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Black Hole Spectroscopy and Tests of General Relativity with GW250114

A. G. Abac1, I. Abouelfettouh2, F. Acernese3,4, K. Ackley5, C. Adamcewicz6, S. Adhicary7, D. Adhikari8,9, N. Adhikari10, R. X. Adhikari11 et al. (The LIGO Scientific Collaboration, The Virgo Collaboration, and The KAGRA Collaboration†)

R. X. Adhikari11, V. K. Adkins12, S. Afroz13, A. Agapito14, D. Agarwal15, M. Agathos16, N. Aggarwal17, S. Aggarwal18, O. D. Aguiar19, I.-L. Ahrend20, L. Aiello21,22, A. Ain23, P. Ajith24, T. Akutsu25,26, S. Albanesi27,28, W. Ali29,30, S. Al-Kershi8,9, C. Alléné31, A. Allocca32,4, S. Al-Shammari33, P. A. Altin34, S. Alvarez-Lopez35, W. Amar31, O. Amarasinghe33, A. Amato36,37, F. Amicucci38,39, C. Amra40, A. Ananyeva11, S. B. Anderson11, W. G. Anderson11, M. Andia41, M. Ando42, M. Andrés-Carcasona43, T. Andrić44,45,8,9, J. Anglin46, S. Ansoldi47,48, J. M. Antelis49, S. Antier41, M. Aoumi50, E. Z. Appavuravther51,52, S. Appert11, S. K. Apple53, K. Arai11, A. Araya42, M. C. Araya11, M. Arca Sedda44,45, J. S. Areeda54, N. Aritomi2, F. Armato29,30, S. Armstrong55, N. Arnaud56, M. Arogeti57, S. M. Aronson12, K. G. Arun58, G. Ashton59, Y. Aso25,60, L. Asprea28, M. Assiduo61,62, S. Assis de Souza Melo63, S. M. Aston64, P. Astone38, F. Attadio39,38, F. Aubin65, K. AultONeal66, G. Avallone67, E. A. Avila49, S. Babak20, C. Badger68, S. Bae69, S. Bagnasco28, L. Baiotti70, R. Bajpai71, T. Baka72,37, A. M. Baker6, K. A. Baker73, T. Baker74, G. Baldi75,76, N. Baldicchi77,51, M. Ball78, G. Ballardin63, S. W. Ballmer79, S. Banagiri6, B. Banerjee44, D. Bankar80, T. M. Baptiste12, P. Baral10, M. Baratti81,82, J. C. Barayoga11, B. C. Barish11, D. Barker2, N. Barman80, P. Barneo83,84,85, F. Barone86,4, B. Barr87, L. Barsotti35, M. Barsuglia20, D. Barta88, A. M. Bartoletti89, M. A. Barton87, I. Bartos46, A. Basalaev8,9, R. Bassiri90, A. Basti82,81, M. Bawaj77,51, P. Baxi91, J. C. Bayley87, A. C. Baylor10, P. A. Baynard, II57, M. Bazzan92,93, V. M. Bedakihale94, F. Beirnaert95, M. Bejger96, D. Belardinelli22, A. S. Bell87, D. S. Bellie97, L. Bellizzi81,82, W. Benoit18, I. Bentara56, J. D. Bentley98, M. Ben Yaala55, S. Bera99,100, F. Bergamin33, B. K. Berger90, S. Bernuzzi27, M. Beroiz11, C. P. L. Berry87, D. Bersanetti29, T. Bertheas101, A. Bertolini37,36, J. Betzwieser64, D. Beveridge73, G. Bevilacqua102, N. Bevins103, S. Bhagwat119, R. Bhandare104, R. Bhatt11, D. Bhattacharjee105,106, S. Bhattacharyya107, S. Bhaumik46, V. Biancalana102, A. Bianchi37,108, I. A. Bilenko109, G. Billingsley11, A. Binetti110, S. Bini11,75,76, C. Binu111, S. Biot112, O. Birnholtz113, S. Biscoveanu97, A. Bisht9, M. Bitossi63,81, M.-A. Bizouard114, S. Blaber115, J. K. Blackburn11, L. A. Blagg78, C. D. Blair73,64, D. G. Blair73, N. Bode8,9, N. Boettner98, G. Boileau114, M. Boldrini38, G. N. Bolingbroke116, A. Bolliand117,40, L. D. Bonavena46, R. Bondarescu83, F. Bondu118, E. Bonilla90, M. S. Bonilla54, A. Bonino119, R. Bonnand31,117, A. Borchers8,9, S. Borhanian7, V. Boschi81, S. Bose120, V. Bossilkov64, Y. Bothra37,108, A. Boudon56, L. Bourg57, M. Boyle121, A. Bozzi63, C. Bradaschia81, P. R. Brady10, A. Branch64, M. Branchesi44,45, I. Braun105, T. Briant122, A. Brillet114, M. Brinkmann8,9, P. Brockill10, E. Brockmueller8,9, A. F. Brooks11, B. C. Brown46, D. D. Brown116, M. L. Brozzetti77,51, S. Brunett11, G. Bruno15, R. Bruntz123, J. Bryant119, Y. Bu124, F. Bucci62, J. Buchanan123, O. Bulashenko83,84, T. Bulik125, H. J. Bulten37, A. Buonanno126,1, K. Burtnyk2, R. Buscicchio127,128, D. Buskulic31, C. Buy101, R. L. Byer90, G. S. Cabourn Davies74, R. Cabrita15, V. Cáceres-Barbosa7, L. Cadonati57, G. Cagnoli129, C. Cahillane79, A. Calafat99, T. A. Callister130, E. Calloni32,4, S. R. Callos78, G. Caneva Santoro43, K. C. Cannon42, H. Cao35, L. A. Capistran131, E. Capocasa20, E. Capote2,11, G. Capurri82,81, G. Carapella67,132, F. Carbognani63, M. Carlassara8,9, J. B. Carlin124, T. K. Carlson133, M. F. Carney105, M. Carpinelli127,63, G. Carrillo78, J. J. Carter8,9, G. Carullo119,134, A. Casallas-Lagos135, J. Casanueva Diaz63, C. Casentini136,22, S. Y. Castro-Lucas137, S. Caudill133, M. Cavaglià106, R. Cavalieri63, A. Ceja54, G. Cella81, P. Cerdá-Durán138,139, E. Cesarini22, N. Chabbra34, W. Chaibi114, A. Chakraborty13, P. Chakraborty8,9, S. Chakraborty104, S. Chalathadka Subrahmanya98, J. C. L. Chan140, M. Chan115, K. Chandra7, K. Chang141, S. Chao142,141, P. Charlton143, E. Chassande-Mottin20, C. Chatterjee144, Debarati Chatterjee80, Deep Chatterjee35, M. Chaturvedi104, S. Chaty20, A. Chen145, A. H.-Y. Chen146, D. Chen147, H. Chen142, H. Y. Chen148, S. Chen144, Yanbei Chen149, Yitian Chen121, H. P. Cheng150, P. Chessa77,51, H. T. Cheung91, S. Y. Cheung6, F. Chiadini151,132, G. Chiarini8,9,93, A. Chiba152, A. Chincarini29, M. L. Chiofalo82,81, A. Chiummo4,63, C. Chou146, S. Choudhary73, N. Christensen114,153, S. S. Y. Chua34, G. Ciani75,76, P. Ciecielag96, M. Cieślar125, M. Cifaldi22, B. Cirok154, F. Clara2, A. Clark119, J. A. Clark11,57, T. A. Clarke6, P. Clearwater155, S. Clesse112, F. Cleva114,117, E. Coccia44,45,43, E. Codazzo156,157, P.-F. Cohadon122, S. Colace30, E. Colangeli74, M. Colleoni99, C. G. Collette158, J. Collins64, S. Colloms87, A. Colombo159,128, C. M. Compton2, G. Connolly78, L. Conti93, T. R. Corbitt12, I. Cordero-Carrión160, S. Corezzi77,51, M. Corman1, N. J. Cornish161, I. Coronado162, A. Corsi163, R. Cottingham64, M. W. Coughlin18, A. Couineaux38, P. Couvares11,57, D. M. Coward73, R. Coyne164, A. Cozzumbo44, J. D. E. Creighton10, T. D. Creighton165, P. Cremonese99, S. Crook64, R. Crouch2, J. Csizmazia2, J. R. Cudell166, T. J. Cullen11, A. Cumming87, E. Cuoco167,168, M. Cusinato138, L. V. Da Conceição169, T. Dal Canton41, S. Dal Pra170, G. Dálya101, B. D’Angelo29, S. Danilishin36,37, S. D’Antonio38, K. Danzmann9,8,9, K. E. Darroch123, L. P. Dartez64, R. Das107, A. Dasgupta94, V. Dattilo63, A. Daumas20, N. Davari171,172, I. Dave104, A. Davenport137, M. Davier41, T. F. Davies73, D. Davis11, L. Davis73, M. C. Davis18, P. Davis173,174, E. J. Daw175, M. Dax1, J. De Bolle95, M. Deenadayalan80, J. Degallaix176, M. De Laurentis32,4, F. De Lillo23, S. Della Torre128, W. Del Pozzo82,81, A. Demagny31, F. De Marco39,38, G. Demasi177,62, F. De Matteis21,22, N. Demos35, T. Dent178, A. Depasse15, N. DePergola103, R. De Pietri179,180, R. De Rosa32,4, C. De Rossi63, M. Desai35, R. DeSalvo181, A. DeSimone182, R. De Simone151,132, A. Dhani1, R. Diab46, M. C. Díaz165, M. Di Cesare32,4, G. Dideron183, T. Dietrich1, L. Di Fiore4, C. Di Fronzo73, M. Di Giovanni39,38, T. Di Girolamo32,4, D. Diksha37,36, J. Ding20,184, S. Di Pace39,38, I. Di Palma39,38, D. Di Piero185,48, F. Di Renzo56, Divyajyoti33, A. Dmitriev119, J. P. Docherty87, Z. Doctor97, N. Doerksen169, E. Dohmen2, A. Doke133, A. Domiciano De Souza186, L. D’Onofrio38, F. Donovan35, K. L. Dooley33, T. Dooney72, S. Doravari80, O. Dorosh187, W. J. D. Doyle123, M. Drago39,38, J. C. Driggers2, L. Dunn124, U. Dupletsa44, P.