J/ApJ/879/10ivo://CDS.VizieR/J/ApJ/879/10doi:10.26093/cds/vizier.18790010CDSAbbott B.P.Abbott R.Abbott T.D.Abraham S.Acernese F.Ackley K.,Adams C.Adhikari R.X.Adya V.B.Affeldt C.Agathos M.Agatsuma K.,Aggarwal N.Aguiar O.D.Aiello L.Ain A.Ajith P.Allen G.Allocca A.,Aloy M.A.Altin P.A.Amato A.Ananyeva A.Anderson S.B.Anderson W.G.,Angelova S.V.Antier S.Appert S.Arai K.Araya M.C.Areeda J.S.,Arene M.Arnaud N.Ascenzi S.Ashton G.Aston S.M.Astone P.Aubin F.,Aufmuth P.AultONeal K.Austin C.Avendano V.Avila-Alvarez A.,Babak S.Bacon P.Badaracco F.Bader M.K.M.Bae S.Bailes M.,Baker P.T.Baldaccini F.Ballardin G.Ballmer S.W.Banagiri S.,Barayoga J.C.Barclay S.E.Barish B.C.Barker D.Barkett K.Barnum S.,Barone F.Barr B.Barsotti L.Barsuglia M.Barta D.Bartlett J.,Bartos I.Bassiri R.Basti A.Bawaj M.Bayley J.C.Bazzan M.Becsy B.,Bejger M.Belahcene I.Bell A.S.Beniwal D.Berger B.K.Bergmann G.,Bernuzzi S.Bero J.J.Berry C.P.L.Bersanetti D.Bertolini A.,Betzwieser J.Bhandare R.Bidler J.Bilenko I.A.Bilgili S.A.,Billingsley G.Birch J.Birney R.Birnholtz O.Biscans S.,Biscoveanu S.Bisht A.Bitossi M.Bizouard M.A.Blackburn J.K.,Blair C.D.Blair D.G.Blair R.M.Bloemen S.Bode N.Boer M.,Boetzel Y.Bogaert G.Bondu F.Bonilla E.Bonnand R.Booker P.,Boom B.A.Booth C.D.Bork R.Boschi V.Bose S.Bossie K.Bossilkov V.,Bosveld J.Bouffanais Y.Bozzi A.Bradaschia C.Brady P.R.Bramley A.,Branchesi M.Brau J.E.Briant T.Briggs J.H.Brighenti F.Brillet A.,Brinkmann M.Brisson V.Brockill P.Brooks A.F.Brown D.D.Brunett S.,Buikema A.Bulik T.Bulten H.J.Buonanno A.Buskulic D.Buy C.,Byer R.L.Cabero M.Cadonati L.Cagnoli G.Cahillane C.Bustillo J.C.,Callister T.A.Calloni E.Camp J.B.Campbell W.A.Canepa M.,Cannon K.C.Cao H.Cao J.Capocasa E.Carbognani F.Caride S.,Carney M.F.Carullo G.Diaz J.C.Casentini C.Caudill S.Cavaglia M.,Cavalier F.Cavalieri R.Cella G.Cerda-Duran P.Cerretani G.,Cesarini E.Chaibi O.Chakravarti K.Chamberlin S.J.Chan M.Chao S.,Charlton P.Chase E.A.Chassande-Mottin E.Chatterjee D.Chaturvedi M.,Cheeseboro B.D.Chen H.Y.Chen X.Chen Y.Cheng H.-P.Cheong C.K.,Chia H.Y.Chincarini A.Chiummo A.Cho G.Cho H.S.Cho M.,Christensen N.Chu Q.Chua S.Chung K.W.Chung S.Ciani G.,Ciobanu A.A.Ciolfi R.Cipriano F.Cirone A.Clara F.Clark J.A.,Clearwater P.Cleva F.Cocchieri C.Coccia E.Cohadon P.-F.Cohen D.,Colgan R.Colleoni M.Collette C.G.Collins C.Cominsky L.R.,Constancio M.Conti L.Cooper S.J.Corban P.Corbitt T.R.Cordero-Carrion I.Corley K.R.Cornish N.Corsi A.Cortese S.Costa C.A.,Cotesta R.Coughlin M.W.Coughlin S.B.Coulon J.-P.Countryman S.T.,Couvares P.Covas P.B.Cowan E.E.Coward D.M.Cowart M.J.Coyne D.C.,Coyne R.Creighton J.D.E.Creighton T.D.Cripe J.Croquette M.,Crowder S.G.Cullen T.J.Cumming A.Cunningham L.Cuoco E.Canton T.D.,Dalya G.Danilishin S.L.D'Antonio S.Danzmann K.Dasgupta A.Da SilvaCosta C.F.Datrier L.E.H.Dattilo V.Dave I.Davier M.Davis D.,Daw E.J.DeBra D.Deenadayalan M.Degallaix J.De Laurentis M.,Deleglise S.Del Pozzo W.DeMarchi L.M.Demos N.Dent T.De Pietri R.,Derby J.De Rosa R.De Rossi C.DeSalvo R.de Varona O.Dhurandhar S.,Diaz M.C.Dietrich T.Di Fiore L.Di Giovanni M.Di Girolamo T.DiLieto A.Ding B.Di Pace S.Di Palma I.Di Renzo F.Dmitriev A.,Doctor Z.Donovan F.Dooley K.L.Doravari S.Dorrington I.Downes T.P.,Drago M.Driggers J.C.Du Z.Ducoin J.