Erratum: “Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015–2017 LIGO Data” (2019, ApJ, 879, 10)

B. P. Abbott; R. Abbott; T. D. Abbott; S. Abraham; F. Acernese; K. Ackley; C. Adams; R. X. Adhikari; V. B. Adya; C. Affeldt; M. Agathos; K. Agatsuma; N. Aggarwal; O. D. Aguiar; L. Aiello; A. Ain; P. Ajith; G. Allen; A. Allocca; M. A. Aloy; P. A. Altin; A. Amato; A. Ananyeva; S. B. Anderson; W. G. Anderson; S. V. Angelova; S. Antier; S. Appert; K. Arai; M. C. Araya; J. S. Areeda; M. Arène; N. Arnaud; S. Ascenzi; G. Ashton; S. M. Aston; P. Astone; F. Aubin; P. Aufmuth; K. AultONeal; C. Austin; V. Avendano; A. Avila-Alvarez; S. Babak; P. Bacon; F. Badaracco; M. K. M. Bader; S. Bae; M. Bailes; P. T. Baker; F. Baldaccini; G. Ballardin; S. W. Ballmer; S. Banagiri; J. C. Barayoga; S. E. Barclay; B. C. Barish; D. Barker; K. Barkett; S. Barnum; F. Barone; B. Barr; L. Barsotti; M. Barsuglia; D. Barta; J. Bartlett; I. Bartos; R. Bassiri; A. Basti; M. Bawaj; J. C. Bayley; M. Bazzan; B. Bécsy; M. Bejger; I. Belahcene; A. S. Bell; D. Beniwal; B. K. Berger; G. Bergmann; S. Bernuzzi; J. J. Bero; C. 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J. Cowart; D. C. Coyne; R. Coyne; J. D. E. Creighton; T. D. Creighton; J. Cripe; M. Croquette; S. G. Crowder; T. J. Cullen; A. Cumming; L. Cunningham; E. Cuoco; T. Dal Canton; G. Dálya; S. L. Danilishin; S. D’Antonio; K. Danzmann; A. Dasgupta; C. F. Da Silva Costa; L. E. H. Datrier; V. Dattilo; I. Dave; M. Davier; D. Davis; E. J. Daw; D. DeBra; M. Deenadayalan; J. Degallaix; M. De Laurentis; S. Deléglise; W. Del Pozzo; L. M. DeMarchi; N. Demos; T. Dent; R. De Pietri; J. Derby; R. De Rosa; C. De Rossi; R. DeSalvo; O. de Varona; S. Dhurandhar; M. C. Díaz; T. Dietrich; L. Di Fiore; M. Di Giovanni; T. Di Girolamo; A. Di Lieto; B. Ding; S. Di Pace; I. Di Palma; F. Di Renzo; A. Dmitriev; Z. Doctor; F. Donovan; K. L. Dooley; S. Doravari; I. Dorrington; T. P. Downes; M. Drago; J. C. Driggers; Z. Du; J.-G. Ducoin; P. Dupej; S. E. Dwyer; P. J. Easter; T. B. Edo; M. C. Edwards; A. Effler; P. Ehrens; J. Eichholz; S. S. Eikenberry; M. Eisenmann; R. A. Eisenstein; R. C. Essick; H. Estelles; D. 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M. Magee; E. Majorana; I. Maksimovic; A. Malik; N. Man; V. Mandic; V. Mangano; G. L. Mansell; M. Manske; M. Mantovani; F. Marchesoni; F. Marion; S. Márka; Z. Márka; C. Markakis; A. S. Markosyan; A. Markowitz; E. Maros; A. Marquina; S. Marsat; F. Martelli; I. W. Martin; R. M. Martin; D. V. Martynov; K. Mason; E. Massera; A. Masserot; T. J. Massinger; M. Masso-Reid; S. Mastrogiovanni; A. Matas; F. Matichard; L. Matone; N. Mavalvala; N. Mazumder; J. J. McCann; R. McCarthy; D. E. McClelland; S. McCormick; L. McCuller; S. C. McGuire; J. McIver; D. J. McManus; T. McRae; S. T. McWilliams; D. Meacher; G. D. Meadors; M. Mehmet; A. K. Mehta; J. Meidam; A. Melatos; G. Mendell; R. A. Mercer; L. Mereni; E. L. Merilh; M. Merzougui; S. Meshkov; C. Messenger; C. Messick; R. Metzdorff; P. M. Meyers; H. Miao; C. Michel; H. Middleton; E. E. Mikhailov; L. Milano; A. L. Miller; A. Miller; M. Millhouse; J. C. Mills; M. C. Milovich-Goff; O. Minazzoli; Y. Minenkov; A. Mishkin; C. Mishra; T. Mistry; S. 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Paoli; A. Parida; W. Parker; D. Pascucci; A. Pasqualetti; R. Passaquieti; D. Passuello; M. Patil; B. Patricelli; B. L. Pearlstone; C. Pedersen; M. Pedraza; R. Pedurand; A. Pele; S. Penn; C. J. Perez; A. Perreca; H. P. Pfeiffer; M. Phelps; K. S. Phukon; O. J. Piccinni; M. Pichot; F. Piergiovanni; G. Pillant; L. Pinard; M. Pirello; M. Pitkin; R. Poggiani; D. Y. T. Pong; S. Ponrathnam; P. Popolizio; E. K. Porter; J. Powell; A. K. Prajapati; J. Prasad; K. Prasai; R. Prasanna; G. Pratten; T. Prestegard; S. Privitera; G. A. Prodi; L. G. Prokhorov; O. Puncken; M. Punturo; P. Puppo; M. Pürrer; H. Qi; V. Quetschke; P. J. Quinonez; E. A. Quintero; R. Quitzow-James; F. J. Raab; H. Radkins; N. Radulescu; P. Raffai; S. Raja; C. Rajan; B. Rajbhandari; M. Rakhmanov; K. E. Ramirez; A. Ramos-Buades; Javed Rana; K. Rao; P. Rapagnani; V. Raymond; M. Razzano; J. Read; T. Regimbau; L. Rei; S. Reid; D. H. Reitze; W. Ren; F. Ricci; C. J. Richardson; J. W. Richardson; P. M. Ricker; K. Riles; M. Rizzo; N. A. 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Tso; L. Tsukada; D. Tsuna; D. Tuyenbayev; K. Ueno; D. Ugolini; C. S. Unnikrishnan; A. L. Urban; S. A. Usman; H. Vahlbruch; G. Vajente; G. Valdes; N. van Bakel; M. van Beuzekom; J. F. J. van den Brand; C. Van Den Broeck; D. C. Vander-Hyde; J. V. van Heijningen; L. van der Schaaf; A. A. van Veggel; M. Vardaro; V. Varma; S. Vass; M. Vasúth; A. Vecchio; G. Vedovato; J. Veitch; P. J. Veitch; K. Venkateswara; G. Venugopalan; D. Verkindt; F. Vetrano; A. Viceré; A. D. Viets; D. J. Vine; J.-Y. Vinet; S. Vitale; T. Vo; H. Vocca; C. Vorvick; S. P. Vyatchanin; A. R. Wade; L. E. Wade; M. Wade; R. Walet; M. Walker; L. Wallace; S. Walsh; G. Wang; H. Wang; J. Z. Wang; W. H. Wang; Y. F. Wang; R. L. Ward; Z. A. Warden; J. Warner; M. Was; J. Watchi; B. Weaver; L.-W. Wei; M. Weinert; A. J. Weinstein; R. Weiss; F. Wellmann; L. Wen; E. K. Wessel; P. Weßels; J. W. Westhouse; K. Wette; J. T. Whelan; B. F. Whiting; C. Whittle; D. M. Wilken; D. Williams; A. R. Williamson; J. L. Willis; B. Willke; M. H. Wimmer; W. Winkler; C. C. Wipf; H. Wittel; G. Woan; J. Woehler; J. K. Wofford; J. Worden; J. L. Wright; D. S. Wu; D. M. Wysocki; L. Xiao; H. Yamamoto; C. C. Yancey; L. Yang; M. J. Yap; M. Yazback; D. W. Yeeles; Hang Yu; Haocun Yu; S. H. R. Yuen; M. Yvert; A. K. Zadrożny; M. Zanolin; T. Zelenova; J.-P. Zendri; M. Zevin; J. Zhang; L. Zhang; T. Zhang; C. Zhao; M. Zhou; Z. Zhou; X. J. Zhu; M. E. Zucker; J. Zweizig; The LIGO Scientific Collaboration and the Virgo Collaboration; Z. Arzoumanian; S. Bogdanov; I. Cognard; A. Corongiu; T. Enoto; P. Freire; K. C. Gendreau; L. Guillemot; A. K. Harding; F. Jankowski; M. J. Keith; M. Kerr; A. Lyne; J. Palfreyman; A. Possenti; A. Ridolfi; B. Stappers; G. Theureau; P. Weltervrede