-A. Duverne20, D. D’Urso171,156, P. Dutta Roy46, H. Duval188, S. E. Dwyer2, C. Eassa2, W. E. East183, M. Ebersold189,31, T. Eckhardt98, G. Eddolls79, A. Effler64, J. Eichholz34, H. Einsle114, M. Eisenmann25, M. Emma59, K. Endo152, R. Enficiaud1, L. Errico32,4, R. Espinosa165, M. Esposito4,32, R. C. Essick190, H. Estellés1, T. Etzel11, M. Evans35, T. Evstafyeva183, B. E. Ewing7, J. M. Ezquiaga140, F. Fabrizi61,62, V. Fafone21,22, S. Fairhurst33, A. M. Farah130, B. Farr78, W. M. Farr191,192, G. Favaro92, M. Favata193, M. Fays166, M. Fazio55, J. Feicht11, M. M. Fejer90, R. Felicetti185,48, E. Fenyvesi88,194, J. Fernandes195, T. Fernandes196,138, D. Fernando111, S. Ferraiuolo197,39,38, T. A. Ferreira12, F. Fidecaro82,81, P. Figura96, E. Finch11, A. Fiori81,82, I. Fiori63, M. Fishbach190, R. P. Fisher123, R. Fittipaldi198,132, V. Fiumara199,132, R. Flaminio31, S. M. Fleischer200, L. S. Fleming201, E. Floden18, H. Fong115, J. A. Font138,139, F. Fontinele-Nunes18, C. Foo1, B. Fornal202, K. Franceschetti179, N. Franchini320, F. Frappez31, S. Frasca39,38, F. Frasconi81, J. P. Freed66, Z. Frei203, A. Freise37,108, O. Freitas196,138, R. Frey78, W. Frischhertz64, P. Fritschel35, V. V. Frolov64, G. G. Fronzé28, M. Fuentes-Garcia11, S. Fujii204, T. Fujimori205, P. Fulda46, M. Fyffe64, B. Gadre72, J. R. Gair1, S. Galaudage186, V. Galdi206, R. Gamba7, A. Gamboa1, S. Gamoji181, D. Ganapathy207, A. Ganguly80, B. Garaventa29, J. García-Bellido208, C. García-Quirós189, J. W. Gardner34, K. A. Gardner115, S. Garg42, J. Gargiulo63, X. Garrido41, A. Garron99, F. Garufi32,4, P. A. Garver90, C. Gasbarra21,22, B. Gateley2, F. Gautier209, V. Gayathri10, T. Gayer79, G. Gemme29, A. Gennai81, V. Gennari101, J. George104, R. George148, O. Gerberding98, L. Gergely154, Archisman Ghosh95, Sayantan Ghosh195, Shaon Ghosh193, Shrobana Ghosh8,9, Suprovo Ghosh210, Tathagata Ghosh80, J. A. Giaime12,64, K. D. Giardina64, D. R. Gibson201, C. Gier55, S. Gkaitatzis82,81, J. Glanzer11, F. Glotin41, J. Godfrey78, R. V. Godley8,9, P. Godwin11, A. S. Goettel33, E. Goetz115, J. Golomb11, S. Gomez Lopez39,38, B. Goncharov44, G. González12, P. Goodarzi211, S. Goode6, A. W. Goodwin-Jones15, M. Gosselin63, R. Gouaty31, D. W. Gould34, K. Govorkova35, A. Grado77,51, V. Graham87, A. E. Granados18, M. Granata176, V. Granata212,132, S. Gras35, P. Grassia11, J. Graves57, C. Gray2, R. Gray87, G. Greco51, A. C. Green37,108, L. Green213, S. M. Green74, S. R. Green214, C. Greenberg133, A. M. Gretarsson66, H. K. Griffin18, D. Griffith11, H. L. Griggs57, G. Grignani77,51, C. Grimaud31, H. Grote33, S. Grunewald1, D. Guerra138, D. Guetta215, G. M. Guidi61,62, A. R. Guimaraes12, H. K. Gulati94, F. Gulminelli173,174, H. Guo145, W. Guo73, Y. Guo37,36, Anuradha Gupta216, I. Gupta7, N. C. Gupta94, S. K. Gupta46, V. Gupta18, N. Gupte1, J. Gurs98, N. Gutierrez176, N. Guttman6, F. Guzman131, D. Haba217, M. Haberland1, S. Haino218, E. D. Hall35, E. Z. Hamilton99, G. Hammond87, M. Haney37, J. Hanks2, C. Hanna7, M. D. Hannam33, O. A. Hannuksela219, A. G. Hanselman130, H. Hansen2, J. Hanson64, S. Hanumasagar57, R. Harada42, A. R. Hardison182, S. Harikumar187, K. Haris37,72, I. Harley-Trochimczyk131, T. Harmark134, J. Harms44,45, G. M. Harry220, I. W. Harry74, J. Hart105, B. Haskell96,221,222, C. J. Haster213, K. Haughian87, H. Hayakawa50, K. Hayama223, M. C. Heintze64, J. Heinze119, J. Heinzel35, H. Heitmann114, F. Hellman207, A. F. Helmling-Cornell78, G. Hemming63, O. Henderson-Sapir116, M. Hendry87, I. S. Heng87, M. H. Hennig87, C. Henshaw57, M. Heurs8,9, A. L. Hewitt224,225, J. Heynen15, J. Heyns35, S. Higginbotham33, S. Hild36,37, S. Hill87, Y. Himemoto226, N. Hirata25, C. Hirose227, D. Hofman176, B. E. Hogan66, N. A. Holland37,108, I. J. Hollows175, D. E. Holz130, L. Honet112, D. J. Horton-Bailey207, J. Hough87, S. Hourihane11, N. T. Howard144, E. J. Howell73, C. G. Hoy74, C. A. Hrishikesh21, P. Hsi35, H.-F. Hsieh142, H.-Y. Hsieh142, C. Hsiung228, S.-H. Hsu146, W.-F. Hsu110, Q. Hu87, H. Y. Huang141, Y. Huang7, Y. T. Huang79, A. D. Huddart229, B. Hughey66, V. Hui31, S. Husa99, R. Huxford7, L. Iampieri39,38, G. A. Iandolo36, M. Ianni22,21, G. Iannone132, J. Iascau78, K. Ide230, R. Iden217, A. Ierardi44,45, S. Ikeda147, H. Imafuku42, Y. Inoue141, G. Iorio92, P. Iosif185,48, M. H. Iqbal34, J. Irwin87, R. Ishikawa230, M. Isi192, K. S. Isleif231,321, Y. Itoh205,232, M. Iwaya204, B. R. Iyer24, C. Jacquet101, P.-E. Jacquet122, T. Jacquot41, S. J. Jadhav233, S. P. Jadhav155, M. Jain133, T. Jain224, A. L. James11, K. Jani144, J. Janquart15, N. N. Janthalur233, S. Jaraba234, P. Jaranowski235, R. Jaume99, W. Javed33, A. Jennings2, M. Jensen2, W. Jia35, J. Jiang150, H.-B. Jin236,237, G. R. Johns123, N. A. Johnson46, N. Johnson-McDaniel216, M. C. Johnston213, R. Johnston87, N. Johny8,9, D. H. Jones34, D. I. Jones210, R. Jones87, H. E. Jose78, P. Joshi7, S. K. Joshi80, G. Joubert56, J. Ju238, L. Ju73, K. Jung239, J. Junker34, V. Juste112, H. B. Kabagoz64,35, T. Kajita240, I. Kaku205, V. Kalogera97, M. Kalomenopoulos213, M. Kamiizumi50, N. Kanda232,205, S. Kandhasamy80, G. Kang241, N. C. Kannachel6, J. B. Kanner11, S. A. KantiMahanty18, S. J. Kapadia80, D. P. Kapasi54, M. Karthikeyan133, M. Kasprzack11, H. Kato152, T. Kato204, E. Katsavounidis35, W. Katzman64, R. Kaushik104, K. Kawabe2, R. Kawamoto205, D. Keitel99, L. J. Kemperman116, J. Kennington7, F. A. Kerkow18, R. Kesharwani80, J. S. Key242, R. Khadela8,9, S. Khadka90, S. S. Khadkikar7, F. Y. Khalili109, F. Khan8,9, T. Khanam163, M. Khursheed104, N. M. Khusid191,192, W. Kiendrebeogo114,243, N. Kijbunchoo116, C. Kim244, J. C. Kim245, K. Kim246, M. H. Kim238, S. Kim247, Y.-M. Kim246, C. Kimball97, K. Kimes54, M. Kinnear33, J. S. Kissel2, S. Klimenko46, A. M. Knee115, E. J. Knox78, N. Knust8,9, K. Kobayashi204, S. M. Koehlenbeck90, G. Koekoek37,36, K. Kohri248,249, K. Kokeyama33,250, S. Koley44,166, P. Kolitsidou119, A. E. Koloniari251, K. Komori42, A. K. H. Kong142, A. Kontos252, L. M. Koponen119, M. Korobko98, X. Kou18, A. Koushik23, N. Kouvatsos68, M. Kovalam73, T. Koyama152, D. B. Kozak11, S. L. Kranzhoff36,37, V. Kringel8,9, N. V. Krishnendu119, S. Kroker253, A. Królak254,187, K. Kruska8,9, J. Kubisz255, G. Kuehn8,9, S. Kulkarni216, A. Kulur Ramamohan34, Achal Kumar46, Anil Kumar233, Praveen Kumar178, Prayush Kumar24, Rahul Kumar2, Rakesh Kumar94, J. Kume256,257,42, K. Kuns35, N. Kuntimaddi33, S. Kuroyanagi208,258, S. Kuwahara42, K. Kwak239, K. Kwan34, S. Kwon42, G. Lacaille87, D. Laghi189,101, A. H. Laity164, E. Lalande259, M. Lalleman23, P. C. Lalremruati260, M. Landry2, B. B. Lane35, R. N. Lang35, J. Lange148, R. Langgin213, B. Lantz90, I. La Rosa99, J. Larsen200, A. Lartaux-Vollard41, P. D. Lasky6, J. Lawrence165, M. Laxen64, C. Lazarte138, A. Lazzarini11, C. Lazzaro157,156, P. Leaci39,38, L. Leali18, Y. K. Lecoeuche115, H. M. Lee261, H. W. Lee262, J. Lee79, K. Lee238, R.-K. Lee142, R. Lee35, Sungho Lee246, Sunjae Lee238, Y. Lee141, I. N. Legred11, J. Lehmann8,9, L. Lehner183, M. Le Jean176,117, A. Lemaître263, M. Lenti62,177, M. Leonardi75,76,264, M. Lequime40, N. Leroy41, M. Lesovsky11, N. Letendre31, M. Lethuillier56, Y. Levin6, K. Leyde74, A. K. Y. Li11, K. L. Li265, T. G. F. Li110, X. Li149, Y. Li97, Z. Li87, A. Lihos123, E. T. Lin142, F. Lin141, L. C.-C. Lin265, Y.-C. Lin142, C. Lindsay201, S. D. Linker181, A. Liu219, G. C. Liu228, Jian Liu73, F. Llamas Villarreal165, J. Llobera-Querol99, R. K. L. Lo140, J.-P. Locquet110, S. C. G. Loggins266, M. R. Loizou133, L. T. London68, A. Longo61,62, D. Lopez166, M. Lopez Portilla72, A. Lorenzo-Medina178, V. Loriette41, M. Lormand64, G. Losurdo267,81, E. Lotti133, T. P. Lott, IV57, J. D. Lough8,9, H. A. Loughlin35, C. O. Lousto111, N. Low124, N. Lu34, L. Lucchesi81, H. Lück9,8,9, D. Lumaca22, A. P. Lundgren268,269, A. W. Lussier259, S. Ma183, R. Macas74, M. MacInnis35, D. M. Macleod33, I. A. O. MacMillan11, A. Macquet41, K. Maeda152, S. Maenaut110, S. S. Magare80, R. M. Magee11, E. Maggio1, R. Maggiore37,108, M. Magnozzi29,30, P. Mahapatra33, M. Mahesh98, M. Maini164, S. Majhi80, E. Majorana39,38, C. N. Makarem11, D. Malakar106, J. A. Malaquias-Reis19, U. Mali190, S. Maliakal11, A. Malik104, L. Mallick169,190, A.