-G.Dupej P.Dwyer S.E.,Easter P.J.Edo T.B.Edwards M.C.Effler A.Ehrens P.Eichholz J.,Eikenberry S.S.Eisenmann M.Eisenstein R.A.Essick R.C.Estelles H.,Estevez D.Etienne Z.B.Etzel T.Evans M.Evans T.M.Fafone V.,Fair H.Fairhurst S.Fan X.Farinon S.Farr B.Farr W.M.Fauchon-Jones E.J.Favata M.Fays M.Fazio M.Fee C.Feicht J.Fejer M.M.,Feng F.Fernandez-Galiana A.Ferrante I.Ferreira E.C.Ferreira T.A.,Ferrini F.Fidecaro F.Fiori I.Fiorucci D.Fishbach M.Fisher R.P.,Fishner J.M.Fitz-Axen M.Flaminio R.Fletcher M.Flynn E.Fong H.,Font J.A.Forsyth P.W.F.Fournier J.-D.Frasca S.Frasconi F.Frei Z.,Freise A.Frey R.Frey V.Fritschel P.Frolov V.V.Fulda P.Fyffe M.,Gabbard H.A.Gadre B.U.Gaebel S.M.Gair J.R.Gammaitoni L.,Ganija M.R.Gaonkar S.G.Garcia A.Garcia-Quiros C.Garufi F.,Gateley B.Gaudio S.Gaur G.Gayathri V.Gemme G.Genin E.Gennai A.,George D.George J.Gergely L.Germain V.Ghonge S.Ghosh A.Ghosh A.,Ghosh S.Giacomazzo B.Giaime J.A.Giardina K.D.Giazotto A.Gill K.,Giordano G.Glover L.Godwin P.Goetz E.Goetz R.Goncharov B.,Gonzalez G.Castro J.M.G.Gopakumar A.Gorodetsky M.L.Gossan S.E.,Gosselin M.Gouaty R.Grado A.Graef C.Granata M.Grant A.Gras S.,Grassia P.Gray C.Gray R.Greco G.Green A.C.Green R.,Gretarsson E.M.Groot P.Grote H.Grunewald S.Gruning P.Guidi G.M.,Gulati H.K.Guo Y.Gupta A.Gupta M.K.Gustafson E.K.Gustafson R.,Haegel L.Halim O.Hall B.R.Hall E.D.Hamilton E.Z.Hammond G.,Haney M.Hanke M.M.Hanks J.Hanna C.Hannam M.D.Hannuksela O.A.,Hanson J.Hardwick T.Haris K.Harms J.Harry G.M.Harry I.W.,Haster C.-J.Haughian K.Hayes F.J.Healy J.Heidmann A.Heintze M.C.,Heitmann H.Hello P.Hemming G.Hendry M.Heng I.S.Hennig J.,Heptonstall A.W.Vivanco F.H.Heurs M.Hild S.Hinderer T.Ho W.C.G.,Hoak D.Hochheim S.Hofman D.Holgado A.M.Holland N.A.Holt K.,Holz D.E.Hopkins P.Horst C.Hough J.Howell E.J.Hoy C.G.Hreibi A.,Huerta E.A.Huet D.Hughey B.Hulko M.Husa S.Huttner S.H.Huynh-Dinh T.Idzkowski B.Iess A.Ingram C.Inta R.Intini G.Irwin B.,Isa H.N.Isac J.-M.Isi M.Iyer B.R.Izumi K.Jacqmin T.Jadhav S.J.,Jani K.Janthalur N.N.Jaranowski P.Jenkins A.C.Jiang J.,Johnson D.S.Jones A.W.Jones D.I.Jones R.Jonker R.J.G.Ju L.,Junker J.Kalaghatgi C.V.Kalogera V.Kamai B.Kandhasamy S.Kang G.,Kanner J.B.Kapadia S.J.Karki S.Karvinen K.S.Kashyap R.,Kasprzack M.Katsanevas S.Katsavounidis E.Katzman W.Kaufer S.,Kawabe K.Keerthana N.V.Kefelian F.Keitel D.Kennedy R.Key J.S.,Khalili F.Y.Khan H.Khan I.Khan S.Khan Z.Khazanov E.A.,Khursheed M.Kijbunchoo N.Kim C.Kim J.C.Kim K.Kim W.Kim W.S.,Kim Y.