J/ApJ/785/119ivo://CDS.VizieR/J/ApJ/785/119doi:10.26093/cds/vizier.17850119CDSAasi J.Abadie J.Abbott B.P.Abbott R.Abbott T.Abernathy M.R.,Accadia T.Acernese F.Adams C.Adams T.Adhikari R.X.Affeldt C.,Agathos M.Aggarwal N.Aguiar O.D.Ajith P.Allen B.Allocca A.,Ceron E.A.Amariutei D.Anderson R.A.Anderson S.B.Anderson W.G.,Arai K.Araya M.C.Arceneaux C.Areeda J.Ast S.Aston S.M.,Astone P.Aufmuth P.Aulbert C.Austin L.Aylott B.E.Babak S.,Baker P.T.Ballardin G.Ballmer S.W.Barayoga J.C.Barker D.,Barnum S.H.Barone F.Barr B.Barsotti L.Barsuglia M.Barton M.A.,Bartos I.Bassiri R.Basti A.Batch J.Bauchrowitz J.Bauer TH.S.,Bebronne M.Behnke B.Bejger M.Beker M.G.Bell A.S.Bell C.,Belopolski I.Bergmann G.Berliner J.M.Bersanetti D.Bertolini A.,Bessis D.Betzwieser J.Beyersdorf P.T.Bhadbhade T.Bilenko I.A.,Billingsley G.Birch J.Bitossi M.Bizouard M.A.Black E.,Blackburn J.K.Blackburn L.Blair D.Blom M.Bock O.Bodiya T.P.,Boer M.Bogan C.Bond C.Bondu F.Bonelli L.Bonnand R.Bork R.,Born M.Boschi V.Bose S.Bosi L.Bowers J.Bradaschia C.Brady P.R.,Braginsky V.B.Branchesi M.Brannen C.A.Brau J.E.Breyer J.,Briant T.Bridges D.O.Brillet A.Brinkmann M.Brisson V.Britzger M.,Brooks A.F.Brown D.A.Brown D.D.Bruckner F.Bulik T.Bulten H.J.,Buonanno A.Buskulic D.Buy C.Byer R.L.Cadonati L.Cagnoli G.,Calderon Bustillo J.Calloni E.Camp J.B.Campsie P.Cannon K.C.,Canuel B.Cao J.Capano C.D.Carbognani F.Carbone L.Caride S.,Castiglia A.Caudill S.Cavaglia M.Cavalier F.Cavalieri R.Cella G.,Cepeda C.Cesarini E.Chakraborty R.Chalermsongsak T.Chao S.,Charlton P.Chassande-Mottin E.Chen X.Chen Y.Chincarini A.,Chiummo A.Cho H.S.Chow J.Christensen N.Chu Q.Chua S.S.Y.,Chung S.Ciani G.Clara F.Clark D.E.Clark J.A.Cleva F.Coccia E.,Cohadon P.-F.Colla A.Colombini M.Constancio M.JRConte A.Conte R.,Cook D.Corbitt T.R.Cordier M.Cornish N.Corsi A.Costa C.A.,Coughlin M.W.Coulon J.-P.Countryman S.Couvares P.Coward D.M.,Cowart M.Coyne D.C.Craig K.Creighton J.D.E.Creighton T.D.,Crowder S.G.Cumming A.Cunningham L.Cuoco E.Dahl K.Dal Canton T.,Damjanic M.Danilishin S.L.D'Antonio S.Danzmann K.Dattilo V.,Daudert B.Daveloza H.Davier M.Davies G.S.Daw E.J.Day R.,Dayanga T.De Rosa R.Debreczeni G.Degallaix J.Del Pozzo W.,Deleeuw E.Deleglise S.Denker T.Dent T.Dereli H.Dergachev V.,Derosa R.Desalvo R.Dhurandhar S.Di Fiore L.Di Lieto A.,Di Palma I.Di Virgilio A.Diaz M.Dietz A.Dmitry K.Donovan F.,Dooley K.L.Doravari S.Drago M.Drever R.W.P.Driggers J.C.Du Z.,Dumas J.-C.Dwyer S.Eberle T.Edwards M.Effler A.Ehrens P.,Eichholz J.Eikenberry S.S.Endroczi G.Essick R.Etzel T.Evans K.,Evans M.Evans T.Factourovich M.Fafone V.Fairhurst S.Fang Q.,Farinon S.Farr B.Farr W.Favata M.Fazi D.Fehrmann H.Feldbaum D.,Ferrante I.Ferrini F.Fidecaro F.Finn L.S.Fiori I.Fisher R.,Flaminio R.Foley E.Foley S.Forsi E.Fotopoulos N.Fournier J.-D.,Franco S.Frasca S.Frasconi F.Frede M.Frei M.Frei Z.Freise A.,Frey R.Fricke T.T.Fritschel P.Frolov V.V.Fujimoto M.