-K. Malz59, N. Man114, M. Mancarella100, V. Mandic18, V. Mangano171,156, B. Mannix78, G. L. Mansell79, M. Manske10, M. Mantovani63, M. Mapelli92,93,270, C. Marinelli102, F. Marion31, A. S. Markosyan90, A. Markowitz11, E. Maros11, S. Marsat101, F. Martelli61,62, I. W. Martin87, R. M. Martin193, B. B. Martinez131, D. A. Martinez54, M. Martinez43,271, V. Martinez129, A. Martini75,76, J. C. Martins19, D. V. Martynov119, E. J. Marx35, L. Massaro36,37, A. Masserot31, M. Masso-Reid87, S. Mastrogiovanni38, T. Matcovich51, M. Matiushechkina8,9, L. Maurin209, N. Mavalvala35, N. Maxwell2, G. McCarrol64, R. McCarthy2, D. E. McClelland34, S. McCormick64, L. McCuller11, S. McEachin123, C. McElhenny123, G. I. McGhee87, J. McGinn87, K. B. M. McGowan144, J. McIver115, A. McLeod73, I. McMahon189, T. McRae34, R. McTeague87, D. Meacher10, B. N. Meagher79, R. Mechum111, Q. Meijer72, A. Melatos124, C. S. Menoni137, F. Mera2, R. A. Mercer10, L. Mereni176, K. Merfeld163, E. L. Merilh64, J. R. Mérou99, J. D. Merritt78, M. Merzougui114, C. Messick10, B. Mestichelli44, M. Meyer-Conde272, F. Meylahn8,9, A. Mhaske80, A. Miani75,76, H. Miao273, C. Michel176, Y. Michimura42, H. Middleton119, D. P. Mihaylov105, S. J. Miller11, M. Millhouse57, E. Milotti185,48, V. Milotti92, Y. Minenkov22, E. M. Minihan66, Ll. M. Mir43, L. Mirasola156,157, M. Miravet-Tenés138, C.-A. Miritescu43, A. Mishra24, C. Mishra107, T. Mishra46, A. L. Mitchell37,108, J. G. Mitchell66, K. Mitman121, S. Mitra80, V. P. Mitrofanov109, K. Mitsuhashi25, R. Mittleman35, O. Miyakawa50, S. Miyoki50, A. Miyoko66, G. Mo35, L. Mobilia61,62, S. R. P. Mohapatra11, S. R. Mohite7, M. Molina-Ruiz207, M. Mondin181, M. Montani61,62, C. J. Moore224, D. Moraru2, A. More80, S. More80, C. Moreno135, E. A. Moreno35, G. Moreno2, A. Moreso Serra83, S. Morisaki42,204, Y. Moriwaki152, G. Morras208, A. Moscatello92, M. Mould35, B. Mours65, C. M. Mow-Lowry37,108, L. Muccillo177,62, F. Muciaccia39,38, D. Mukherjee119, Samanwaya Mukherjee24, Soma Mukherjee165, Subroto Mukherjee94, Suvodip Mukherjee13, N. Mukund35, A. Mullavey64, H. Mullock115, J. Mundi220, C. L. Mungioli73, M. Murakoshi230, P. G. Murray87, D. Nabari75,76, S. L. Nadji8,9, A. Nagar28,274, N. Nagarajan87, K. Nakagaki50, K. Nakamura25, H. Nakano275, M. Nakano11, D. Nanadoumgar-Lacroze43, D. Nandi12, V. Napolano63, P. Narayan216, I. Nardecchia22, T. Narikawa204, H. Narola72, L. Naticchioni38, R. K. Nayak260, L. Negri72, A. Nela87, C. Nelle78, A. Nelson131, T. J. N. Nelson64, M. Nery8,9, A. Neunzert2, S. Ng54, L. Nguyen Quynh276, S. A. Nichols12, A. B. Nielsen277, Y. Nishino25,42, A. Nishizawa278, S. Nissanke279,37, W. Niu7, F. Nocera63, J. Noller280, M. Norman33, C. North33, J. Novak117,234,281, R. Nowicki144, J. F. Nuño Siles208, L. K. Nuttall74, K. Obayashi230, J. Oberling2, J. O’Dell229, E. Oelker35, M. Oertel234,117,282,281, G. Oganesyan44,45, T. O’Hanlon64, M. Ohashi50, F. Ohme8,9, R. Oliveri117,282,281, R. Omer18, B. O’Neal123, M. Onishi152, K. Oohara283, B. O’Reilly64, M. Orselli51,77, R. O’Shaughnessy111, S. O’Shea87, S. Oshino50, C. Osthelder11, I. Ota12, D. J. Ottaway116, A. Ouzriat56, H. Overmier64, B. J. Owen284, R. Ozaki230, A. E. Pace7, R. Pagano12, M. A. Page25, A. Pai195, L. Paiella44, A. Pal285, S. Pal260, M. A. Palaia81,82, M. Pálfi203, P. P. Palma39,21,22, C. Palomba38, P. Palud20, H. Pan142, J. Pan73, K. C. Pan142, P. K. Panda233, Shiksha Pandey7, Swadha Pandey35, P. T. H. Pang37,72, F. Pannarale39,38, K. A. Pannone54, B. C. Pant104, F. H. Panther73, M. Panzeri61,62, F. Paoletti81, A. Paolone38,286, A. Papadopoulos87, E. E. Papalexakis211, L. Papalini81,82, G. Papigkiotis251, A. Paquis41, A. Parisi77,51, B.-J. Park246, J. Park287, W. Parker64, G. Pascale8,9, D. Pascucci95, A. Pasqualetti63, R. Passaquieti82,81, L. Passenger6, D. Passuello81, O. Patane2, A. V. Patel141, D. Pathak80, A. Patra33, B. Patricelli82,81, B. G. Patterson33, K. Paul107, S. Paul78, E. Payne11, T. Pearce33, M. Pedraza11, A. Pele11, F. E. Peña Arellano288, X. Peng119, Y. Peng57, S. Penn289, M. D. Penuliar54, A. Perego75,76, Z. Pereira133, C. Périgois290,93,92, G. Perna92, A. Perreca75,76,44, J. Perret20, S. Perriès56, J. W. Perry37,108, D. Pesios251, S. Peters166, S. Petracca206, C. Petrillo77, H. P. Pfeiffer1, H. Pham64, K. A. Pham18, K. S. Phukon119, H. Phurailatpam219, M. Piarulli101, L. Piccari39,38, O. J. Piccinni34, M. Pichot114, M. Piendibene82,81, F. Piergiovanni61,62, L. Pierini38, G. Pierra38, V. Pierro291,132, M. Pietrzak96, M. Pillas166, F. Pilo81, L. Pinard176, I. M. Pinto291,132,292,32, M. Pinto63, B. J. Piotrzkowski10, M. Pirello2, M. D. Pitkin224,87, A. Placidi51, E. Placidi39,38, M. L. Planas99, W. Plastino212,22, C. Plunkett35, R. Poggiani82,81, E. Polini35, J. Pomper81,82, L. Pompili1, J. Poon219, E. Porcelli37, E. K. Porter20, C. Posnansky7, R. Poulton63, J. Powell155, G. S. Prabhu80, M. Pracchia166, B. K. Pradhan80, T. Pradier65, A. K. Prajapati94, V. Prasad7, K. Prasai293, R. Prasanna233, P. Prasia80, G. Pratten119, G. Principe185,48, G. A. Prodi75,76, P. Prosperi81, P. Prosposito21,22, A. C. Providence66, A. Puecher1, J. Pullin12, P. Puppo38, M. Pürrer164, H. Qi16, J. Qin34, G. Quéméner174,117, V. Quetschke165, P. J. Quinonez66, N. Qutob57, R. Rading231, I. Rainho138, S. Raja104, C. Rajan104, B. Rajbhandari111, K. E. Ramirez64, F. A. Ramis Vidal99, M. Ramos Arevalo165, A. Ramos-Buades99,37, S. Ranjan57, K. Ransom64, P. Rapagnani39,38, B. Ratto66, A. Ravichandran133, A. Ray97, V. Raymond33, M. Razzano82,81, J. Read54, T. Regimbau31, S. Reid55, C. Reissel35, D. H. Reitze11, A. I. Renzini127,11, B. Revenu294,41, A. Revilla Peña83, R. Reyes181, L. Ricca15, F. Ricci39,38, M. Ricci38,39, A. Ricciardone82,81, J. Rice79, J. W. Richardson211, M. L. Richardson116, A. Rijal66, K. Riles91, H. K. Riley33, S. Rinaldi270, J. Rittmeyer98, C. Robertson229, F. Robinet41, M. Robinson2, A. Rocchi22, L. Rolland31, J. G. Rollins11, A. E. Romano295, R. Romano3,4, A. Romero31, I. M. Romero-Shaw224, J. H. Romie64, S. Ronchini7, T. J. Roocke116, L. Rosa4,32, T. J. Rosauer211, C. A. Rose57, D. Rosińska125, M. P. Ross53, M. Rossello-Sastre99, S. Rowan87, S. K. Roy191,192, S. Roy15, D. Rozza127,128, P. Ruggi63, N. Ruhama239, E. Ruiz Morales296,208, K. Ruiz-Rocha144, S. Sachdev57, T. Sadecki2, P. Saffarieh37,108, S. Safi-Harb169, M. R. Sah13, S. Saha142, T. Sainrat65, S. Sajith Menon215,39,38, K. Sakai297, Y. Sakai272, M. Sakellariadou68, S. Sakon7, O. S. Salafia159,128,127, F. Salces-Carcoba11, L. Salconi63, M. Saleem148, F. Salemi39,38, M. Sallé37, S. U. Salunkhe80, S. Salvador174,173, A. Salvarese148, A. Samajdar72,37, A. Sanchez2, E. J. Sanchez11, L. E. Sanchez11, N. Sanchis-Gual138, J. R. Sanders182, E. M. Sänger1, F. Santoliquido44,45, F. Sarandrea28, T. R. Saravanan80, N. Sarin6, P. Sarkar8,9, A. Sasli251, P. Sassi51,77, B. Sassolas176, B. S. Sathyaprakash7,33, R. Sato227, S. Sato152, Yukino Sato152, Yu Sato152, O. Sauter46, R. L. Savage2, T. Sawada50, H. L. Sawant80, S. Sayah176, V. Scacco21,22, D. Schaetzl11, M. Scheel149, A. Schiebelbein190, M. G. Schiworski79, P. Schmidt119, S. Schmidt72, R. Schnabel98, M. Schneewind8,9, F. Schiettekatte259, R. M. S. Schofield78, K. Schouteden110, B. W. Schulte8,9, B. F. Schutz33,8,9, E. Schwartz298, M. Scialpi299, J. Scott87, S. M. Scott34, R. M. Sedas64, T. C. Seetharamu87, M. Seglar-Arroyo43, Y. Sekiguchi300, D. Sellers64, N. Sembo205, A. S. Sengupta301, E. G. Seo87, J. W. Seo110, V. Sequino32,4, M. Serra38, A. Sevrin188, T. Shaffer2, U. S. Shah57, M. A. Shaikh261, L. Shao302, A. K. Sharma99, Preeti Sharma12, Prianka Sharma104, Ritwik Sharma18, S. Sharma Chaudhary106, P. Shawhan126, N. S. Shcheblanov303,263, E. Sheridan144, Z.