-M.Kimball C.King E.J.King P.J.Kinley-Hanlon M.Kirchhoff R.,Kissel J.S.Kleybolte L.Klika J.H.Klimenko S.Knowles T.D.Koch P.,Koehlenbeck S.M.Koekoek G.Koley S.Kondrashov V.Kontos A.Koper N.,Korobko M.Korth W.Z.Kowalska I.Kozak D.B.Kringel V.Krishnendu N.,Krolak A.Kuehn G.Kumar A.Kumar P.Kumar R.Kumar S.Kuo L.,Kutynia A.Kwang S.Lackey B.D.Lai K.H.Lam T.L.Landry M.Lane B.B.,Lang R.N.Lange J.Lantz B.Lanza R.K.Lartaux-Vollard A.Lasky P.D.,Laxen M.Lazzarini A.Lazzaro C.Leaci P.Leavey S.Lecoeuche Y.K.,Lee C.H.Lee H.K.Lee H.M.Lee H.W.Lee J.Lee K.Lehmann J.,Lenon A.Leroy N.Letendre N.Levin Y.Li J.Li K.J.L.Li T.G.F.,Li X.Lin F.Linde F.Linker S.D.Littenberg T.B.Liu J.Liu X.,Lo R.K.L.Lockerbie N.A.London L.T.Longo A.Lorenzini M.Loriette V.,Lormand M.Losurdo G.Lough J.D.Lousto C.O.Lovelace G.Lower M.E.,Luck H.Lumaca D.Lundgren A.P.Lynch R.Ma Y.Macas R.Macfoy S.,MacInnis M.Macleod D.M.Macquet A.Magana-Sandoval F.MaganaZertuche L.Magee R.M.Majorana E.Maksimovic I.Malik A.Man N.,Mandic V.Mangano V.Mansell G.L.Manske M.Mantovani M.Marchesoni F.,Marion F.Marka S.Marka Z.Markakis C.Markosyan A.S.Markowitz A.,Maros E.Marquina A.Marsat S.Martelli F.Martin I.W.Martin R.M.,Martynov D.V.Mason K.Massera E.Masserot A.Massinger T.J.Masso-Reid M.Mastrogiovanni S.Matas A.Matichard F.Matone L.Mavalvala N.,Mazumder N.McCann J.J.McCarthy R.McClelland D.E.McCormick S.,McCuller L.McGuire S.C.McIver J.McManus D.J.McRae T.,McWilliams S.T.Meacher D.Meadors G.D.Mehmet M.Mehta A.K.Meidam J.,Melatos A.Mendell G.Mercer R.A.Mereni L.Merilh E.L.Merzougui M.,Meshkov S.Messenger C.Messick C.Metzdorff R.Meyers P.M.Miao H.,Michel C.Middleton H.Mikhailov E.E.Milano L.Miller A.L.Miller A.,Millhouse M.Mills J.C.Milovich-Goff M.C.Minazzoli O.Minenkov Y.,Mishkin A.Mishra C.Mistry T.Mitra S.Mitrofanov V.P.,Mitselmakher G.Mittleman R.Mo G.Moffa D.Mogushi K.,Mohapatra S.R.P.Montani M.Moore C.J.Moraru D.Moreno G.Morisaki S.,Mours B.Mow-Lowry C.M.Mukherjee A.Mukherjee D.Mukherjee S.,Mukund N.Mullavey A.Munch J.Muniz E.A.Muratore M.Murray P.G.,Nagar A.Nardecchia I.Naticchioni L.Nayak R.K.Neilson J.,Nelemans G.Nelson T.J.N.Nery M.Neunzert A.Ng K.Y.Ng S.Nguyen P.,Nichols D.Nissanke S.Nocera F.North C.Nuttall L.K.,Obergaulinger M.Oberling J.O'Brien B.D.O'Dea G.D.Ogin G.H.Oh J.J.,Oh S.H.Ohme F.Ohta H.Okada M.A.Oliver M.Oppermann P.Oram R.J.,O'Reilly B.Ormiston R.G.Ortega L.F.O'Shaughnessy R.Ossokine S.,Ottaway D.J.Overmier H.Owen B.J.Pace A.E.Pagano G.Page M.A.,Pai A.Pai S.A.Palamos J.R.Palashov O.Palomba C.Pal-Singh A.,Pan H.-W.Pang B.Pang P.T.H.Pankow C.Pannarale F.Pant B.C.,Paoletti F.Paoli A.Parida A.Parker W.Pascucci D.Pasqualetti A.,Passaquieti R.Passuello D.Patil M.Patricelli B.Pearlstone B.L.,Pedersen C.Pedraza M.Pedurand R.Pele A.Penn S.Perez C.J.,Perreca A.Pfeiffer H.P.Phelps M.Phukon K.S.Piccinni O.J.Pichot M.,Piergiovanni F.Pillant G.Pinard L.Pirello M.Pitkin M.Poggiani R.,Pong D.Y.T.Ponrathnam S.Popolizio P.Porter E.K.Powell J.,Prajapati A.K.Prasad J.Prasai K.Prasanna R.Pratten G.,Prestegard T.Privitera S.Prodi G.A.Prokhorov L.G.Puncken O.,Punturo M.Puppo P.Purrer M.Qi H.Quetschke V.Quinonez P.J.,Quintero E.A.Quitzow-James R.Raab F.J.Radkins H.Radulescu N.,Raffai P.Raja S.Rajan C.Rajbhandari B.Rakhmanov