-K.Fulda P.,Fyffe M.Gair J.Gammaitoni L.Garcia J.Garufi F.Gehrels N.,Gemme G.Genin E.Gennai A.Gergely 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V.Kandhasamy S.Kang G.,Kanner J.B.Kasprzack M.Kasturi R.Katsavounidis E.Katzman W.,Kaufer H.Kaufman K.Kawabe K.Kawamura S.Kawazoe F.Kefelian F.,Keitel D.Kelley D.B.Kells W.Keppel D.G.Khalaidovski A.,Khalili F.Y.Khazanov E.A.Kim B.K.Kim C.Kim K.Kim N.Kim W.,Kim Y.-M.King E.J.King P.J.Kinzel D.L.Kissel J.S.Klimenko S.,Kline J.Koehlenbeck S.Kokeyama K.Kondrashov V.Koranda S.,Korth W.Z.Kowalska I.Kozak D.Kremin A.Kringel V.Krishnan B.,Krolak A.Kucharczyk C.Kudla S.Kuehn G.Kumar A.Kumar P.Kumar R.,Kurdyumov R.Kwee P.Landry M.Lantz B.Larson S.Lasky P.D.,Lawrie C.Lazzarini A.Le Roux A.Leaci P.Lebigot E.O.Lee C.-H.,Lee H.K.Lee H.M.Lee J.Leonardi M.Leong J.R.Leroy N.Letendre N.,Levine B.Lewis J.B.Lhuillier V.Li T.G.F.Lin A.C.Littenberg T.B.,Litvine V.Liu F.Liu H.Liu Y.Liu Z.Lloyd D.Lockerbie N.A.,Lockett V.Lodhia D.Loew K.Logue J.Lombardi A.L.Lorenzini M.,Loriette V.Lormand M.Losurdo G.Lough J.Luan J.Lubinski M.J.,Luck H.Lundgren A.P.Macarthur J.Macdonald E.Machenschalk B.,Macinnis M.Macleod D.M.Magana-sandoval F.Mageswaran M.Mailand K.,Majorana E.Maksimovic I.Malvezzi V.Man N.Manca G.M.Mandel I.,Mandic V.Mangano V.Mantovani M.Marchesoni F.Marion F.Marka S.,Marka Z.Markosyan A.Maros E.Marque J.Martelli F.Martin I.W.,Martin R.M.Martinelli L.Martynov D.Marx J.N.Mason K.Masserot A.,Massinger T.J.Matichard F.Matone L.Matzner R.A.Mavalvala N.,May G.Mazumder N.Mazzolo G.McCarthy R.McClelland D.E.,McGuire S.C.McIntyre G.McIver J.Meacher D.Meadors G.D.Mehmet M.,Meidam J.Meier T.Melatos A.Mendell G.Mercer R.A.Meshkov S.,Messenger C.Meyer M.S.Miao H.Michel C.Mikhailov E.E.Milano L.,Miller J.Minenkov Y.Mingarelli C.M.F.Mitra S.Mitrofanov V.P.,Mitselmakher G.Mittleman R.Moe B.Mohan M.Mohapatra S.R.P.,Mokler F.Moraru D.Moreno G.Morgado N.Mori T.Morriss S.R.,Mossavi K.Mours B.Mow-Lowry C.M.Mueller C.L.Mueller G.,Mukherjee S.Mullavey A.Munch J.Murphy D.Murray P.G.Mytidis A.,Nagy M.F.Nanda Kumar D.Nardecchia I.Nash T.Naticchioni L.,Nayak R.Necula V.Nelemans G.Neri I.Neri M.Newton G.Nguyen T.,Nishida E.Nishizawa A.Nitz A.Nocera F.Nolting D.Normandin M.E.,Nuttall L.K.Ochsner E.O'Dell J.Oelker E.Ogin G.H.Oh J.J.,Oh S.H.Ohme F.Oppermann P.O'Reilly B.Ortega Larcher W.,O'Shaughnessy R.Osthelder C.Ottaway D.J.Ottens R.S.Ou J.,Overmier H.Owen B.J.Padilla C.Pai A.Palomba C.Pan Y.Pankow C.,Paoletti F.Paoletti R.Papa M.A.Paris H.Pasqualetti A.,Passaquieti R.Passuello D.Pedraza M.Peiris P.Penn S.Perreca A.,Phelps M.Pichot M.Pickenpack M.Piergiovanni F.Pierro V.Pinard L.,Pindor B.Pinto I.M.Pitkin M.Poeld J.Poggiani R.Poole V.Poux C.,Predoi V.Prestegard T.Price L.R.Prijatelj M.Principe M.,Privitera S.Prix R.Prodi G.A.Prokhorov L.Puncken O.Punturo M.,Puppo P.Quetschke V.Quintero E.Quitzow-James R.Raab F.J.,Rabeling D.S.Racz I.Radkins H.Raffai P.Raja S.Rajalakshmi G.,Rakhmanov M.Ramet C.Rapagnani P.Raymond V.Re V.Reed C.M.,Reed T.Regimbau T.Reid S.Reitze