-H. Shi142, M. Shikauchi42, R. Shimomura304, H. Shinkai304, S. Shirke80, D. H. Shoemaker35, D. M. Shoemaker148, R. W. Short2, S. ShyamSundar104, A. Sider158, H. Siegel191,192, D. Sigg2, L. Silenzi36,37, L. Silvestri39,170, M. Simmonds116, L. P. Singer305, Amitesh Singh216, Anika Singh11, D. Singh207, N. Singh99, S. Singh217,60, A. M. Sintes99, V. Sipala171,156, V. Skliris33, B. J. J. Slagmolen34, D. A. Slater200, T. J. Slaven-Blair73, J. Smetana119, J. R. Smith54, L. Smith87,185,48, R. J. E. Smith6, W. J. Smith144, S. Soares de Albuquerque Filho61, M. Soares-Santos189, K. Somiya217, I. Song142, S. Soni35, V. Sordini56, F. Sorrentino29, H. Sotani306, F. Spada81, V. Spagnuolo37, A. P. Spencer87, P. Spinicelli63, A. K. Srivastava94, F. Stachurski87, C. J. Stark123, D. A. Steer307, N. Steinle169, J. Steinlechner36,37, S. Steinlechner36,37, N. Stergioulas251, P. Stevens41, S. P. Stevenson155, M. StPierre164, M. D. Strong12, A. Strunk2, A. L. Stuver103,‡, M. Suchenek96, S. Sudhagar96, Y. Sudo230, N. Sueltmann98, L. Suleiman54, K. D. Sullivan12, J. Sun241, L. Sun34, S. Sunil94, J. Suresh114, B. J. Sutton68, P. J. Sutton33, K. Suzuki217, M. Suzuki204, S. N. Swain119, B. L. Swinkels37, A. Syx117, M. J. Szczepańczyk308, P. Szewczyk125, M. Tacca37, H. Tagoshi204, K. Takada204, H. Takahashi272, R. Takahashi25, A. Takamori42, S. Takano309, H. Takeda310,311, K. Takeshita217, I. Takimoto Schmiegelow44,45, M. Takou-Ayaoh79, C. Talbot130, M. Tamaki204, N. Tamanini101, D. Tanabe141, K. Tanaka50, S. J. Tanaka230, S. Tanioka33, D. B. Tanner46, W. Tanner8,9, L. Tao211, R. D. Tapia7, E. N. Tapia San Martín37, C. Taranto21,22, A. Taruya312, J. D. Tasson153, J. G. Tau111, D. Tellez54, R. Tenorio99, H. Themann181, A. Theodoropoulos138, M. P. Thirugnanasambandam80, L. M. Thomas11, M. Thomas64, P. Thomas2, J. E. Thompson210, S. R. Thondapu104, K. A. Thorne64, E. Thrane6, J. Tissino44,45, A. Tiwari80, Pawan Tiwari44, Praveer Tiwari195, S. Tiwari189, V. Tiwari119, M. R. Todd79, M. Toffano92, A. M. Toivonen18, K. Toland87, A. E. Tolley74, T. Tomaru25, V. Tommasini11, T. Tomura50, H. Tong6, C. Tong-Yu141, A. Torres-Forné138,139, C. I. Torrie11, I. Tosta e Melo313, E. Tournefier31, M. Trad Nery114, K. Tran123, A. Trapananti52,51, R. Travaglini168, F. Travasso52,51, G. Traylor64, M. Trevor126, M. C. Tringali63, A. Tripathee91, G. Troian185,48, A. Trovato185,48, L. Trozzo4, R. J. Trudeau11, T. Tsang33, S. Tsuchida314, L. Tsukada213, K. Turbang188,23, M. Turconi114, C. Turski95, H. Ubach83,84, N. Uchikata204, T. Uchiyama50, R. P. Udall11, T. Uehara315, K. Ueno42, V. Undheim277, L. E. Uronen219, T. Ushiba50, M. Vacatello81,82, H. Vahlbruch8,9, N. Vaidya11, G. Vajente11, A. Vajpeyi6, J. Valencia99, M. Valentini108,37, S. A. Vallejo-Peña295, S. Vallero28, V. Valsan10, M. van Dael37,316, E. Van den Bossche188, J. F. J. van den Brand36,108,37, C. Van Den Broeck72,37, M. van der Sluys37,72, A. Van de Walle41, J. van Dongen37,108, K. Vandra103, M. VanDyke120, H. van Haevermaet23, J. V. van Heijningen37,108, P. Van Hove65, J. Vanier259, M. VanKeuren105, J. Vanosky2, N. van Remortel23, M. Vardaro36,37, A. F. Vargas124, V. Varma133, A. N. Vazquez90, A. Vecchio119, G. Vedovato93, J. Veitch87, P. J. Veitch116, S. Venikoudis15, R. C. Venterea18, P. Verdier56, M. Vereecken15, D. Verkindt31, B. Verma133, Y. Verma104, S. M. Vermeulen11, F. Vetrano61, A. Veutro38,39, A. Viceré61,62, S. Vidyant79, A. D. Viets89, A. Vijaykumar190, A. Vilkha111, N. Villanueva Espinosa138, V. Villa-Ortega178, E. T. Vincent57, J.-Y. Vinet114, S. Viret56, S. Vitale35, H. Vocca77,51, D. Voigt98, E. R. G. von Reis2, J. S. A. von Wrangel8,9, W. E. Vossius231, L. Vujeva140, S. P. Vyatchanin109, J. Wack11, L. E. Wade105, M. Wade105, K. J. Wagner111, L. Wallace11, E. J. Wang90, H. Wang217, J. Z. Wang91, W. H. Wang165, Y. F. Wang1, G. Waratkar195, J. Warner2, M. Was31, T. Washimi25, N. Y. Washington11, D. Watarai42, B. Weaver2, S. A. Webster87, N. L. Weickhardt98, M. Weinert8,9, A. J. Weinstein11, R. Weiss35, L. Wen73, K. Wette34, J. T. Whelan111, B. F. Whiting46, C. L. Whittall119, C. Whittle11, E. G. Wickens74, D. Wilken8,9,9, A. T. Wilkin211, B. M. Williams120, D. Williams87, M. J. Williams74, N. S. Williams1, J. L. Willis11, B. Willke9,8,9, M. Wils110, L. Wilson105, C. W. Winborn106, J. Winterflood73, C. C. Wipf11, G. Woan87, J. Woehler36,37, N. E. Wolfe35, H. T. Wong141, I. C. F. Wong219,110, K. Wong190, T. Wouters72,37, J. L. Wright2, M. Wright87,72, B. Wu79, C. Wu142, D. S. Wu8,9, H. Wu142, K. Wu120, Q. Wu53, Y. Wu97, Z. Wu101, E. Wuchner54, D. M. Wysocki10, V. A. Xu207, Y. Xu99, N. Yadav28, H. Yamamoto11, K. Yamamoto152, T. S. Yamamoto42, T. Yamamoto50, R. Yamazaki230, T. Yan119, K. Z. Yang18, Y. Yang146, Z. Yarbrough12, J. Yebana99, S.-W. Yeh142, A. B. Yelikar144, X. Yin35, J. Yokoyama317,42, T. Yokozawa50, S. Yuan73, H. Yuzurihara50, M. Zanolin66, M. Zeeshan111, T. Zelenova63, J.-P. Zendri93, M. Zeoli15, M. Zerrad40, M. Zevin97, L. Zhang11, N. Zhang57, R. Zhang150, T. Zhang119, C. Zhao73, Yue Zhao162, Yuhang Zhao20, Z.-C. Zhao318, Y. Zheng106, H. Zhong18, H. Zhou79, H. O. Zhu73, Z.-H. Zhu318,319, A. B. Zimmerman148, L. Zimmermann56, M. E. Zucker35,11, and J. Zweizig11 (The LIGO Scientific Collaboration, The Virgo Collaboration, and The KAGRA Collaboration†)

  • 1Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-14476 Potsdam, Germany
  • 2LIGO Hanford Observatory, Richland, Washington 99352, USA
  • 3Dipartimento di Farmacia, Università di Salerno, I-84084 Fisciano, Salerno, Italy
  • 4INFN, Sezione di Napoli, I-80126 Napoli, Italy
  • 5University of Warwick, Coventry CV4 7AL, United Kingdom
  • 6OzGrav, School of Physics and Astronomy, Monash University, Clayton 3800, Victoria, Australia
  • 7The Pennsylvania State University, University Park, Pennsylvania 16802, USA
  • 8Max Planck Institute for Gravitational Physics (Albert Einstein Institute), D-30167 Hannover, Germany
  • 9Leibniz Universität Hannover, D-30167 Hannover, Germany
  • 10University of Wisconsin-Milwaukee, Milwaukee, Wisconsin 53201, USA
  • 11LIGO Laboratory, California Institute of Technology, Pasadena, California 91125, USA
  • 12Louisiana State University, Baton Rouge, Louisiana 70803, USA
  • 13Tata Institute of Fundamental Research, Mumbai 400005, India
  • 14Centre de Physique Théorique, Aix-Marseille Université, Campus de Luminy, 163 Avenue de Luminy, 13009 Marseille, France
  • 15Université catholique de Louvain, B-1348 Louvain-la-Neuve, Belgium
  • 16Queen Mary University of London, London E1 4NS, United Kingdom
  • 17University of California, Davis, Davis, California 95616, USA
  • 18University of Minnesota, Minneapolis, Minnesota 55455, USA
  • 19Instituto Nacional de Pesquisas Espaciais, 12227-010 São José dos Campos, São Paulo, Brazil
  • 20Université Paris Cité, CNRS, Astroparticule et Cosmologie, F-75013 Paris, France
  • 21Università di Roma Tor Vergata, I-00133 Roma, Italy
  • 22INFN, Sezione di Roma Tor Vergata, I-00133 Roma, Italy
  • 23Universiteit Antwerpen, 2000 Antwerpen, Belgium
  • 24International Centre for Theoretical Sciences, Tata Institute of Fundamental Research, Bengaluru 560089, India
