D.Tang L.Tanner D.B.,Tarabrin S.P.Taylor J.R.Taylor R.Terenzi R.Thacker J.Thorne K.A.,Thorne K.S.Thuring A.Tokmakov K.V.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 J.F.J.van der Putten S.Vass S.Vaulin R.Vavoulidis M.,Vecchio A.Vedovato G.van Veggel A.A.Veitch J.Veitch P.,Veltkamp C.Verkindt D.Vetrano F.Vicere A.Villar A.Vinet J.-Y.,Vocca H.Vorvick C.Vyachanin S.P.Waldman S.J.Wallace L.Ward R.L.,Was M.Weidner A.Weinert M.Weinstein A.J.Weiss R.Wen L.Wen S.,Wette K.Whelan J.T.Whitcomb S.E.Whiting B.F.Wilkinson C.,Willems P.A.Williams H.R.Williams L.Willke B.Wilmut I.,Winkelmann L.Winkler W.Wipf C.C.Wiseman A.G.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 M.E.Zweizig J.,(the Ligo Scientific Collaboration The Virgo Collaboration)Begin S.,Corongiu A.D'Amico N.Freire P.C.C.Hessels J.W.T.Hobbs G.B.,Kramer M.Lyne A.G.Manchester R.N.Marshall F.E.Middleditch J.,Possenti A.Ransom S.M.Stairs I.H.Stappers B.2018-01-08T06:37:53Z2012-05-14T13:46:27ZCDS support team

CDS, Observatoire de Strasbourg, 11 rue de l'Universite, F-67000 Strasbourg, France

cds-question@unistra.frpulsarsradio-sourcesWe 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 ~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 the measured 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 2.3x10^-26^ for J1603-7202 and our best (lowest) limit on the inferred pulsar ellipticity is 7.0x10^-8^ for J2124-3358.2010ApJ...713..671Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/713/671CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/189 : Catalog of Pulsars (Taylor+ 1995)J/AZh/88/954 : Geometry of radio pulsar magnetospheres (Malov+, 2011)J/AZh/88/22 : Angles rotation/magnetic moment in pulsars (Malov+, 2011)J/other/PASA/27.64 : Parkes Radio Telescope pulsar timing (Weltevrede+, 2010)J/AZh/87/238 : Pulse profiles of radio pulsars at 102 and 111MHz (Malov+,J/AZh/84/685 : Scattering of pulsar radio emission (Kuz'min+, 2007)J/MNRAS/372/777 : Parkes Multibeam Pulsar Survey. VI. (Lorimer+, 2006)J/MNRAS/353/1311 : Long-term timing observations of 374 pulsars (Hobbs+, 2004)J/AZh/79/501 : Radio luminosities of normal + millisecond pulsars (Kuz'min,J/A+AS/147/195 : Pulsar spectra of radio emission (Maron+, 2000)J/A+A/339/123 : PSR J1012+5307 evolutionary tracks (Driebe+ 1998)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/713/671https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/713/671http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/713/671https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/713/671https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/713/671http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/713/671GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/713/671/table1 (Information on the non-glitching pulsars in our search, including the start and end times of the radio observations used in producing the parameter fits for our search, and upper limit results)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/713/671/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/713/671/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/713/671/table1?GETtext/xml+votable180.050000true5.959875-72.0753890.0055555555555555566/323 2411 4750 6051 9232 12875 12975 13018 13363 14413 18947 19994 20078 22154 23664 26824 27543 28751 28778 28870 28889 28905 28914 28970 29091 29180 29213 29466 29575 29636 29831 30334 30402 30619 30630 30696 30794 31228 33321 34034 37435 38133 39784 41258 42250 42841 42916 42955 44088 45897 47125 47168 47741 48193 49053https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/713/671?format=asciiRadiodefaultJ/ApJ/713/671/table1Information on the non-glitching pulsars in our search, including the start and end times of the radio observations used in producing the parameter fits for our search, and upper limit resultssdSpin-down limitphys.energydoublerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPSRPulsar identification (JHHMM+DDMMA; sometimes J1748+2446aa)meta.id;meta.maincharn_PSRPulsar pecularities (1)meta.notecharMJDstStart Modified Julian Date of the observationdtime.epochintMJDendEnd Modified Julian Date of the observationdtime.epochintnuSpin-frequency {nu}Hztime.periodfloatdnu/dtSpin-down rateHz/sphys.energydoublen_dnu/dt[a] corrected spin-down (1)meta.notecharDistDistance of pulsarkpcpos.distance;pos.heliocentricfloath0_95_Joint 95% upper limits on h_0_ (strain tensor amplitude)stat.fit.paramdoubleellEquatorial ellipticity {epsilon}=(Ixx-Iyy)/Izz (Izz = pulsar's principal moment of inertia)src.ellipticitydoubleh95/hsdRatio h^95%^_0_/h^sd^_0_ (h^sd^_0_: spin-down limit on strain tensor amplitude)stat.fit.paramfloatSimbadSimbad column added by the CDSmeta.refchar_RAPositions, from SIMBAD or ATNF database; the positions of pulsars in globular clusters are however frequently inaccurate (right ascension part)degpos.eq.ra;meta.main_DEPositions, from SIMBAD or ATNF database; the positions of pulsars in globular clusters are however frequently inaccurate (declination part)degpos.eq.dec;meta.main