M.Ramirez K.E.,Ramos-Buades A.Rana J.Rao K.Rapagnani P.Raymond V.Razzano M.,Read J.Regimbau T.Rei L.Reid S.Reitze D.H.Ren W.Ricci F.,Richardson C.J.Richardson J.W.Ricker P.M.Riles K.Rizzo M.,Robertson N.A.Robie R.Robinet F.Rocchi A.Rolland L.Rollins J.G.,Roma V.J.Romanelli M.Romano R.Romel C.L.Romie J.H.Rose K.,Rosinska D.Rosofsky S.G.Ross M.P.Rowan S.Rudiger A.Ruggi P.,Rutins G.Ryan K.Sachdev S.Sadecki T.Sakellariadou M.Salconi L.,Saleem M.Samajdar A.Sammut L.Sanchez E.J.Sanchez L.E.Sanchis-Gual N.Sandberg V.Sanders J.R.Santiago K.A.Sarin N.Sassolas B.,Saulson P.R.Sauter O.Savage R.L.Schale P.Scheel M.Scheuer J.,Schmidt P.Schnabel R.Schofield R.M.S.Schonbeck A.Schreiber E.,Schulte B.W.Schutz B.F.Schwalbe S.G.Scott J.Scott S.M.Seidel E.,Sellers D.Sengupta A.S.Sennett N.Sentenac D.Sequino V.Sergeev A.,Setyawati Y.Shaddock D.A.Shaffer T.Shahriar M.S.Shaner M.B.,Shao L.Sharma P.Shawhan P.Shen H.Shink R.Shoemaker D.H.,Shoemaker D.M.ShyamSundar S.Siellez K.Sieniawska M.Sigg D.,Silva A.D.Singer L.P.Singh N.Singhal A.Sintes A.M.,Sitmukhambetov S.Skliris 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der Schaaf L.vanVeggel A.A.Vardaro M.Varma V.Vass S.Vasuth M.Vecchio A.,Vedovato G.Veitch J.Veitch P.J.Venkateswara K.Venugopalan G.,Verkindt D.Vetrano F.Vicere A.Viets A.D.Vine D.J.Vinet J.-Y.,Vitale S.Vo T.Vocca H.Vorvick C.Vyatchanin S.P.Wade A.R.,Wade L.E.Wade M.Walet R.Walker M.Wallace L.Walsh S.Wang G.,Wang H.Wang J.Z.Wang W.H.Wang Y.F.Ward R.L.Warden Z.A.Warner J.,Was M.Watchi J.Weaver B.Wei L.-W.Weinert M.Weinstein A.J.,Weiss R.Wellmann F.Wen L.Wessel E.K.Wessels P.Westhouse J.W.,Wette K.Whelan J.T.Whiting B.F.Whittle C.Wilken D.M.Williams D.,Williamson A.R.Willis J.L.Willke B.Wimmer M.H.Winkler W.Wipf C.C.,Wittel H.Woan G.Woehler J.Wofford J.K.Worden J.Wright J.L.,Wu D.S.Wysocki D.M.Xiao L.Yamamoto H.Yancey C.C.Yang L.Yap M.J.,Yazback M.Yeeles D.W.Yu H.Yu H.Yuen S.H.R.Yvert M.Zadrozny A.K.,Zanolin M.Zelenova T.Zendri J.-P.Zevin M.Zhang J.Zhang L.,Zhang T.Zhao C.Zhou M.Zhou Z.Zhu X.J.Zucker M.E.Zweizig J.,Arzoumanian Z.Bogdanov S.Cognard I.Corongiu A.Enoto T.Freire P.,Gendreau K.C.Guillemot L.Harding A.K.Jankowski F.Keith M.J.,Kerr M.Lyne A.Palfreyman J.Possenti A.Ridolfi A.Stappers B.,Theureau G.Weltervrede P.2021-09-10T13:34:32Z2021-01-18T12:17:46ZCDS support team

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

cds-question@unistra.frpulsarsgravitational-wavesstellar-distanceWe present a search for gravitational waves from 221 pulsars with rotation frequencies >~10Hz. We use advanced LIGO data from its first and second observing runs spanning 2015-2017, which provides the highest-sensitivity gravitational-wave data so far obtained. In this search we target emission from both the l=m=2 mass quadrupole mode, with a frequency at twice that of the pulsar's rotation, and the l=2, m=1 mode, with a frequency at the pulsar rotation frequency. The search finds no evidence for gravitational-wave emission