  • 25Gravitational Wave Science Project, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka City, Tokyo 181-8588, Japan
  • 26Advanced Technology Center, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka City, Tokyo 181-8588, Japan
  • 27Theoretisch-Physikalisches Institut, Friedrich-Schiller-Universität Jena, D-07743 Jena, Germany
  • 28INFN Sezione di Torino, I-10125 Torino, Italy
  • 29INFN, Sezione di Genova, I-16146 Genova, Italy
  • 30Dipartimento di Fisica, Università degli Studi di Genova, I-16146 Genova, Italy
  • 31Université Savoie Mont Blanc, CNRS, Laboratoire d’Annecy de Physique des Particules—IN2P3, F-74000 Annecy, France
  • 32Università di Napoli “Federico II,” I-80126 Napoli, Italy
  • 33Cardiff University, Cardiff CF24 3AA, United Kingdom
  • 34OzGrav, Australian National University, Canberra, Australian Capital Territory 0200, Australia
  • 35LIGO Laboratory, Massachusetts Institute of Technology, Cambridge, Massachusetts 02139, USA
  • 36Maastricht University, 6200 MD Maastricht, Netherlands
  • 37Nikhef, 1098 XG Amsterdam, Netherlands
  • 38INFN, Sezione di Roma, I-00185 Roma, Italy
  • 39Università di Roma “La Sapienza,” I-00185 Roma, Italy
  • 40Aix Marseille Univ, CNRS, Centrale Med, Institut Fresnel, F-13013 Marseille, France
  • 41Université Paris-Saclay, CNRS/IN2P3, IJCLab, 91405 Orsay, France
  • 42University of Tokyo, Tokyo, 113-0033, Japan
  • 43Institut de Física d’Altes Energies (IFAE), The Barcelona Institute of Science and Technology, Campus UAB, E-08193 Bellaterra (Barcelona), Spain
  • 44Gran Sasso Science Institute (GSSI), I-67100 L’Aquila, Italy
  • 45INFN, Laboratori Nazionali del Gran Sasso, I-67100 Assergi, Italy
  • 46University of Florida, Gainesville, Florida 32611, USA
  • 47Dipartimento di Scienze Matematiche, Informatiche e Fisiche, Università di Udine, I-33100 Udine, Italy
  • 48INFN, Sezione di Trieste, I-34127 Trieste, Italy
  • 49Tecnologico de Monterrey, Escuela de Ingeniería y Ciencias, 64849 Monterrey, Nuevo León, Mexico
  • 50Institute for Cosmic Ray Research, KAGRA Observatory, The University of Tokyo, 238 Higashi-Mozumi, Kamioka-cho, Hida City, Gifu 506-1205, Japan
  • 51INFN, Sezione di Perugia, I-06123 Perugia, Italy
  • 52Università di Camerino, I-62032 Camerino, Italy
  • 53University of Washington, Seattle, Washington 98195, USA
  • 54California State University Fullerton, Fullerton, California 92831, USA
  • 55SUPA, University of Strathclyde, Glasgow G1 1XQ, United Kingdom
  • 56Université Claude Bernard Lyon 1, CNRS, IP2I Lyon/IN2P3, UMR 5822, F-69622 Villeurbanne, France
  • 57Georgia Institute of Technology, Atlanta, Georgia 30332, USA
  • 58Chennai Mathematical Institute, Chennai 603103, India
  • 59Royal Holloway, University of London, London TW20 0EX, United Kingdom
  • 60Astronomical course, The Graduate University for Advanced Studies (SOKENDAI), 2-21-1 Osawa, Mitaka City, Tokyo 181-8588, Japan
  • 61Università degli Studi di Urbino “Carlo Bo,” I-61029 Urbino, Italy
  • 62INFN, Sezione di Firenze, I-50019 Sesto Fiorentino, Firenze, Italy
  • 63European Gravitational Observatory (EGO), I-56021 Cascina, Pisa, Italy
  • 64LIGO Livingston Observatory, Livingston, Louisiana 70754, USA
  • 65Université de Strasbourg, CNRS, IPHC UMR 7178, F-67000 Strasbourg, France
  • 66Embry-Riddle Aeronautical University, Prescott, Arizona 86301, USA
  • 67Dipartimento di Fisica “E.R. Caianiello,” Università di Salerno, I-84084 Fisciano, Salerno, Italy
  • 68King’s College London, University of London, London WC2R 2LS, United Kingdom
  • 69Korea Institute of Science and Technology Information, Daejeon 34141, Republic of Korea
  • 70International College, Osaka University, 1-1 Machikaneyama-cho, Toyonaka City, Osaka 560-0043, Japan
  • 71Accelerator Laboratory, High Energy Accelerator Research Organization (KEK), 1-1 Oho, Tsukuba City, Ibaraki 305-0801, Japan
  • 72Institute for Gravitational and Subatomic Physics (GRASP), Utrecht University, 3584 CC Utrecht, Netherlands
  • 73OzGrav, University of Western Australia, Crawley, Western Australia 6009, Australia
  • 74University of Portsmouth, Portsmouth, PO1 3FX, United Kingdom
  • 75Università di Trento, Dipartimento di Fisica, I-38123 Povo, Trento, Italy
  • 76INFN, Trento Institute for Fundamental Physics and Applications, I-38123 Povo, Trento, Italy
  • 77Università di Perugia, I-06123 Perugia, Italy
  • 78University of Oregon, Eugene, Oregon 97403, USA
  • 79Syracuse University, Syracuse, New York 13244, USA
  • 80Inter-University Centre for Astronomy and Astrophysics, Pune 411007, India
  • 81INFN, Sezione di Pisa, I-56127 Pisa, Italy
  • 82Università di Pisa, I-56127 Pisa, Italy
  • 83Institut de Ciències del Cosmos (ICCUB), Universitat de Barcelona (UB), c. Martí i Franquès, 1, 08028 Barcelona, Spain
  • 84Departament de Física Quàntica i Astrofísica (FQA), Universitat de Barcelona (UB), c. Martí i Franqués, 1, 08028 Barcelona, Spain
  • 85Institut d’Estudis Espacials de Catalunya, c. Gran Capità, 2-4, 08034 Barcelona, Spain
  • 86Dipartimento di Medicina, Chirurgia e Odontoiatria “Scuola Medica Salernitana,” Università di Salerno, I-84081 Baronissi, Salerno, Italy
  • 87IGR, University of Glasgow, Glasgow G12 8QQ, United Kingdom
  • 88HUN-REN Wigner Research Centre for Physics, H-1121 Budapest, Hungary
  • 89Concordia University Wisconsin, Mequon, Wisconsin 53097, USA
  • 90Stanford University, Stanford, California 94305, USA
  • 91University of Michigan, Ann Arbor, Michigan 48109, USA
  • 92Università di Padova, Dipartimento di Fisica e Astronomia, I-35131 Padova, Italy
  • 93INFN, Sezione di Padova, I-35131 Padova, Italy
  • 94Institute for Plasma Research, Bhat, Gandhinagar 382428, India
  • 95Universiteit Gent, B-9000 Gent, Belgium
  • 96Nicolaus Copernicus Astronomical Center, Polish Academy of Sciences, 00-716, Warsaw, Poland
  • 97Northwestern University, Evanston, Illinois 60208, USA
  • 98Universität Hamburg, D-22761 Hamburg, Germany
  • 99IAC3–IEEC, Universitat de les Illes Balears, E-07122 Palma de Mallorca, Spain
  • 100Aix-Marseille Université, Université de Toulon, CNRS, CPT, Marseille, France
  • 101Laboratoire des 2 Infinis—Toulouse (L2IT-IN2P3), F-31062 Toulouse Cedex 9, France
  • 102Università di Siena, Dipartimento di Scienze Fisiche, della Terra e dell’Ambiente, I-53100 Siena, Italy
  • 103Villanova University, Villanova, Pennsylvania 19085, USA
  • 104RRCAT, Indore, Madhya Pradesh 452013, India
  • 105Kenyon College, Gambier, Ohio 43022, USA
  • 106Missouri University of Science and Technology, Rolla, Missouri 65409, USA
  • 107Indian Institute of Technology Madras, Chennai 600036, India
  • 108Department of Physics and Astronomy, Vrije Universiteit Amsterdam, 1081 HV Amsterdam, Netherlands
  • 109Lomonosov Moscow State University, Moscow 119991, Russia
  • 110Katholieke Universiteit Leuven, Oude Markt 13, 3000 Leuven, Belgium
  • 111Rochester Institute of Technology, Rochester, New York 14623, USA
  • 112Université libre de Bruxelles, 1050 Bruxelles, Belgium
  • 113Bar-Ilan University, Ramat Gan, 5290002, Israel
  • 114Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Artemis, F-06304 Nice, France
  • 115University of British Columbia, Vancouver, British Columbia V6T 1Z4, Canada
  • 116OzGrav, University of Adelaide, Adelaide, South Australia 5005, Australia
  • 117Centre national de la recherche scientifique, 75016 Paris, France
  • 118Univ Rennes, CNRS, Institut FOTON—UMR 6082, F-35000 Rennes, France
  • 119University of Birmingham, Birmingham B15 2TT, United Kingdom