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Erratum: "Searches for Gravitational Waves from Known Pulsars at Two Harmonics in 2015–2017 LIGO Data" (2019, ApJ, 879, 10)

B. P. Abbott¹, R. Abbott¹, T. D. Abbott², S. Abraham³, F. Acernese^4,5, K. Ackley⁶, C. Adams⁷, R. X. Adhikari¹, V. B. Adya^8,9, C. Affeldt^8,9, M. Agathos¹⁰, K. Agatsuma¹¹, N. Aggarwal¹², O. D. Aguiar¹³, L. Aiello^14,15, A. Ain³, P. Ajith¹⁶, G. Allen¹⁷, A. Allocca^18,19, M. A. Aloy²⁰, P. A. Altin²¹, A. Amato²², A. Ananyeva¹, S. B. Anderson¹, W. G. Anderson²³, S. V. Angelova²⁴, S. Antier²⁵, S. Appert¹, K. Arai¹, M. C. Araya¹, J. S. Areeda²⁶, M. Arène²⁷, N. Arnaud^25,28, S. Ascenzi^29,30, G. Ashton⁶, S. M. Aston⁷, P. Astone³¹, F. Aubin³², P. Aufmuth⁹, K. AultONeal³³, C. Austin², V. Avendano³⁴, A. Avila-Alvarez²⁶, S. Babak^27,35, P. Bacon²⁷, F. Badaracco^14,15, M. K. M. Bader³⁶, S. Bae³⁷, M. Bailes³⁸, P. T. Baker³⁹, F. Baldaccini^40,41, G. Ballardin²⁸, S. W. Ballmer⁴², S. Banagiri⁴³, J. C. Barayoga¹, S. E. Barclay⁴⁴, B. C. Barish¹, D. Barker⁴⁵, K. Barkett⁴⁶, S. Barnum¹², F. Barone^4,5, B. Barr⁴⁴, L. Barsotti¹², M. Barsuglia²⁷, D. Barta⁴⁷, J. Bartlett⁴⁵, I. Bartos⁴⁸, R. Bassiri⁴⁹, A. Basti^18,19, M. Bawaj^41,50, J. C. Bayley⁴⁴, M. Bazzan^51,52, B. Bécsy⁵³, M. Bejger^27,54, I. Belahcene²⁵, A. S. Bell⁴⁴, D. Beniwal⁵⁵, B. K. Berger⁴⁹, G. Bergmann^8,9, S. Bernuzzi^56,57, J. J. Bero⁵⁸, C. P. L. Berry⁵⁹, D. Bersanetti⁶⁰, A. Bertolini³⁶, J. Betzwieser⁷, R. Bhandare⁶¹, J. Bidler²⁶, I. A. Bilenko⁶², S. A. Bilgili³⁹, G. Billingsley¹, J. Birch⁷, R. Birney²⁴, O. Birnholtz⁵⁸, S. Biscans^1,12, S. Biscoveanu⁶, A. Bisht⁹, M. Bitossi^19,28, M. A. Bizouard²⁵, J. K. Blackburn¹, C. D. Blair⁷, D. G. Blair⁶³, R. M. Blair⁴⁵, S. Bloemen⁶⁴, N. Bode^8,9, M. Boer⁶⁵, Y. Boetzel⁶⁶, G. Bogaert⁶⁵, F. Bondu⁶⁷, E. Bonilla⁴⁹, R. Bonnand³², P. Booker^8,9, B. A. Boom³⁶, C. D. Booth⁶⁸, R. Bork¹, V. Boschi²⁸, S. Bose^3,69, K. Bossie⁷, V. Bossilkov⁶³, J. Bosveld⁶³, Y. Bouffanais²⁷, A. Bozzi²⁸, C. Bradaschia¹⁹, P. R. Brady²³, A. Bramley⁷, M. Branchesi^14,15, J. E. Brau⁷⁰, T. Briant⁷¹, J. H. Briggs⁴⁴, F. Brighenti^72,73, A. Brillet⁶⁵, M. Brinkmann^8,9, V. Brisson^191,25, P. Brockill²³, A. F. Brooks¹, D. D. Brown⁵⁵, S. Brunett¹, A. Buikema¹², T. Bulik⁷⁴, H. J. Bulten^36,75, A. Buonanno^35,76, D. Buskulic³², C. Buy²⁷, R. L. Byer⁴⁹, M. Cabero^8,9, L. Cadonati⁷⁷, G. Cagnoli^22,78, C. Cahillane¹, J. Calderón Bustillo⁶, T. A. Callister¹, E. Calloni^5,79, J. B. Camp⁸⁰, W. A. Campbell⁶, M. Canepa^60,81, K. C. Cannon⁸², H. Cao⁵⁵, J. Cao⁸³, E. Capocasa²⁷, F. Carbognani²⁸, S. Caride⁸⁴, M. F. Carney⁵⁹, G. Carullo¹⁸, J. Casanueva Diaz¹⁹, C. Casentini^29,30, S. Caudill³⁶, M. Cavaglià⁸⁵, F. Cavalier²⁵, R. Cavalieri²⁸, G. Cella¹⁹, P. Cerdá-Durán²⁰, G. Cerretani^18,19, E. Cesarini^30,86, O. Chaibi⁶⁵, K. Chakravarti³, S. J. Chamberlin⁸⁷, M. Chan⁴⁴, S. Chao⁸⁸, P. Charlton⁸⁹, E. A. Chase⁵⁹, E. Chassande-Mottin²⁷, D. Chatterjee²³, M. Chaturvedi⁶¹, B. D. Cheeseboro³⁹, H. Y. Chen⁹⁰, X. Chen⁶³, Y. Chen⁴⁶, H.-P. Cheng⁴⁸, C. K. Cheong⁹¹, H. Y. Chia⁴⁸, A. Chincarini⁶⁰, A. Chiummo²⁸, G. Cho⁹², H. S. Cho⁹³, M. Cho⁷⁶, N. Christensen^65,94, Q. Chu⁶³, S. Chua⁷¹, K. W. Chung⁹¹, S. Chung⁶³, G. Ciani^51,52, A. A. 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Deenadayalan³, J. Degallaix²², M. De Laurentis^5,79, S. Deléglise⁷¹, W. Del Pozzo^18,19, L. M. DeMarchi⁵⁹, N. Demos¹², T. Dent^8,9,109, R. De Pietri^57,110, J. Derby²⁶, R. De Rosa^5,79, C. De Rossi^22,28, R. DeSalvo¹¹¹, O. de Varona^8,9, S. Dhurandhar³, M. C. Díaz¹⁰⁴, T. Dietrich³⁶, L. Di Fiore⁵, M. Di Giovanni^96,112, T. Di Girolamo^5,79, A. Di Lieto^18,19, B. Ding¹⁰⁰, S. Di Pace^31,113, I. Di Palma^31,113, F. Di Renzo^18,19, A. Dmitriev¹¹, Z. Doctor⁹⁰, F. Donovan¹², K. L. Dooley^68,85, S. Doravari^8,9, I. Dorrington⁶⁸, T. P. Downes²³, M. Drago^14,15, J. C. Driggers⁴⁵, Z. Du⁸³, J.