from any pulsar at either frequency. For the l=m=2 mode search, we provide updated upper limits on the gravitational-wave amplitude, mass quadrupole moment, and fiducial ellipticity for 167 pulsars, and the first such limits for a further 55. For 20 young pulsars these results give limits that are below those inferred from the pulsars' spin-down. For the Crab and Vela pulsars our results constrain gravitational-wave emission to account for less than 0.017% and 0.18% of the spin-down luminosity, respectively. For the recycled millisecond pulsar J0711-6830 our limits are only a factor of 1.3 above the spin-down limit, assuming the canonical value of 10^38^kg.m^2^ for the star's moment of inertia, and imply a gravitational-wave-derived upper limit on the star's ellipticity of 1.2x10^-8^. We also place new limits on the emission amplitude at the rotation frequency of the pulsars.2019ApJ...879...10Ahttps://cdsarc.cds.unistra.fr/viz-bin/cat/J/ApJ/879/10CatalogResearchIsServedByTAP VizieR generic serviceIsServedByConesearch servicerelated-toB/psr : ATNF Pulsar Catalogue (Manchester+, 2005)J/MNRAS/353/1311 : Long-term timing observations of 374 pulsars (Hobbs+, 2004)J/ApJ/602/264 : Proper motions & radial velocities in M15 (McNamara+, 2004)J/AJ/133/1287 : JHK photom. of 24 Gal. globular clusters (Valenti+, 2007)J/ApJ/713/671 : Gravitational waves from pulsars (Abbott+, 2010)J/MNRAS/402/1729 : JHK photometry of 36 Gal. globular clusters (Valenti+ 2010)J/MNRAS/414/1679 : 315 glitches in the rotation of pulsars (Espinoza+, 2011)J/ApJ/763/80 : GBT 350MHz survey. I. 13 new pulsars (Boyles+, 2013)J/ApJ/785/119 : Gravitational waves from known pulsars (Aasi+, 2014)J/MNRAS/458/3341 : 42 ms pulsars high-precision timing (Desvignes+, 2016)J/ApJ/839/12 : Gravitational waves search from known PSR (Abbott+, 2017)J/ApJS/247/33 : Fermi LAT fourth source catalog (4FGL) (Abdollahi+, 2020)https://cds.unistra.fr/vizier-org/licences_vizier.htmlhttps://vizier.cds.unistra.fr/viz-bin/VizieR-2?-source=J/ApJ/879/10https://vizier.iucaa.in/viz-bin/VizieR-2?-source=J/ApJ/879/10http://vizieridia.saao.ac.za/viz-bin/VizieR-2?-source=J/ApJ/879/10https://vizier.cds.unistra.fr/viz-bin/votable?-source=J/ApJ/879/10https://vizier.iucaa.in/viz-bin/votable?-source=J/ApJ/879/10http://vizieridia.saao.ac.za/viz-bin/votable?-source=J/ApJ/879/10GETtext/xml+votablehttps://tapvizier.cds.unistra.fr/TAPVizieR/tapCone search capability for table J/ApJ/879/10/table1 (Upper limits of gravitational wave amplitude and other derived quantities from erratum published in 2020, ApJ, 899, 170)https://vizier.cds.unistra.fr/viz-bin/conesearch/J/ApJ/879/10/table1?https://vizier.iucaa.in/viz-bin/conesearch/J/ApJ/879/10/table1?http://vizieridia.saao.ac.za/viz-bin/conesearch/J/ApJ/879/10/table1?GETtext/xml+votable180.050000true5.8203759.390050.0055555555555555566/323 813 1684 1791 2396 2411 2857 2943 3441 3681 3894 4750 6051 7047 7049 7670 7786 8022 8458 8788 9232 9459 9965 