D.H.Ricci F.Riesen R.Riles K.,Robertson N.A.Robinet F.Rocchi A.Roddy S.Rodriguez C.Rodruck M.,Roever C.Rolland L.Rollins J.G.Romano 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M.P.,Thomas M.Thomas P.Thorne K.A.Thorne K.S.Thrane E.Tiwari V.,Tokmakov K.V.Tomlinson C.Toncelli A.Tonelli M.Torre O.,Torres C.V.Torrie C.I.Travasso F.Traylor G.Tse M.Ugolini D.,Unnikrishnan C.S.Vahlbruch H.Vajente G.Vallisneri M.,van den Brand J.F.J.Van Den Broeck C.van der Putten S.,van der Sluys M.V.van Heijningen J.van Veggel A.A.Vass S.Vasuth M.,Vaulin R.Vecchio A.Vedovato G.Veitch J.Veitch P.J.,Venkateswara K.Verkindt D.Verma S.Vetrano F.Vicere A.,Vincent-Finley R.Vinet J.-Y.Vitale S.Vlcek B.Vo T.Vocca H.,Vorvick C.Vousden W.D.Vrinceanu D.Vyachanin S.P.Wade A.Wade L.,Wade M.Waldman S.J.Walker M.Wallace L.Wan Y.Wang J.Wang M.,Wang X.Wanner A.Ward R.L.Was M.Weaver B.Wei L.-W.Weinert M.,Weinstein A.J.Weiss R.Welborn T.Wen L.Wessels P.West M.,Westphal T.Wette K.Whelan J.T.Whitcomb S.E.White D.J.,Whiting B.F.Wibowo S.Wiesner K.Wilkinson C.Williams L.,Williams R.Williams T.Willis J.L.Willke B.Wimmer M.Winkelmann L.,Winkler W.Wipf C.C.Wittel H.Woan G.Worden J.Yablon J.,Yakushin I.Yamamoto H.Yancey C.C.Yang H.Yeaton-Massey D.,Yoshida S.Yum H.Yvert M.Zadrozny A.Zanolin M.Zendri J.-P.,Zhang F.Zhang L.Zhao C.Zhu H.Zhu X.J.Zotov N.Zucker M.E.,Zweizig J.Buchner S.Cognard I.Corongiu A.D'Amico N.Espinoza C.M.,Freire P.C.C.Gotthelf E.V.Guillemot L.Hessels J.W.T.Hobbs G.B.,Kramer M.Lyne A.G.Marshall F.E.Possenti A.Ransom S.M.Ray P.S.,Roy J.Stappers B.W.(the Virgo Collaboration),(the LIGO Scientific Collaboration)2017-12-11T07:42:42Z2017-06-27T07:32:39ZCDS support team

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

cds-question@unistra.frpulsarsstellar-distanceWe present the results of searches for gravitational waves from a large selection of pulsars using data from the most recent science runs (S6, VSR2 and VSR4) of the initial generation of interferometric gravitational wave detectors LIGO (Laser Interferometric Gravitational-wave Observatory) and Virgo. We do not see evidence for gravitational wave emission from any of the targeted sources but produce upper limits on the emission amplitude. We highlight the results from seven young pulsars with large spin-down luminosities. We reach within a factor of five of the canonical spin-down limit for all seven of these, whilst for the Crab and Vela pulsars we further surpass their spin-down limits. We present new or updated limits for 172 other pulsars (including both young and millisecond pulsars). Now that the detectors are undergoing major upgrades, and, for completeness, we bring together all of the most up-to-date results from all pulsars searched for during the operations of the first-generation LIGO, Virgo and GEO600 detectors. This gives a total of 195 pulsars including the most recent results described in this