-G. Ducoin²⁵, P. Dupej⁴⁴, S. E. Dwyer⁴⁵, P. J. Easter⁶, T. B. Edo¹⁰⁸, M. C. Edwards⁹⁴, A. Effler⁷, P. Ehrens¹, J. Eichholz¹, S. S. Eikenberry⁴⁸, M. Eisenmann³², R. A. Eisenstein¹², R. C. Essick⁹⁰, H. Estelles⁹⁹, D. Estevez³², Z. B. Etienne³⁹, T. Etzel¹, M. Evans¹², T. M. Evans⁷, V. Fafone^14,29,30, H. Fair⁴², S. Fairhurst⁶⁸, X. Fan⁸³, S. Farinon⁶⁰, B. Farr⁷⁰, W. M. Farr¹¹, E. J. Fauchon-Jones⁶⁸, M. 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Gill³³, G. Giordano^4,5, L. Glover¹¹¹, P. Godwin⁸⁷, E. Goetz⁴⁵, R. Goetz⁴⁸, B. Goncharov⁶, G. González², J. M. Gonzalez Castro^18,19, A. Gopakumar¹²⁴, M. L. Gorodetsky⁶², S. E. Gossan¹, M. Gosselin²⁸, R. Gouaty³², A. Grado^5,125, C. Graef⁴⁴, M. Granata²², A. Grant⁴⁴, S. Gras¹², P. Grassia¹, C. Gray⁴⁵, R. Gray⁴⁴, G. Greco^72,73, A. C. Green^11,48, R. Green⁶⁸, E. M. Gretarsson³³, P. Groot⁶⁴, H. Grote⁶⁸, S. Grunewald³⁵, P. Gruning²⁵, G. M. Guidi^72,73, H. K. Gulati¹⁰⁷, Y. Guo³⁶, A. Gupta⁸⁷, M. K. Gupta¹⁰⁷, E. K. Gustafson¹, R. Gustafson¹²⁶, L. Haegel⁹⁹, O. Halim^14,15, B. R. Hall⁶⁹, E. D. Hall¹², E. Z. Hamilton⁶⁸, G. Hammond⁴⁴, M. Haney⁶⁶, M. M. Hanke^8,9, J. Hanks⁴⁵, C. Hanna⁸⁷, M. D. Hannam⁶⁸, O. A. Hannuksela⁹¹, J. Hanson⁷, T. Hardwick², K. Haris¹⁶, J. Harms^14,15, G. M. Harry¹²⁷, I. W. Harry³⁵, C.-J. Haster¹¹⁸, K. Haughian⁴⁴, F. J. Hayes⁴⁴, J. Healy⁵⁸, A. Heidmann⁷¹, M. C. Heintze⁷, H. Heitmann⁶⁵, P. Hello²⁵, G. Hemming²⁸, M. Hendry⁴⁴, I. S. Heng⁴⁴, J. Hennig^8,9, A. W. Heptonstall¹, Francisco Hernandez Vivanco⁶, M. Heurs^8,9, S. Hild⁴⁴, T. Hinderer^36,128,129, W. C. G. Ho¹³⁰, D. Hoak²⁸, S. Hochheim^8,9, D. Hofman²², A. M. Holgado¹⁷, N. A. Holland²¹, K. Holt⁷, D. E. Holz⁹⁰, P. Hopkins⁶⁸, C. Horst²³, J. Hough⁴⁴, E. J. Howell⁶³, C. G. Hoy⁶⁸, A. Hreibi⁶⁵, E. A. Huerta¹⁷, D. Huet²⁵, B. Hughey³³, M. Hulko¹, S. Husa⁹⁹, S. H. Huttner⁴⁴, T. Huynh-Dinh⁷, B. Idzkowski⁷⁴, A. Iess^29,30, C. Ingram⁵⁵, R. Inta⁸⁴, G. Intini^31,113, B. Irwin¹¹⁵, H. N. Isa⁴⁴, J.-M. Isac⁷¹, M. Isi¹, B. R. Iyer¹⁶, K. Izumi⁴⁵, T. Jacqmin⁷¹, S. J. Jadhav¹³¹, K. Jani⁷⁷, N. N. Janthalur¹³¹, P. Jaranowski¹³², A. C. Jenkins¹³³, J. Jiang⁴⁸, D. S. Johnson¹⁷, A. W. Jones¹¹, D. I. Jones¹³⁴, R. Jones⁴⁴, R. J. G. Jonker³⁶, L. Ju⁶³, J. Junker^8,9, C. V. Kalaghatgi⁶⁸, V. Kalogera⁵⁹, B. Kamai¹, S. Kandhasamy⁸⁵, G. Kang³⁷, J. B. Kanner¹, S. J. Kapadia²³, S. Karki⁷⁰, K. S. Karvinen^8,9, R. Kashyap¹⁶, M. Kasprzack¹, S. Katsanevas²⁸, E. Katsavounidis¹², W. Katzman⁷, S. Kaufer⁹, K. Kawabe⁴⁵, N. V. Keerthana³, F. Kéfélian⁶⁵, D. Keitel⁴⁴, R. Kennedy¹⁰⁸, J. S. Key¹³⁵, F. Y. Khalili⁶², H. Khan²⁶, I. Khan^14,30, S. Khan^8,9, Z. Khan¹⁰⁷, E. A. Khazanov¹³⁶, M. Khursheed⁶¹, N. Kijbunchoo²¹, Chunglee Kim¹³⁷, J. C. Kim¹³⁸, K. Kim⁹¹, W. Kim⁵⁵, W. S. Kim¹³⁹, Y.-M. Kim¹⁴⁰, C. Kimball⁵⁹, E. J. King⁵⁵, P. J. King⁴⁵, M. Kinley-Hanlon¹²⁷, R. Kirchhoff^8,9, J. S. Kissel⁴⁵, L. Kleybolte¹⁴¹, J. H. Klika²³, S. Klimenko⁴⁸, T. D. Knowles³⁹, P. Koch^8,9, S. M. Koehlenbeck^8,9, G. Koekoek^36,142, S. Koley³⁶, V. Kondrashov¹, A. Kontos¹², N. Koper^8,9, M. Korobko¹⁴¹, W. Z. Korth¹, I. Kowalska⁷⁴, D. B. Kozak¹, V. Kringel^8,9, N. Krishnendu¹⁴³, A. Królak^144,145, G. Kuehn^8,9, A. Kumar¹³¹, P. Kumar¹⁴⁶, R. Kumar¹⁰⁷, S. Kumar¹⁶, L. Kuo⁸⁸, A. Kutynia¹⁴⁴, S. Kwang²³, B. D. Lackey³⁵, K. H. Lai⁹¹, T. L. Lam⁹¹, M. Landry⁴⁵, B. B. Lane¹², R. N. Lang¹⁴⁷, J. Lange⁵⁸, B. Lantz⁴⁹, R. K. Lanza¹², A. Lartaux-Vollard²⁵, P. D. Lasky⁶, M. Laxen⁷, A. Lazzarini¹, C. Lazzaro⁵², P. Leaci^31,113, S. Leavey^8,9, Y. K. Lecoeuche⁴⁵, C. H. Lee⁹³, H. K. Lee¹⁴⁸, H. M. Lee¹⁴⁹, H. W. Lee¹³⁸, J. Lee⁹², K. Lee⁴⁴, J. Lehmann^8,9, A. Lenon³⁹, N. Leroy²⁵, N. Letendre³², Y. Levin^6,98, J. Li⁸³, K. J. L. Li⁹¹, T. G. F. Li⁹¹, X. Li⁴⁶, F. Lin⁶, F. Linde³⁶, S. D. Linker¹¹¹, T. B. Littenberg¹⁵⁰, J. Liu⁶³, X. Liu²³, R. K. L. Lo^1,91, N. A. Lockerbie²⁴, L. T. London⁶⁸, A. Longo^151,152, M. Lorenzini^14,15, V. Loriette¹⁵³, M. Lormand⁷, G. Losurdo¹⁹, J. D. Lough^8,9, C. O. Lousto⁵⁸, G. Lovelace²⁶, M. E. Lower³⁸, H. Lück^8,9, D. Lumaca^29,30, A. P. Lundgren¹⁵⁴, R. Lynch¹², Y. Ma⁴⁶, R. Macas⁶⁸, S. Macfoy²⁴, M. MacInnis¹², D. M. Macleod⁶⁸, A. Macquet⁶⁵, F. Magaña-Sandoval⁴², L. Magaña