10048 11287 11351 12188 12405 12446 12490 12871 12875 12958 12971 12975 12986 13018 13050 13191 13291 13363 13465 13750 14357 14375 14401 14413 14454 14545 15030 15396 15644 15653 17341 17955 18153 18520 18702 18947 19025 19249 19306 19419 19535 19994 20078 20552 20817 20896 22154 23258 23664 23794 23983 24185 24193 24384 24564 25065 25795 26203 26532 26555 26824 26993 27049 27543 28732 28751 28819 28829 28838 28870 28873 28881 28889 28892 28897 28905 28914 28920 28924 28970 29002 29091 29097 29139 29180 29208 29213 29271 29281 29325 29402 29466 29471 29505 29511 29529 29531 29532 29534 29575 29636 29831 29920 30071 30193 30219 30241 30301 30314 30331 30334 30337 30402 30404 30416 30420 30421 30566 30597 30619 30630 30653 30696 30702 30710 30715 30716 30794 31101 31228 31239 31902 31976 32018 32113 32160 33457 34034 36893 37161 37183 37341 37346 37435 37721 37923 37930 37940 38361 38488 39235 39784 39996 40345 41217 41258 41681 41685 41758 41804 41937 41964 42173 42176 42209 42250 42332 42438 42591 42812 42916 42955 43531 43905 43915 44088 44103 44241 44356 45618 46237 47125 47168 47196 47306 47741 48193 48845 48882 49053https://cdsarc.cds.unistra.fr/viz-bin/moc/J/ApJ/879/10?format=asciiRadiodefaultJ/ApJ/879/10/table1Upper limits of gravitational wave amplitude and other derived quantities from erratum published in 2020, ApJ, 899, 170SimbadNameSimbad column added by the CDSmeta.idcharnullableA17Display data from Abbott+, 2017, J/ApJ/839/12meta.ref.urlintnullablerecnoRecord number assigned by the VizieR team. Should Not be used for identification.meta.recordintPSRPulsar J2000 coordinate namemeta.id;meta.maincharFreq[9/707.3] Pulsar rotation frequencyHzem.freqfloatProt/dt[4.4e-22/4.3e-13]? Intrinsic rotational period derivative (1)s/sstat.fit.omcdoublenullabler_Prot/dtReference note for the period derivative value (2)stat.fit.omccharDist[0.1/13.81]? Distance to the pulsarkpcpos.distance;pos.heliocentricfloatnullabler_DistReference note for the pulsar distance (2)meta.ref;pos.framecharH0sd[1.2e-28/3.4e-24]? Spin-down limit of gravitational wave amplitudesrc.var.amplitudedoublenullableC21ULB[1.2e-26/8.5e-23]? Observed 95% credible upper limit on amplitude from the l=2, m=1 mode using the Bayesian analysis (3)src.var.amplitudedoublenullableC21ULrB[5.8e-26/1.5e-23]? Observed 95% credible upper limit on amplitude from the l=2, m=1 mode using restricted orientation priors using the Bayesian analysis (3)src.var.amplitudedoublenullableC21ULF[2.5e-26/2.1e-23]? Observed 95% confidence upper limit on amplitude from the l=2, m=1 mode using the F-statistic analysis (3)src.var.amplitudedoublenullableC21ULrG[1e-25/1.1e-23]? Observed 95% confidence upper limit on amplitude from the l=2, m=1 mode using restricted orientation priors using the G-statistic analysis (3)src.var.amplitudedoublenullableC21UL5nV[1.2e-26/10e-25]? Observed 95% confidence upper limit on amplitude from the l=2, m=1 mode using the 5n-vector