  • 120Washington State University, Pullman, Washington 99164, USA
  • 121Cornell University, Ithaca, New York 14850, USA
  • 122Laboratoire Kastler Brossel, Sorbonne Université, CNRS, ENS-Université PSL, Collège de France, F-75005 Paris, France
  • 123Christopher Newport University, Newport News, Virginia 23606, USA
  • 124OzGrav, University of Melbourne, Parkville, Victoria 3010, Australia
  • 125Astronomical Observatory Warsaw University, 00-478 Warsaw, Poland
  • 126University of Maryland, College Park, Maryland 20742, USA
  • 127Università degli Studi di Milano-Bicocca, I-20126 Milano, Italy
  • 128INFN, Sezione di Milano-Bicocca, I-20126 Milano, Italy
  • 129Université de Lyon, Université Claude Bernard Lyon 1, CNRS, Institut Lumière Matière, F-69622 Villeurbanne, France
  • 130University of Chicago, Chicago, Illinois 60637, USA
  • 131University of Arizona, Tucson, Arizona 85721, USA
  • 132INFN, Sezione di Napoli, Gruppo Collegato di Salerno, I-80126 Napoli, Italy
  • 133University of Massachusetts Dartmouth, North Dartmouth, Massachusetts 02747, USA
  • 134Niels Bohr Institute, Copenhagen University, 2100 København, Denmark
  • 135Universidad de Guadalajara, 44430 Guadalajara, Jalisco, Mexico
  • 136Istituto di Astrofisica e Planetologia Spaziali di Roma, 00133 Roma, Italy
  • 137Colorado State University, Fort Collins, Colorado 80523, USA
  • 138Departamento de Astronomía y Astrofísica, Universitat de València, E-46100 Burjassot, València, Spain
  • 139Observatori Astronòmic, Universitat de València, E-46980 Paterna, València, Spain
  • 140Niels Bohr Institute, University of Copenhagen, 2100 Kóbenhavn, Denmark
  • 141National Central University, Taoyuan City 320317, Taiwan
  • 142National Tsing Hua University, Hsinchu City 30013, Taiwan
  • 143OzGrav, Charles Sturt University, Wagga Wagga, New South Wales 2678, Australia
  • 144Vanderbilt University, Nashville, Tennessee 37235, USA
  • 145University of the Chinese Academy of Sciences/International Centre for Theoretical Physics Asia-Pacific, Bejing 100049, China
  • 146Department of Electrophysics, National Yang Ming Chiao Tung University, 101 University Street, Hsinchu, Taiwan
  • 147Kamioka Branch, National Astronomical Observatory of Japan, 238 Higashi-Mozumi, Kamioka-cho, Hida City, Gifu 506-1205, Japan
  • 148University of Texas, Austin, Texas 78712, USA
  • 149CaRT, California Institute of Technology, Pasadena, California 91125, USA
  • 150Northeastern University, Boston, Massachusetts 02115, USA
  • 151Dipartimento di Ingegneria Industriale (DIIN), Università di Salerno, I-84084 Fisciano, Salerno, Italy
  • 152Faculty of Science, University of Toyama, 3190 Gofuku, Toyama City, Toyama 930-8555, Japan
  • 153Carleton College, Northfield, Minnesota 55057, USA
  • 154University of Szeged, Dóm tér 9, Szeged 6720, Hungary
  • 155OzGrav, Swinburne University of Technology, Hawthorn VIC 3122, Australia
  • 156INFN Cagliari, Physics Department, Università degli Studi di Cagliari, Cagliari 09042, Italy
  • 157Università degli Studi di Cagliari, Via Università 40, 09124 Cagliari, Italy
  • 158Université Libre de Bruxelles, Brussels 1050, Belgium
  • 159INAF, Osservatorio Astronomico di Brera sede di Merate, I-23807 Merate, Lecco, Italy
  • 160Departamento de Matemáticas, Universitat de València, E-46100 Burjassot, València, Spain
  • 161Montana State University, Bozeman, Montana 59717, USA
  • 162The University of Utah, Salt Lake City, Utah 84112, USA
  • 163Johns Hopkins University, Baltimore, Maryland 21218, USA
  • 164University of Rhode Island, Kingston, Rhode Island 02881, USA
  • 165The University of Texas Rio Grande Valley, Brownsville, Texas 78520, USA
  • 166Université de Liège, B-4000 Liège, Belgium
  • 167DIFA- Alma Mater Studiorum Università di Bologna, Via Zamboni, 33–40126 Bologna, Italy
  • 168Istituto Nazionale Di Fisica Nucleare—Sezione di Bologna, viale Carlo Berti Pichat 6/2–40127 Bologna, Italy
  • 169University of Manitoba, Winnipeg, MB R3T 2N2, Canada
  • 170INFN-CNAF—Bologna, Viale Carlo Berti Pichat, 6/2, 40127 Bologna BO, Italy
  • 171Università degli Studi di Sassari, I-07100 Sassari, Italy
  • 172INFN, Laboratori Nazionali del Sud, I-95125 Catania, Italy
  • 173Université de Normandie, ENSICAEN, UNICAEN, CNRS/IN2P3, LPC Caen, F-14000 Caen, France
  • 174Laboratoire de Physique Corpusculaire Caen, 6 boulevard du maréchal Juin, F-14050 Caen, France
  • 175The University of Sheffield, Sheffield S10 2TN, United Kingdom
  • 176Université Claude Bernard Lyon 1, CNRS, Laboratoire des Matériaux Avancés (LMA), IP2I Lyon/IN2P3, UMR 5822, F-69622 Villeurbanne, France
  • 177Università di Firenze, Sesto Fiorentino I-50019, Italy
  • 178IGFAE, Universidade de Santiago de Compostela, E-15782 Santiago de Compostela, Spain
  • 179Dipartimento di Scienze Matematiche, Fisiche e Informatiche, Università di Parma, I-43124 Parma, Italy
  • 180INFN, Sezione di Milano Bicocca, Gruppo Collegato di Parma, I-43124 Parma, Italy
  • 181California State University, Los Angeles, Los Angeles, California 90032, USA
  • 182Marquette University, Milwaukee, Wisconsin 53233, USA
  • 183Perimeter Institute, Waterloo, Ontario N2L 2Y5, Canada
  • 184Corps des Mines, Mines Paris, Université PSL, 60 Bd Saint-Michel, 75272 Paris, France
  • 185Dipartimento di Fisica, Università di Trieste, I-34127 Trieste, Italy
  • 186Université Côte d’Azur, Observatoire de la Côte d’Azur, CNRS, Lagrange, F-06304 Nice, France
  • 187National Center for Nuclear Research, 05-400 Świerk-Otwock, Poland
  • 188Vrije Universiteit Brussel, 1050 Brussel, Belgium
  • 189University of Zurich, Winterthurerstrasse 190, 8057 Zurich, Switzerland
  • 190Canadian Institute for Theoretical Astrophysics, University of Toronto, Toronto, Ontario M5S 3H8, Canada
  • 191Stony Brook University, Stony Brook, New York 11794, USA
  • 192Center for Computational Astrophysics, Flatiron Institute, New York, New York 10010, USA
  • 193Montclair State University, Montclair, New Jersey 07043, USA
  • 194HUN-REN Institute for Nuclear Research, H-4026 Debrecen, Hungary
  • 195Indian Institute of Technology Bombay, Powai, Mumbai 400 076, India
  • 196Centro de Física das Universidades do Minho e do Porto, Universidade do Minho, PT-4710-057 Braga, Portugal
  • 197Aix Marseille Univ, CNRS/IN2P3, CPPM, Marseille, France
  • 198CNR-SPIN, I-84084 Fisciano, Salerno, Italy
  • 199Scuola di Ingegneria, Università della Basilicata, I-85100 Potenza, Italy
  • 200Western Washington University, Bellingham, Washington 98225, USA
  • 201SUPA, University of the West of Scotland, Paisley PA1 2BE, United Kingdom
  • 202Barry University, Miami Shores, Florida 33168, USA
  • 203Eötvös University, Budapest 1117, Hungary
  • 204Institute for Cosmic Ray Research, KAGRA Observatory, The University of Tokyo, 5-1-5 Kashiwa-no-Ha, Kashiwa City, Chiba 277-8582, Japan
  • 205Department of Physics, Graduate School of Science, Osaka Metropolitan University, 3-3-138 Sugimoto-cho, Sumiyoshi-ku, Osaka City, Osaka 558-8585, Japan
  • 206University of Sannio at Benevento, I-82100 Benevento, Italy and INFN, Sezione di Napoli, I-80100 Napoli, Italy
  • 207University of California, Berkeley, California 94720, USA
  • 208Instituto de Fisica Teorica UAM-CSIC, Universidad Autonoma de Madrid, 28049 Madrid, Spain
  • 209Laboratoire d’Acoustique de l’Université du Mans, UMR CNRS 6613, F-72085 Le Mans, France
  • 210University of Southampton, Southampton SO17 1BJ, United Kingdom
  • 211University of California, Riverside, Riverside, California 92521, USA