Zertuche⁸⁵, R. M. Magee⁸⁷, E. Majorana³¹, I. Maksimovic¹⁵³, A. Malik⁶¹, N. Man⁶⁵, V. Mandic⁴³, V. Mangano⁴⁴, G. L. Mansell^12,45, M. Manske^21,23, M. Mantovani²⁸, F. Marchesoni^41,50, F. Marion³², S. Márka⁹⁸, Z. Márka⁹⁸, C. Markakis^10,17, A. S. Markosyan⁴⁹, A. Markowitz¹, E. Maros¹, A. Marquina¹⁰², S. Marsat³⁵, F. Martelli^72,73, I. W. Martin⁴⁴, R. M. Martin³⁴, D. V. Martynov¹¹, K. Mason¹², E. Massera¹⁰⁸, A. Masserot³², T. J. Massinger¹, M. Masso-Reid⁴⁴, S. Mastrogiovanni^31,113, A. Matas^35,43, F. Matichard^1,12, L. Matone⁹⁸, N. Mavalvala¹², N. Mazumder⁶⁹, J. J. McCann⁶³, R. McCarthy⁴⁵, D. E. McClelland²¹, S. McCormick⁷, L. McCuller¹², S. C. McGuire¹⁵⁵, J. McIver¹, D. J. McManus²¹, T. McRae²¹, S. T. McWilliams³⁹, D. Meacher⁸⁷, G. D. Meadors⁶, M. Mehmet^8,9, A. K. Mehta¹⁶, J. Meidam³⁶, A. Melatos⁹⁷, G. Mendell⁴⁵, R. A. Mercer²³, L. Mereni²², E. L. Merilh⁴⁵, M. Merzougui⁶⁵, S. Meshkov¹, C. Messenger⁴⁴, C. Messick⁸⁷, R. Metzdorff⁷¹, P. M. Meyers⁹⁷, H. Miao¹¹, C. Michel²², H. Middleton⁹⁷, E. E. Mikhailov¹⁵⁶, L. Milano^5,79, A. L. Miller⁴⁸, A. Miller^31,113, M. Millhouse⁵³, J. C. Mills⁶⁸, M. C. Milovich-Goff¹¹¹, O. Minazzoli^65,157, Y. Minenkov³⁰, A. Mishkin⁴⁸, C. Mishra¹⁵⁸, T. Mistry¹⁰⁸, S. Mitra³, V. P. Mitrofanov⁶², G. Mitselmakher⁴⁸, R. Mittleman¹², G. Mo⁹⁴, D. Moffa¹¹⁵, K. Mogushi⁸⁵, S. R. P. Mohapatra¹², M. Montani^72,73, C. J. Moore¹⁰, D. Moraru⁴⁵, G. Moreno⁴⁵, S. Morisaki⁸², B. Mours³², C. M. Mow-Lowry¹¹, Arunava Mukherjee^8,9, D. Mukherjee²³, S. Mukherjee¹⁰⁴, N. Mukund³, A. Mullavey⁷, J. Munch⁵⁵, E. A. Muñiz⁴², M. Muratore³³, P. G. Murray⁴⁴, A. Nagar^86,159,160, I. Nardecchia^29,30, L. Naticchioni^31,113, R. K. Nayak¹⁶¹, J. Neilson¹¹¹, G. Nelemans^36,64, T. J. N. Nelson⁷, M. Nery^8,9, A. Neunzert¹²⁶, K. Y. Ng¹², S. Ng⁵⁵, P. Nguyen⁷⁰, D. Nichols^36,128, S. Nissanke^36,128, F. Nocera²⁸, C. North⁶⁸, L. K. Nuttall¹⁵⁴, M. Obergaulinger²⁰, J. Oberling⁴⁵, B. D. O'Brien⁴⁸, G. D. O'Dea¹¹¹, G. H. Ogin¹⁶², J. J. Oh¹³⁹, S. H. Oh¹³⁹, F. Ohme^8,9, H. Ohta⁸², M. A. Okada¹³, M. Oliver⁹⁹, P. Oppermann^8,9, Richard J. Oram⁷, B. O'Reilly⁷, R. G. Ormiston⁴³, L. F. Ortega⁴⁸, R. O'Shaughnessy⁵⁸, S. Ossokine³⁵, D. J. Ottaway⁵⁵, H. Overmier⁷, B. J. Owen⁸⁴, A. E. Pace⁸⁷, G. Pagano^18,19, M. A. Page⁶³, A. Pai¹²², S. A. Pai⁶¹, J. R. Palamos⁷⁰, O. Palashov¹³⁶, C. Palomba³¹, A. Pal-Singh¹⁴¹, Huang-Wei Pan⁸⁸, B. Pang⁴⁶, P. T. H. Pang⁹¹, C. Pankow⁵⁹, F. Pannarale^31,113, B. C. Pant⁶¹, F. Paoletti¹⁹, A. Paoli²⁸, A. Parida³, W. Parker^7,155, D. Pascucci⁴⁴, A. Pasqualetti²⁸, R. Passaquieti^18,19, D. Passuello¹⁹, M. Patil¹⁴⁵, B. Patricelli^18,19, B. L. Pearlstone⁴⁴, C. Pedersen⁶⁸, M. Pedraza¹, R. Pedurand^22,163, A. Pele⁷, S. Penn¹⁶⁴, C. J. Perez⁴⁵, A. Perreca^96,112, H. P. Pfeiffer^35,118, M. Phelps^8,9, K. S. Phukon³, O. J. Piccinni^31,113, M. Pichot⁶⁵, F. Piergiovanni^72,73, G. Pillant²⁸, L. Pinard²², M. Pirello⁴⁵, M. Pitkin⁴⁴, R. Poggiani^18,19, D. Y. T. Pong⁹¹, S. Ponrathnam³, P. Popolizio²⁸, E. K. Porter²⁷, J. Powell³⁸, A. K. Prajapati¹⁰⁷, J. Prasad³, K. Prasai⁴⁹, R. Prasanna¹³¹, G. Pratten⁹⁹, T. Prestegard²³, S. Privitera³⁵, G. A. Prodi^96,112, L. G. Prokhorov⁶², O. Puncken^8,9, M. Punturo⁴¹, P. Puppo³¹, M. Pürrer³⁵, H. Qi²³, V. Quetschke¹⁰⁴, P. J. Quinonez³³, E. A. Quintero¹, R. Quitzow-James⁷⁰, F. J. Raab⁴⁵, H. Radkins⁴⁵, N. Radulescu⁶⁵, P. Raffai¹⁰⁶, S. Raja⁶¹, C. Rajan⁶¹, B. Rajbhandari⁸⁴, M. Rakhmanov¹⁰⁴, K. E. Ramirez¹⁰⁴, A. Ramos-Buades⁹⁹, Javed Rana³, K. Rao⁵⁹, P. Rapagnani^31,113, V. Raymond⁶⁸, M. Razzano^18,19, J. Read²⁶, T. Regimbau³², L. Rei⁶⁰, S. Reid²⁴, D. H. Reitze^1,48, W. Ren¹⁷, F. Ricci^31,113, C. J. Richardson³³, J. W. Richardson¹, P. M. Ricker¹⁷, K. Riles¹²⁶, M. Rizzo⁵⁹, N. A. Robertson^1,44, R. Robie⁴⁴, F. Robinet²⁵, A. Rocchi³⁰, L. Rolland³², J. G. Rollins¹, V. J. Roma⁷⁰, M. Romanelli⁶⁷, R. Romano^4,5, C. L. Romel⁴⁵, J. H. Romie⁷, K. Rose¹¹⁵, D. Rosińska^54,165, S. G. Rosofsky¹⁷, M. P. Ross¹⁶⁶, S. Rowan⁴⁴, A. Rüdiger^193,8,9, P. Ruggi²⁸, G. Rutins¹⁶⁷, K. Ryan⁴⁵, S. Sachdev¹, T. Sadecki⁴⁵, M. Sakellariadou¹³³, L. Salconi²⁸, M. Saleem¹⁴³, A. Samajdar³⁶, L. Sammut⁶, E. J. Sanchez¹, L. E. Sanchez¹, N. Sanchis-Gual²⁰, V. Sandberg