analysissrc.var.amplitudedoublenullableC21ULr5nV[1.3e-25/2.1e-25]? Observed 95% confidence upper limit on amplitude from the l=2, m=1 mode using restricted orientation priors using the 5n-vector analysissrc.var.amplitudedoublenullableC22ULB[4e-27/1.7e-25]? Observed 95% credible upper limit on amplitude from the l=m=2 mode using the Bayesian analysis (3)src.var.amplitudedoublenullableC22ULrB[7.2e-27/1.1e-25]? Observed 95% credible upper limit on amplitude from the l=m=2 mode using restricted orientation priors using the Bayesian analysis (3)src.var.amplitudedoublenullableC22ULF[5.6e-27/1.1e-25]? Observed 95% confidence upper limit on amplitude from the l=m=2 mode using the F-statistic analysis (3)src.var.amplitudedoublenullableC22ULrG[1.1e-26/8.8e-26]? Observed 95% confidence upper limit on amplitude from the l=m=2 mode using restricted orientation priors using the G-statistic analysis (3)src.var.amplitudedoublenullableH0ULB[8.8e-27/7.3e-25] Observed 95% credible upper limit on amplitude from the l=m=2 mode using the Bayesian analysis (4)src.var.amplitudedoubleH0ULrB[1.4e-26/2.7e-25]? Observed 95% credible upper limit on amplitude from the l=m=2 mode using restricted orientation priors using the Bayesian analysis (4)src.var.amplitudedoublenullableH0ULF[1.1e-26/2.8e-25]? Observed 95% confidence upper limit on amplitude from the l=m=2 mode using the F-statistic analysis (4)src.var.amplitudedoublenullableH0ULrG[1.3e-26/2e-25]? Observed 95% confidence upper limit on amplitude from the l=m=2 mode using restricted orientation priors using the G-statistic analysis (4)src.var.amplitudedoublenullableH0UL5nV[1.2e-26/4.7e-25]? Observed 95% confidence upper limit on amplitude from the l=m=2 mode using the 5n-vector analysis (4)src.var.amplitudedoublenullableH0ULr5nV[1.9e-26/2.4e-25]? Observed 95% confidence upper limit on amplitude from the l=m=2 mode using restricted orientation priors using the 5n-vector analysis (4)src.var.amplitudedoublenullableQ22ULB[1E+30/1.62e+36]? Derived 95% credible upper limit on the l=m=2 mass quadrupole moment using the Bayesian analysis (4)kg.m**2stat.fit.paramdoublenullableQ22ULrB[6.3E+32/1.13e+34]? Derived 95% credible upper limit on the l=m=2 mass quadrupole moment using restricted orientation priors using the Bayesian analysis (4)kg.m**2stat.fit.paramdoublenullableQ22ULF[9.1e+32/7.02e+34]? Derived 95% confidence upper limit on the l=m=2 mass quadrupole moment using the F-statistic analysis (4)kg.m**2stat.fit.paramdoublenullableQ22ULrG[5.4e+32/8.4e+33]? Derived 95% confidence upper limit on the l=m=2 mass quadrupole moment using restricted orientation priors using the G-statistic analysis (4)kg.m**2stat.fit.paramdoublenullableQ22UL5nV[9E+29/1.45e+35]? Derived 95% confidence upper limit on the l=m=2 mass quadrupole moment using the 5n-vector analysis (4)kg.m**2stat.fit.paramdoublenullableQ22ULr5nV[1.2E+33/9.92e+33]? Derived 95% confidence upper limit on the l=m=2 mass quadrupole moment using restricted