paper.2014ApJ...785..119Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/785/119CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toVII/189 : Catalog of Pulsars (Taylor+ 1995)J/ApJ/713/671 : Gravitational waves from pulsars (Abbott+, 2010)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/785/119https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/785/119http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/785/119https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/785/119https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/785/119http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/785/119GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/785/119/table7 (Limits on the Gravitational Wave Amplitude for Known Pulsars with f_gw_>40 Hz)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/785/119/table7?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/785/119/table7?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/785/119/table7?GETtext/xml+votable180.050000true5.8203759.390050.0055555555555555566/323 1684 2411 3894 4750 6051 8458 8788 9232 9436 9459 11287 12871 12875 12958 12975 13018 13050 13363 13465 13750 14219 14413 17955 18153 18947 19535 19994 20078 20552 20896 22154 23664 24564 25065 26532 26555 26824 27049 27543 28732 28751 28778 28829 28870 28889 28892 28905 28914 28924 28970 29091 29180 29208 29213 29287 29402 29466 29575 29593 29636 29831 29920 30193 30321 30334 30402 30566 30630 30653 30696 30794 31101 31228 31417 31976 32018 32160 32459 33321 34034 37161 37435 38133 39784 39996 41258 41275 41768 42240 42250 42841 42916 42955 44088 44356 45897 46237 47125 47168 47741 48193 48434 48882 49053https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/785/119?format=asciiRadiodefaultJ/ApJ/785/119/table7Limits on the Gravitational Wave Amplitude for Known Pulsars with f_gw_>40 HzrecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintIDPulsar identifier (PSR JHHMM+DDMMA in Simbad)meta.id;meta.maincharn_ID[defg] Note on ID (1)meta.notecharfrotRotational frequencyHztime.periodfloatfgwGravitational wave low-frequencyHztime.periodfloatFrotRotational frequency derivativeHz/stime.perioddoubleDistDistance to the sourcekpcpos.distance;pos.heliocentricfloatn_Dist[c] Note on Dist (2)meta.notecharhsdSpin-down gravitational wave amplitude limitsrc.var.amplitudedoublen_hsd[ab] Note on hsd (3)meta.notecharPriorh95? The prior 95% upper limit on the gravitational wave amplitudesrc.var.amplitudedoublenullableS6/VSR24-h95? The 95% upper limit on the gravitational wave amplitude from S6/VSR2,4src.var.amplitudedoublenullableepsilonFiducial equatorial ellipticitysrc.ellipticitydoubleQ22Mass quadrupole momentkg.m**-2stat.variancedoubleh0Ratio of the limit to the spin-down limitstat.fit.omcfloatSimbadSimbad column added by the CDSmeta.ref.urlchar_RARight Ascension (J2000) from SIMBAD (not part of the original data)degpos.eq.ra;meta.main_DEDeclination (J2000) from SIMBAD (not part of the original data)degpos.eq.dec;meta.main