⁴⁵, J. R. Sanders⁴², K. A. Santiago³⁴, N. Sarin⁶, B. Sassolas²², P. R. Saulson⁴², O. Sauter¹²⁶, R. L. Savage⁴⁵, P. Schale⁷⁰, M. Scheel⁴⁶, J. Scheuer⁵⁹, P. Schmidt⁶⁴, R. Schnabel¹⁴¹, R. M. S. Schofield⁷⁰, A. Schönbeck¹⁴¹, E. Schreiber^8,9, B. W. Schulte^8,9, B. F. Schutz⁶⁸, S. G. Schwalbe³³, J. Scott⁴⁴, S. M. Scott²¹, E. Seidel¹⁷, D. Sellers⁷, A. S. Sengupta¹⁶⁸, N. Sennett³⁵, D. Sentenac²⁸, V. Sequino^14,29,30, A. Sergeev¹³⁶, Y. Setyawati^8,9, D. A. Shaddock²¹, T. Shaffer⁴⁵, M. S. Shahriar⁵⁹, M. B. Shaner¹¹¹, L. Shao³⁵, P. Sharma⁶¹, P. Shawhan⁷⁶, H. Shen¹⁷, R. Shink¹⁶⁹, D. H. Shoemaker¹², D. M. Shoemaker⁷⁷, S. ShyamSundar⁶¹, K. Siellez⁷⁷, M. Sieniawska⁵⁴, D. Sigg⁴⁵, A. D. Silva¹³, L. P. Singer⁸⁰, N. Singh⁷⁴, A. Singhal^14,31, A. M. Sintes⁹⁹, S. Sitmukhambetov¹⁰⁴, V. Skliris⁶⁸, B. J. J. Slagmolen²¹, T. J. Slaven-Blair⁶³, J. R. Smith²⁶, R. J. E. Smith⁶, S. Somala¹⁷⁰, E. J. Son¹³⁹, B. Sorazu⁴⁴, F. Sorrentino⁶⁰, T. Souradeep³, E. Sowell⁸⁴, A. P. Spencer⁴⁴, A. K. Srivastava¹⁰⁷, V. Srivastava⁴², K. Staats⁵⁹, C. Stachie⁶⁵, M. Standke^8,9, D. A. Steer²⁷, M. Steinke^8,9, J. Steinlechner^44,141, S. Steinlechner¹⁴¹, D. Steinmeyer^8,9, S. P. Stevenson³⁸, D. Stocks⁴⁹, R. Stone¹⁰⁴, D. J. Stops¹¹, K. A. Strain⁴⁴, G. Stratta^72,73, S. E. Strigin⁶², A. Strunk⁴⁵, R. Sturani¹⁷¹, A. L. Stuver¹⁷², V. Sudhir¹², T. Z. Summerscales¹⁷³, L. Sun¹, S. Sunil¹⁰⁷, J. Suresh³, P. J. Sutton⁶⁸, B. L. Swinkels³⁶, M. J. Szczepańczyk³³, M. Tacca³⁶, S. C. Tait⁴⁴, C. Talbot⁶, D. Talukder⁷⁰, D. B. Tanner⁴⁸, M. Tápai¹²³, A. Taracchini³⁵, J. D. Tasson⁹⁴, R. Taylor¹, F. Thies^8,9, M. Thomas⁷, P. Thomas⁴⁵, S. R. Thondapu⁶¹, K. A. Thorne⁷, E. Thrane⁶, Shubhanshu Tiwari^96,112, Srishti Tiwari¹²⁴, V. Tiwari⁶⁸, K. Toland⁴⁴, M. Tonelli^18,19, Z. Tornasi⁴⁴, A. Torres-Forné¹⁷⁴, C. I. Torrie¹, D. Töyrä¹¹, F. Travasso^28,41, G. Traylor⁷, M. C. Tringali⁷⁴, A. Trovato²⁷, L. Trozzo^19,175, R. Trudeau¹, K. W. Tsang³⁶, M. Tse¹², R. Tso⁴⁶, L. Tsukada⁸², D. Tsuna⁸², D. Tuyenbayev¹⁰⁴, K. Ueno⁸², D. Ugolini¹⁷⁶, C. S. Unnikrishnan¹²⁴, A. L. Urban², S. A. Usman⁶⁸, H. Vahlbruch⁹, G. Vajente¹, G. Valdes², N. van Bakel³⁶, M. van Beuzekom³⁶, J. F. J. van den Brand^36,75, C. Van Den Broeck^36,177, D. C. Vander-Hyde⁴², J. V. van Heijningen⁶³, L. van der Schaaf³⁶, A. A. van Veggel⁴⁴, M. Vardaro^51,52, V. Varma⁴⁶, S. Vass¹, M. Vasúth⁴⁷, A. Vecchio¹¹, G. Vedovato⁵², J. Veitch⁴⁴, P. J. Veitch⁵⁵, K. Venkateswara¹⁶⁶, G. Venugopalan¹, D. Verkindt³², F. Vetrano^72,73, A. Viceré^72,73, A. D. Viets²³, D. J. Vine¹⁶⁷, J.-Y. Vinet⁶⁵, S. Vitale¹², T. Vo⁴², H. Vocca^40,41, C. Vorvick⁴⁵, S. P. Vyatchanin⁶², A. R. Wade¹, L. E. Wade¹¹⁵, M. Wade¹¹⁵, R. Walet³⁶, M. Walker²⁶, L. Wallace¹, S. Walsh²³, G. Wang^14,19, H. Wang¹¹, J. Z. Wang¹²⁶, W. H. Wang¹⁰⁴, Y. F. Wang⁹¹, R. L. Ward²¹, Z. A. Warden³³, J. Warner⁴⁵, M. Was³², J. Watchi¹⁰⁰, B. Weaver⁴⁵, L.-W. Wei^8,9, M. Weinert^8,9, A. J. Weinstein¹, R. Weiss¹², F. Wellmann^8,9, L. Wen⁶³, E. K. Wessel¹⁷, P. Weßels^8,9, J. W. Westhouse³³, K. Wette²¹, J. T. Whelan⁵⁸, B. F. Whiting⁴⁸, C. Whittle¹², D. M. Wilken^8,9, D. Williams⁴⁴, A. R. Williamson^36,128, J. L. Willis¹, B. Willke^8,9, M. H. Wimmer^8,9, W. Winkler^8,9, C. C. Wipf¹, H. Wittel^8,9, G. Woan⁴⁴, J. Woehler^8,9, J. K. Wofford⁵⁸, J. Worden⁴⁵, J. L. Wright⁴⁴, D. S. Wu^8,9, D. M. Wysocki⁵⁸, L. Xiao¹, H. Yamamoto¹, C. C. Yancey⁷⁶, L. Yang¹¹⁴, M. J. Yap²¹, M. Yazback⁴⁸, D. W. Yeeles⁶⁸, Hang Yu¹², Haocun Yu¹², S. H. R. Yuen⁹¹, M. Yvert³², A. K. Zadrożny^104,144, M. Zanolin³³, T. Zelenova²⁸, J.-P. Zendri⁵², M. Zevin⁵⁹, J. Zhang⁶³, L. Zhang¹, T. Zhang⁴⁴, C. Zhao⁶³, M. Zhou⁵⁹, Z. Zhou⁵⁹, X. J. Zhu⁶, M. E. Zucker^1,12, J. Zweizig¹, The LIGO Scientific Collaboration and the Virgo Collaboration, Z. Arzoumanian¹⁷⁸, S. Bogdanov¹⁷⁹, I. Cognard^180,181, A. Corongiu¹⁸², T. Enoto¹⁸³, P. Freire¹⁸⁴, K. C. Gendreau¹⁷⁸, L. Guillemot^180,181, A. K. Harding¹⁸⁵, F. Jankowski¹⁸⁶, M. J. Keith¹⁸⁶, M. Kerr¹⁸⁷, A. Lyne¹⁸⁶, J. Palfreyman¹⁸⁸, A. Possenti^182,189, A. Ridolfi¹⁸⁴, B. Stappers¹⁸⁶, G. Theureau^180,181,190, and P. Weltervrede¹⁸⁶