orientation priors using the 5n-vector analysis (4)kg.m**2stat.fit.paramdoublenullableellULB[5.7e-9/0.021]? Derived 95% credible upper limit on the fiducial ellipticity using the Bayesian analysis (4)src.ellipticitydoublenullableellULrB[7.8e-6/0.00015]? Derived 95% credible upper limit on the fiducial ellipticity using restricted orientation priors using the Bayesian analysis (4)src.ellipticitydoublenullableellULF[6e-8/0.001]? Derived 95% confidence upper limit on the fiducial ellipticity using the F-statistic analysis (4)src.ellipticitydoublenullableellULrG[6.9e-6/0.00011]? Derived 95% confidence upper limit on the fiducial ellipticity using restricted orientation priors using the G-statistic analysis (4)src.ellipticitydoublenullableellUL5nV[1.1e-8/0.002]? Derived 95% confidence upper limit on the fiducial ellipticity using the 5n-vector analysis (4)src.ellipticitydoublenullableellULr5nV[1.5e-5/0.00013]? Derived 95% confidence upper limit on the fiducial ellipticity using restricted orientation priors using the 5n-vector analysis (4)src.ellipticitydoublenullableH0ULB/H0sd[0.013/3188]? Ratio H0UL_BAYES/H0SD (4)stat.fit.omcdoublenullableH0ULrB/H0sd[0.01/0.2]? Ratio H0ULResBayes/H0SD (4)stat.fit.omcdoublenullableH0ULF/H0sd[0.015/7.3]? Ratio H0ULFStat/H0SD (4)stat.fit.omcdoublenullableH0ULrG/H0sd[0.009/0.06]? Ratio H0ULResGStat/H0SD (4)stat.fit.omcdoublenullableH0UL5nV/H0sd[0.02/4.6]? Ratio H0UL5nVec/H0SD (4)stat.fit.omcdoublenullableH0ULr5nV/H0sd[0.02/0.3]? Ratio H0ULRes5nVec/H0SD (4)stat.fit.omcdoublenullablelogOl2m12B[-6.2/-1.8] Base-10 logarithm of odds for coherent signal versus incoherent signal for the Bayesian analysis (3)stat.snrfloatlogOl2m12rB[-5.3/-3.1]? Base-10 logarithm of odds for coherent signal versus incoherent signal using restricted orientation priors for the Bayesian analysis (3)stat.snrfloatnullablelogOl2m2B[-3.4/-0.5] Base-10 logarithm of odds for coherent signal versus incoherent signal for the Bayesian analysis (4)stat.snrfloatlogOl2m2rB[-2.9/-2.1]? Base-10 logarithm of odds for coherent signal versus incoherent signal using restricted orientation priors for the Bayesian analysis (4)stat.snrfloatnullableP5nVl2m2[0.13/0.99]? P-value for the null hypothesis in the 5n-vector analysis for the l=m=2 modestat.fit.goodnessfloatnullableP5nVl2m1[0.06/0.8]? P-value for the null hypothesis in the 5n-vector analysis for the l=2, m=1 modestat.fit.goodnessfloatnullableFAPl2m2F[0.26/0.8]? False alarm probability in the F-statistic analysis for the l=2, m=2 modestat.fit.goodnessfloatnullableFAPl2m2G[0.75/0.87]? False alarm probability in the G-statistic analysis for the l=2, m=2 modestat.fit.goodnessfloatnullableFAPl2m1F[0.04/0.8]? False alarm probability in the F-statistic analysis for the l=2, m=1 modestat.fit.goodnessfloatnullableFAPl2m1G[0.18/0.75]? False alarm probability in the G-statistic analysis for the l=2, m=1 modestat.fit.goodnessfloatnullable_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