  • 212Dipartimento di Ingegneria Industriale, Elettronica e Meccanica, Università degli Studi Roma Tre, I-00146 Roma, Italy
  • 213University of Nevada, Las Vegas, Las Vegas, Nevada 89154, USA
  • 214University of Nottingham NG7 2RD, United Kingdom
  • 215Ariel University, Ramat HaGolan St 65, Ari’el, Israel
  • 216The University of Mississippi, University, Mississippi 38677, USA
  • 217Graduate School of Science, Institute of Science Tokyo, 2-12-1 Ookayama, Meguro-ku, Tokyo 152-8551, Japan
  • 218Institute of Physics, Academia Sinica, 128 Section II, Academia Road, Nankang, Taipei 11529, Taiwan
  • 219The Chinese University of Hong Kong, Shatin, NT, Hong Kong
  • 220American University, Washington, DC 20016, USA
  • 221Dipartimento di Fisica, Università degli studi di Milano, Via Celoria 16, I-20133, Milano, Italy
  • 222INFN, sezione di Milano, Via Celoria 16, I-20133, Milano, Italy
  • 223Department of Applied Physics, Fukuoka University, 8-19-1 Nanakuma, Jonan, Fukuoka City, Fukuoka 814-0180, Japan
  • 224University of Cambridge, Cambridge CB2 1TN, United Kingdom
  • 225University of Lancaster, Lancaster LA1 4YW, United Kingdom
  • 226College of Industrial Technology, Nihon University, 1-2-1 Izumi, Narashino City, Chiba 275-8575, Japan
  • 227Faculty of Engineering, Niigata University, 8050 Ikarashi-2-no-cho, Nishi-ku, Niigata City, Niigata 950-2181, Japan
  • 228Department of Physics, Tamkang University, No. 151, Yingzhuan Road, Danshui District, New Taipei City 25137, Taiwan
  • 229Rutherford Appleton Laboratory, Didcot OX11 0DE, United Kingdom
  • 230Department of Physical Sciences, Aoyama Gakuin University, 5-10-1 Fuchinobe, Sagamihara City, Kanagawa 252-5258, Japan
  • 231Helmut Schmidt University, D-22043 Hamburg, Germany
  • 232Nambu Yoichiro Institute of Theoretical and Experimental Physics (NITEP), Osaka Metropolitan University, 3-3-138 Sugimoto-cho, Sumiyoshi-ku, Osaka City, Osaka 558-8585, Japan
  • 233Directorate of Construction, Services and Estate Management, Mumbai 400094, India
  • 234Observatoire Astronomique de Strasbourg, 11 Rue de l’Université, 67000 Strasbourg, France
  • 235Faculty of Physics, University of Białystok, 15-245 Białystok, Poland
  • 236National Astronomical Observatories, Chinese Academic of Sciences, 20A Datun Road, Chaoyang District, Beijing, China
  • 237School of Astronomy and Space Science, University of Chinese Academy of Sciences, 20A Datun Road, Chaoyang District, Beijing, China
  • 238Sungkyunkwan University, Seoul 03063, Republic of Korea
  • 239Department of Physics, Ulsan National Institute of Science and Technology (UNIST), 50 UNIST-gil, Ulju-gun, Ulsan 44919, Republic of Korea
  • 240Institute for Cosmic Ray Research, The University of Tokyo, 5-1-5 Kashiwa-no-Ha, Kashiwa City, Chiba 277-8582, Japan
  • 241Chung-Ang University, Seoul 06974, Republic of Korea
  • 242University of Washington Bothell, Bothell, Washington 98011, USA
  • 243Laboratoire de Physique et de Chimie de l’Environnement, Université Joseph KI-ZERBO, 9GH2+3V5, Ouagadougou, Burkina Faso
  • 244Ewha Womans University, Seoul 03760, Republic of Korea
  • 245National Institute for Mathematical Sciences, Daejeon 34047, Republic of Korea
  • 246Korea Astronomy and Space Science Institute, Daejeon 34055, Republic of Korea
  • 247Department of Astronomy and Space Science, Chungnam National University, 9 Daehak-ro, Yuseong-gu, Daejeon 34134, Republic of Korea
  • 248Institute of Particle and Nuclear Studies (IPNS), High Energy Accelerator Research Organization (KEK), 1-1 Oho, Tsukuba City, Ibaraki 305-0801, Japan
  • 249Division of Science, National Astronomical Observatory of Japan, 2-21-1 Osawa, Mitaka City, Tokyo 181-8588, Japan
  • 250Nagoya University, Nagoya, 464-8601, Japan
  • 251Department of Physics, Aristotle University of Thessaloniki, 54124 Thessaloniki, Greece
  • 252Bard College, Annandale-On-Hudson, New York 12504, USA
  • 253Technical University of Braunschweig, D-38106 Braunschweig, Germany
  • 254Institute of Mathematics, Polish Academy of Sciences, 00656 Warsaw, Poland
  • 255Astronomical Observatory, Jagiellonian University, 31-007 Cracow, Poland
  • 256Department of Physics and Astronomy, University of Padova, Via Marzolo, 8-35151 Padova, Italy
  • 257Sezione di Padova, Istituto Nazionale di Fisica Nucleare (INFN), Via Marzolo, 8-35131 Padova, Italy
  • 258Department of Physics, Nagoya University, ES building, Furocho, Chikusa-ku, Nagoya, Aichi 464-8602, Japan
  • 259Université de Montréal/Polytechnique, Montreal, Quebec H3T 1J4, Canada
  • 260Indian Institute of Science Education and Research, Kolkata, Mohanpur, West Bengal 741252, India
  • 261Seoul National University, Seoul 08826, Republic of Korea
  • 262Department of Computer Simulation, Inje University, 197 Inje-ro, Gimhae, Gyeongsangnam-do 50834, Republic of Korea
  • 263NAVIER, École des Ponts, Univ Gustave Eiffel, CNRS, Marne-la-Vallée, France
  • 264Gravitational Wave Science Project, National Astronomical Observatory of Japan (NAOJ), Mitaka City, Tokyo 181-8588, Japan
  • 265Department of Physics, National Cheng Kung University, No. 1, University Road, Tainan City 701, Taiwan
  • 266St. Thomas University, Miami Gardens, Florida 33054, USA
  • 267Scuola Normale Superiore, I-56126 Pisa, Italy
  • 268Institució Catalana de Recerca i Estudis Avançats, E-08010 Barcelona, Spain
  • 269Institut de Física d’Altes Energies, E-08193 Barcelona, Spain
  • 270Institut fuer Theoretische Astrophysik, Zentrum fuer Astronomie Heidelberg, Universitaet Heidelberg, Albert Ueberle Straße 2, 69120 Heidelberg, Germany
  • 271Institucio Catalana de Recerca i Estudis Avançats (ICREA), Passeig de Lluís Companys, 23, 08010 Barcelona, Spain
  • 272Research Center for Space Science, Advanced Research Laboratories, Tokyo City University, 3-3-1 Ushikubo-Nishi, Tsuzuki-Ku, Yokohama, Kanagawa 224-8551, Japan
  • 273Tsinghua University, Beijing 100084, China
  • 274Institut des Hautes Etudes Scientifiques, F-91440 Bures-sur-Yvette, France
  • 275Faculty of Law, Ryukoku University, 67 Fukakusa Tsukamoto-cho, Fushimi-ku, Kyoto City, Kyoto 612-8577, Japan
  • 276Phenikaa Institute for Advanced Study (PIAS), Phenikaa University, Yen Nghia, Ha Dong, Hanoi, Vietnam
  • 277University of Stavanger, 4021 Stavanger, Norway
  • 278Physics Program, Graduate School of Advanced Science and Engineering, Hiroshima University, 1-3-1 Kagamiyama, Higashihiroshima City, Hiroshima 739-8526, Japan
  • 279GRAPPA, Anton Pannekoek Institute for Astronomy and Institute for High-Energy Physics, University of Amsterdam, 1098 XH Amsterdam, Netherlands
  • 280University College London, London WC1E 6BT, United Kingdom
  • 281Observatoire de Paris, 75014 Paris, France
  • 282Laboratoire Univers et Théories, Observatoire de Paris, 92190 Meudon, France
  • 283Graduate School of Science and Technology, Niigata University, 8050 Ikarashi-2-no-cho, Nishi-ku, Niigata City, Niigata 950-2181, Japan
  • 284University of Maryland, Baltimore County, Baltimore, Maryland 21250, USA
  • 285CSIR-Central Glass and Ceramic Research Institute, Kolkata, West Bengal 700032, India
  • 286Consiglio Nazionale delle Ricerche—Istituto dei Sistemi Complessi, I-00185 Roma, Italy
  • 287Department of Astronomy, Yonsei University, 50 Yonsei-Ro, Seodaemun-Gu, Seoul 03722, Republic of Korea
  • 288Department of Physics, University of Guadalajara, Avenida Revolucion 1500, Colonia Olimpica C.P. 44430, Guadalajara, Jalisco, Mexico