Published 2020 August 26 • © 2020. The American Astronomical Society. All rights reserved.
The Astrophysical Journal, Volume 899, Number 2 Citation B. P. Abbott et al 2020 ApJ 899 170 DOI 10.3847/1538-4357/abaabb

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¹ LIGO, California Institute of Technology, Pasadena, CA 91125, USA

² Louisiana State University, Baton Rouge, LA 70803, USA

³ Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India

⁴ Università di Salerno, Fisciano, I-84084 Salerno, Italy

⁵ INFN, Sezione di Napoli, Complesso Universitario di Monte S.Angelo, I-80126 Napoli, Italy

⁶ OzGrav, School of Physics & Astronomy, Monash University, Clayton 3800, Victoria, Australia

⁷ LIGO Livingston Observatory, Livingston, LA 70754, USA

⁸ Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany

⁹ Leibniz Universität Hannover, D-30167 Hannover, Germany

¹⁰ University of Cambridge, Cambridge CB2 1TN, UK

¹¹ University of Birmingham, Birmingham B15 2TT, UK

¹² LIGO, Massachusetts Institute of Technology, Cambridge, MA 02139, USA

¹³ Instituto Nacional de Pesquisas Espaciais, 12227-010 Sao José dos Campos, Sao Paulo, Brazil

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¹⁶ International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India

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²³ University of Wisconsin-Milwaukee, Milwaukee, WI 53201, USA

²⁴ SUPA, University of Strathclyde, Glasgow G1 1XQ, UK

²⁵ LAL, Univ. Paris-Sud, CNRS/IN2P3, Université Paris-Saclay, F-91898 Orsay, France

²⁶ California State University Fullerton, Fullerton, CA 92831, USA

²⁷ APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS/IN2P3, CEA/Irfu, Observatoire de Paris, Sorbonne Paris Cité, F-75205 Paris Cedex 13, France

²⁸ European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy

²⁹ Università di Roma Tor Vergata, I-00133 Roma, Italy

³⁰ INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy

³¹ INFN, Sezione di Roma, I-00185 Roma, Italy

³² Laboratoire d'Annecy de Physique des Particules (LAPP), Univ. Grenoble Alpes, Université Savoie Mont Blanc, CNRS/IN2P3, F-74941 Annecy, France

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³⁷ Korea Institute of Science and Technology Information, Daejeon 34141, Republic of Korea

³⁸ OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia

³⁹ West Virginia University, Morgantown, WV 26506, USA

⁴⁰ Università di Perugia, I-06123 Perugia, Italy

⁴¹ INFN, Sezione di Perugia, I-06123 Perugia, Italy

⁴² Syracuse University, Syracuse, NY 13244, USA

⁴³ University of Minnesota, Minneapolis, MN 55455, USA

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⁴⁵ LIGO Hanford Observatory, Richland, WA 99352, USA

⁴⁶ Caltech CaRT, Pasadena, CA 91125, USA

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⁵⁸ Rochester Institute of Technology, Rochester, NY 14623, USA

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⁶⁰ INFN, Sezione di Genova, I-16146 Genova, Italy

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⁶² Faculty of Physics, Lomonosov Moscow State University, Moscow 119991, Russia

⁶³ OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia

⁶⁴ Department of Astrophysics/IMAPP, Radboud University Nijmegen, P.O. Box 9010, 6500 GL Nijmegen, The Netherlands

⁶⁵ Artemis, Université Côte d'Azur, Observatoire Côte d'Azur, CNRS, CS 34229, F-06304 Nice Cedex 4, France

⁶⁶ Physik-Institut, University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland

⁶⁷ Univ Rennes, CNRS, Institut FOTON—UMR6082, F-3500 Rennes, France

⁶⁸ Cardiff University, Cardiff CF24 3AA, UK

⁶⁹ Washington State University, Pullman, WA 99164, USA

⁷⁰ University of Oregon, Eugene, OR 97403, USA

⁷¹ Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France

⁷² Universit'`a degli Studi di Urbino "Carlo Bo," I-61029 Urbino, Italy

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⁷⁴ Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland

⁷⁵ VU University Amsterdam, 1081 HV Amsterdam, The Netherlands

⁷⁶ University of Maryland, College Park, MD 20742, USA

⁷⁷ School of Physics, Georgia Institute of Technology, Atlanta, GA 30332, USA

⁷⁸ Université Claude Bernard Lyon 1, F-69622 Villeurbanne, France

⁷⁹ Università di Napoli "Federico II," Complesso Universitario di Monte S.Angelo, I-80126 Napoli, Italy

⁸⁰ NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA

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⁹⁰ University of Chicago, Chicago, IL 60637, USA

⁹¹ The Chinese University of Hong Kong, Shatin, NT, Hong Kong

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¹⁵⁸ Indian Institute of Technology Madras, Chennai 600036, India

¹⁵⁹ INFN Sezione di Torino, Via P. Giuria 1, I-10125 Torino, Italy

¹⁶⁰ Institut des Hautes Etudes Scientifiques, F-91440 Bures-sur-Yvette, France

¹⁶¹ IISER-Kolkata, Mohanpur, West Bengal 741252, India

¹⁶² Whitman College, 345 Boyer Avenue, Walla Walla, WA 99362, USA

¹⁶³ Université de Lyon, F-69361 Lyon, France

¹⁶⁴ Hobart and William Smith Colleges, Geneva, NY 14456, USA

¹⁶⁵ Janusz Gil Institute of Astronomy, University of Zielona Góra, 65-265 Zielona Góra, Poland

¹⁶⁶ University of Washington, Seattle, WA 98195, USA

¹⁶⁷ SUPA, University of the West of Scotland, Paisley PA1 2BE, UK

¹⁶⁸ Indian Institute of Technology, Gandhinagar Ahmedabad Gujarat 382424, India

¹⁶⁹ Université de Montréal/Polytechnique, Montreal, QC H3T 1J4, Canada

¹⁷⁰ Indian Institute of Technology Hyderabad, Sangareddy, Khandi, Telangana 502285, India

¹⁷¹ International Institute of Physics, Universidade Federal do Rio Grande do Norte, Natal RN 59078-970, Brazil

¹⁷² Villanova University, 800 Lancaster Ave., Villanova, PA 19085, USA

¹⁷³ Andrews University, Berrien Springs, MI 49104, USA

¹⁷⁴ Max Planck Institute for Gravitationalphysik (Albert Einstein Institute), D-14476 Potsdam-Golm, Germany

¹⁷⁵ Università di Siena, I-53100 Siena, Italy

¹⁷⁶ Trinity University, San Antonio, TX 78212, USA

¹⁷⁷ Van Swinderen Institute for Particle Physics and Gravity, University of Groningen, Nijenborgh 4, 9747 AG Groningen, The Netherlands

¹⁷⁸ X-Ray Astrophysics Laboratory, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA

¹⁷⁹ Columbia Astrophysics Laboratory, Columbia University, 550 West 120th Street, New York, NY 10027, USA

¹⁸⁰ Laboratoire de Physique et Chimie de l'Environnement et de l'Espace—Université d'Orléans/CNRS, F-45071 Orléans Cedex 02, France

¹⁸¹ Station de Radioastronomie de Nançay, Observatoire de Paris, CNRS/INSU, F-18330 Nançay, France

¹⁸² INAF–Osservatorio Astronomico di Cagliari, via della Scienza 5, I-09047 Selargius, Italy

¹⁸³ Hakubi Center for Advanced Research and Department of Astronomy, Kyoto University, Kyoto 606-8302, Japan

¹⁸⁴ Max-Planck-Institut für Radioastronomie, Auf dem Hügel 69, D-53121 Bonn, Germany

¹⁸⁵ Astrophysics Science Division, NASA Goddard Space Flight Center, Greenbelt, MD 20771, USA

¹⁸⁶ Jodrell Bank Centre for Astrophysics, School of Physics and Astronomy, University of Manchester, Manchester, M13 9PL, UK

¹⁸⁷ Space Science Division, Naval Research Laboratory, Washington, DC 20375-5352, USA

¹⁸⁸ Department of Physical Sciences, University of Tasmania, Private Bag 37, Hobart, Tasmania 7001, Australia

¹⁸⁹ Università di Cagliari, Dipartimento di Fisica, I-09042, Monserrato, Italy

¹⁹⁰ LUTH, Observatoire de Paris, PSL Research University, CNRS, Université Paris Diderot, Sorbonne Paris Cité, F-92195 Meudon, France

Author notes

¹⁹¹ Deceased, 2018 February.

¹⁹² Deceased, 2017 November.

¹⁹³ Deceased, 2018 July.

Dates

Received 2020 July 28
Accepted 2020 July 28
Published 2020 August 26

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Two analysis errors have been identified that affect the results for a handful of the high-value pulsars given in Table 1 of Abbott et al. (2019). One affects the Bayesian analysis for the five pulsars that glitched during the analysis period, and the other affects the 5n-vector analysis for J0711–6830. Updated results after correcting the errors are shown in Table 1, which now supersedes the results given for those pulsars in Table 1 of Abbott et al. (2019). Updated versions of figures can be seen in Figures 1–4.

**Figure 1.** Upper limits on C₂₁ and C₂₂ for 221 pulsars. The stars show the observed 95% credible upper limits on observed amplitudes for each pulsar. The solid lines show an estimate of the expected sensitivity of the searches.
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**Figure 2.** Upper limits on h₀ for 221 pulsars. The stars show the observed 95% credible upper limits on observed amplitude for each pulsar. The solid line shows an estimate of the expected sensitivity of the search. Triangles show the limits on gravitational-wave amplitude derived from each pulsar's observed spin-down.
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**Figure 3.** Histogram of ratios of upper limits on h₀ compared to the spin-down limit.
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**Figure 4.** Upper limits on mass quadrupole Q₂₂ and fiducial ellipticity ε for 221 pulsars. The filled circles show the limits as derived from the observed upper limits on the gravitational-wave amplitude h₀ assuming the canonical moment of inertia and distances. Triangles show the limits derived from each pulsar's observed spin-down. The diagonal lines show contours of equal characteristic age τ assuming that braking is entirely through gravitational-wave emission. The distributions of these limits are also show in histogram form to the right of the figure, with the filled and open histograms showing our observed limits and the spin-down limits, respectively.
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Table 1. Limits on Gravitational-wave Amplitude and Other Derived Quantities for Five High-value Pulsars from the Three Analysis Methods

Pulsar Name	f_rot	${\dot{P}}_{\mathrm{rot}}$	Distance	${h}_{0}^{\mathrm{sd}}$	Analysis	${C}_{21}^{95 \% }$	${C}_{22}^{95 \% }$	${h}_{0}^{95 \% }$	${Q}_{22}^{95 \% }$	${\varepsilon }^{95 \% }$	${h}_{0}^{95 \% }/{h}_{0}^{\mathrm{sd}}$	Statistic^a	Statistic^b
(J2000)	(Hz)	(s s⁻¹)	(kpc)		Method				(kg m²)			${}^{l=2,m=\mathrm{1,2}}$	${}^{l=2,m=2}$
J0205+6449^c	15.2	$1.9\times {10}^{-13}$	2.00 (c)	$6.9\times {10}^{-25}$	Bayesian	$2.2(1.6)\times {10}^{-24}$	$2.2(2.9)\times {10}^{-26}$	$4.5(5.7)\times {10}^{-26}$	$7.2(9.0)\times {10}^{33}$	$0.9(1.2)\times {10}^{-4}$	0.065(0.082)	−4.8(−4.7)	−2.8(−2.6)
					${ \mathcal F }$ -statistic	$2.2\times {10}^{-24}$	$4.5\times {10}^{-26}$	$8.8\times {10}^{-26}$	$1.4\times {10}^{34}$	$1.8\times {10}^{-4}$	0.13	0.71	0.26
					5n-vector	⋯	⋯	$2.9(4.5)\times {10}^{-26}$	$4.6(7.1)\times {10}^{33}$	$5.9(9.2)\times {10}^{-5}$	0.042(0.065)	⋯	0.41

J0534+2200^c	29.7	$4.2\times {10}^{-13}$	2.00	$1.4\times {10}^{-24}$	Bayesian	$8.1(5.9)\times {10}^{-26}$	$8.9(7.6)\times {10}^{-27}$	$1.9(1.5)\times {10}^{-26}$	$7.8(6.3)\times {10}^{32}$	$1.0(0.8)\times {10}^{-5}$	0.013(0.011)	−5.2(−5.3)	−2.6(−2.6)
					${ \mathcal F }$ -statistic	$1.6(1.1)\times {10}^{-25}$	$1.1(1.1)\times {10}^{-26}$	$2.2(1.3)\times {10}^{-26}$	$9.1(5.4)\times {10}^{32}$	$1.2(0.7)\times {10}^{-5}$	0.015(0.0091)	0.32(0.18)	0.65(0.87)
					5n-vector	$1.7(1.3)\times {10}^{-25}$	⋯	$2.9(2.9)\times {10}^{-26}$	$1.2(1.2)\times {10}^{33}$	$1.6(1.6)\times {10}^{-5}$	0.02(0.02)	0.70	0.45

J0711–6830^c	182.1	$1.4\times {10}^{-20}$	0.11 (b)	$1.2\times {10}^{-26}$	Bayesian	$2.6\times {10}^{-26}$	$7.0\times {10}^{-27}$	$1.5\times {10}^{-26}$	$9.3\times {10}^{29}$	$1.2\times {10}^{-8}$	1.3	−3.1	−1.9
					${ \mathcal F }$ -statistic	⋯	⋯	⋯	⋯	⋯	⋯	⋯	⋯
					5n-vector	$3.0\times {10}^{-26}$	⋯	$1.5\times {10}^{-26}$	$9.1\times {10}^{29}$	$1.2\times {10}^{-8}$	1.3	0.79	0.39

J0835–4510^c	11.2	$1.2\times {10}^{-13}$	0.29 (j)	$3.3\times {10}^{-24}$	Bayesian	$1.5(1.4)\times {10}^{-23}$	$1.3(1.0)\times {10}^{-25}$	$2.4(2.1)\times {10}^{-25}$	$1.0(0.9)\times {10}^{34}$	$1.3(1.1)\times {10}^{-4}$	0.073(0.062)	−3.3(−3.1)	−1.8(−2.1)
					${ \mathcal F }$ -statistic	$1.3(1.1)\times {10}^{-23}$	$1.1(0.9)\times {10}^{-25}$	$2.6(2.0)\times {10}^{-25}$	$1.1(0.8)\times {10}^{34}$	$1.4(1.1)\times {10}^{-4}$	0.078(0.06)	0.75(0.75)	0.75(0.75)
					5n-vector	⋯	⋯	$2.3(2.4)\times {10}^{-25}$	$9.7(9.9)\times {10}^{33}$	$1.3(1.3)\times {10}^{-4}$	0.07(0.071)	⋯	0.41

J1028–5819	10.9	$1.6\times {10}^{-14}$	1.42 (b)	$2.4\times {10}^{-25}$	Bayesian	$2.0\times {10}^{-23}$	$1.0\times {10}^{-25}$	$2.4\times {10}^{-25}$	$5.2\times {10}^{34}$	$6.7\times {10}^{-4}$	1	−3.8	−2.2
					${ \mathcal F }$ -statistic	⋯	⋯	⋯	⋯	⋯	⋯	⋯	⋯
					5n-vector	⋯	⋯	$1.9\times {10}^{-25}$	$4.1\times {10}^{34}$	$5.3\times {10}^{-4}$	0.8	⋯	0.40

J1718–3825	13.4	$1.3\times {10}^{-14}$	3.49 (b)	$9.7\times {10}^{-26}$	Bayesian	$3.2\times {10}^{-24}$	$3.7\times {10}^{-26}$	$7.8\times {10}^{-26}$	$2.8\times {10}^{34}$	$3.6\times {10}^{-4}$	0.8	−5.7	−2.5
					${ \mathcal F }$ -statistic	⋯	⋯	⋯	⋯	⋯	⋯	⋯	⋯
					5n-vector	⋯	⋯	$6.5\times {10}^{-26}$	$2.3\times {10}^{34}$	$3.0\times {10}^{-4}$	0.67	⋯	0.67

Notes. For references and other notes see Table 2 in Abbott et al. (2019). Values in parentheses are those produced using the restricted orientation priors described in Section 2.2.4 of Abbott et al. (2019).

^aFor the Bayesian method this column shows the base-10 logarithm of the Bayesian odds, ${ \mathcal O }$ ${ \mathcal O }$ , comparing a coherent signal model at both the l = 2, m = 1, 2 modes to incoherent signal models. For the ${ \mathcal F }-/{ \mathcal G }$ ${ \mathcal F }-/{ \mathcal G }$ -statistic method this column shows the false-alarm probability for a signal just at the l = 2, m = 1 mode, assuming that the $2{ \mathcal F }$ $2{ \mathcal F }$ value has a χ² distribution with 4 degrees of freedom and the $2{ \mathcal G }$ $2{ \mathcal G }$ value has a χ² distribution with 2 degrees of freedom. For the 5n-vector method this column shows the p-value for a search for a signal at just the l = 2, m = 1 mode, where the null hypothesis being tested is that the data are consistent with pure Gaussian noise. ^bThis is the same as in footnote a, but for all the methods the assumed signal model is from the l = m = 2 mode. ^cThe observed $\dot{P}$ $\dot{P}$ has been corrected to account for the relative motion between the pulsar and observer.

Only a portion of this table is shown here to demonstrate its form and content. A machine-readable version of the full table is available.

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Bayesian analysis.—For the glitching pulsars, the signal phase evolution caused by the glitch was wrongly applied twice and was therefore not consistent with our expected model of the pulsar phase. This error did not affect the ${ \mathcal F }/{ \mathcal G }$ -statistic or 5n-vector analysis.

Analyses of the five pulsars PSR J0205+6449, PSR J0534+2200, PSR J0835–4510, PSR J1028–5819, and PSR J1718–3825 have been repeated after correcting for the error. There are small quantitative differences in the results, but the changes do not affect the main conclusions of the paper. The largest differences are for PSR J0835–4510 (the Vela pulsar), for which the updated upper limits from the Bayesian method are found to be between 1.1 and 2 times larger than those obtained when the error was present. This appears primarily to be due to the error leading to the decohering of a strong spectral line in the LIGO Livingston detector and thus lowering the amplitude limit.

5n-vector analysis.—An error was also identified in the settings of the 5n-vector analysis, which affected the upper limit computation at the rotation frequency for ${C}_{21}^{95 \% }$ of J0711–6830. Specifically, we found an incorrect choice for the range of amplitudes used to inject simulated signals in the O2 data. The updated upper limit is about 2.5 times worse than that obtained when the error was present. This error did not affect the Bayesian or ${ \mathcal F }/{ \mathcal G }$ -statistic results.

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