  • 289Hobart and William Smith Colleges, Geneva, New York 14456, USA
  • 290INAF, Osservatorio Astronomico di Padova, I-35122 Padova, Italy
  • 291Dipartimento di Ingegneria, Università del Sannio, I-82100 Benevento, Italy
  • 292Museo Storico della Fisica e Centro Studi e Ricerche “Enrico Fermi,” I-00184 Roma, Italy
  • 293Kennesaw State University, Kennesaw, Georgia 30144, USA
  • 294Subatech, CNRS/IN2P3—IMT Atlantique—Nantes Université, 4 rue Alfred Kastler BP 20722 44307 Nantes CÉDEX 03, France
  • 295Universidad de Antioquia, Medellín, Colombia
  • 296Departamento de Física—ETSIDI, Universidad Politécnica de Madrid, 28012 Madrid, Spain
  • 297Department of Electronic Control Engineering, National Institute of Technology, Nagaoka College, 888 Nishikatakai, Nagaoka City, Niigata 940-8532, Japan
  • 298Trinity College, Hartford, Connecticut 06106, USA
  • 299Dipartimento di Fisica e Scienze della Terra, Università Degli Studi di Ferrara, Via Saragat, 1, 44121 Ferrara FE, Italy
  • 300Faculty of Science, Toho University, 2-2-1 Miyama, Funabashi City, Chiba 274-8510, Japan
  • 301Indian Institute of Technology, Palaj, Gandhinagar, Gujarat 382355, India
  • 302Kavli Institute for Astronomy and Astrophysics, Peking University, Yiheyuan Road 5, Haidian District, Beijing 100871, China
  • 303Laboratoire MSME, Cité Descartes, 5 Boulevard Descartes, Champs-sur-Marne, 77454 Marne-la-Vallée Cedex 2, France
  • 304Faculty of Information Science and Technology, Osaka Institute of Technology, 1-79-1 Kitayama, Hirakata City, Osaka 573-0196, Japan
  • 305NASA Goddard Space Flight Center, Greenbelt, Maryland 20771, USA
  • 306Faculty of Science and Technology, Kochi University, 2-5-1 Akebono-cho, Kochi-shi, Kochi 780-8520, Japan
  • 307Laboratoire de Physique de l’École Normale Supérieure, ENS, (CNRS, Université PSL, Sorbonne Université, Université Paris Cité), F-75005 Paris, France
  • 308Faculty of Physics, University of Warsaw, Ludwika Pasteura 5, 02-093 Warszawa, Poland
  • 309Laser Interferometry and Gravitational Wave Astronomy, Max Planck Institute for Gravitational Physics, Callinstrasse 38, 30167 Hannover, Germany
  • 310The Hakubi Center for Advanced Research, Kyoto University, Yoshida-honmachi, Sakyou-ku, Kyoto City, Kyoto 606-8501, Japan
  • 311Department of Physics, Kyoto University, Kita-Shirakawa Oiwake-cho, Sakyou-ku, Kyoto City, Kyoto 606-8502, Japan
  • 312Yukawa Institute for Theoretical Physics (YITP), Kyoto University, Kita-Shirakawa Oiwake-cho, Sakyou-ku, Kyoto City, Kyoto 606-8502, Japan
  • 313University of Catania, Department of Physics and Astronomy, Via S. Sofia, 64, 95123 Catania CT, Italy
  • 314National Institute of Technology, Fukui College, Geshi-cho, Sabae-shi, Fukui 916-8507, Japan
  • 315Department of Communications Engineering, National Defense Academy of Japan, 1-10-20 Hashirimizu, Yokosuka City, Kanagawa 239-8686, Japan
  • 316Eindhoven University of Technology, 5600 MB Eindhoven, Netherlands
  • 317Kavli Institute for the Physics and Mathematics of the Universe (Kavli IPMU), WPI, The University of Tokyo, 5-1-5 Kashiwa-no-Ha, Kashiwa City, Chiba 277-8583, Japan
  • 318Department of Astronomy, Beijing Normal University, Xinjiekouwai Street 19, Haidian District, Beijing 100875, China
  • 319School of Physics and Technology, Wuhan University, Bayi Road 299, Wuchang District, Wuhan, Hubei, 430072, China
  • 320CENTRA, Departamento de Fìsica, Instituto Superior Tècnico—IST, Universidade de Lisboa—UL, Avenida Rovisco Pais 1, 1049-001 Lisboa, Portugal
  • 321Department of Astronomy, Columbia University, New York, New York 10027, USA

  • *Full author list given at the end of the Letter.
  • †Contact author: lvc.publications@ligo.org
  • ‡Deceased.

Phys. Rev. Lett. 136, 041403 – Published 29 January, 2026

DOI: https://doi.org/10.1103/6c61-fm1n

Abstract

The binary black hole signal GW250114, the loudest gravitational wave detected to date, offers a unique opportunity to test Einstein’s general relativity (GR) in the high-velocity, strong-gravity regime and probe whether the remnant conforms to the Kerr metric. Upon perturbation, black holes emit a spectrum of damped sinusoids with specific, complex frequencies. Our analysis of the postmerger signal shows that at least two quasinormal modes are required to explain the data, with the most damped remaining statistically significant for about one cycle. We probe the remnant’s Kerr nature by constraining the spectroscopic pattern of the dominant quadrupolar (ℓ=m=2) mode and its first overtone to match the Kerr prediction to tens of percent at multiple postpeak times. The measured mode amplitudes and phases agree with a numerical-relativity simulation having parameters close to GW250114. By fitting a parametrized waveform that incorporates the full inspiral-merger-ringdown sequence, we constrain the fundamental (ℓ=m=4) mode to tens of percent and bound the quadrupolar frequency to within a few percent of the GR prediction. We perform a suite of tests—spanning inspiral, merger, and ringdown—finding constraints that are comparable to, and in some cases 2–3 times more stringent than those obtained by combining dozens of events in the fourth Gravitational-Wave Transient Catalog. These results constitute the most stringent single-event verification of GR and the Kerr nature of black holes to date, and outline the power of black-hole spectroscopy for future gravitational-wave observations.

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synopsis

General Relativity Survives a Tough Trial

Published 29 January, 2026

An analysis of a record-breaking gravitational-wave detection tests whether general relativity holds under extreme conditions.

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References (222)

  1. J. Aasi et al. (LIGO Scientific Collaboration), Advanced LIGO, Classical Quantum Gravity 32, 074001 (2015).
  2. A. G. Abac et al., GW250114: Testing Hawking’s area law and the Kerr nature of black holes, arXiv:2509.0000.
  3. F. Acernese et al. (Virgo Collaboration), Advanced Virgo: A second-generation interferometric gravitational wave detector, Classical Quantum Gravity 32, 024001 (2015).
  4. T. Akutsu et al. (KAGRA Collaboration), Overview of KAGRA: Detector design and construction history, Prog. Theor. Exp. Phys. 2021, 05A101 (2021).
  5. A. Einstein, On the general thoery of relativity, Sitzungsber. K. Preuss. Akad. Wiss. 49, 778 (1915), https://ui.adsabs.harvard.edu/abs/1915SPAW.......778E/abstract.
  6. R. P. Kerr, Gravitational field of a spinning mass as an example of algebraically special metrics, Phys. Rev. Lett. 11, 237 (1963).
  7. R. L. Arnowitt, S. Deser, and C. W. Misner, The dynamics of general relativity, Gen. Relativ. Gravit. 40, 1997 (2008).
  8. Y. Foures-Bruhat, Theoreme d’existence pour certains systemes derivees partielles non lineaires, Acta Math. 88, 141 (1952).
  9. K. Schwarzschild, On the gravitational field of a mass point according to Einstein’s theory, Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.) 1916, 189 (1916).
  10. E. T. Newman, E. Couch, K. Chinnapared, A. Exton, A. Prakash, and R. Torrence, Metric of a rotating, charged mass, J. Math. Phys. (N.Y.) 6, 918 (1965).
  11. W. Israel, Event horizons in static electrovac space-times, Commun. Math. Phys. 8, 245 (1968).
  12. B. Carter, Axisymmetric black hole has only two degrees of freedom, Phys. Rev. Lett. 26, 331 (1971).
  13. S. W. Hawking, Black holes in general relativity, Commun. Math. Phys. 25, 152 (1972).
  14. D. C. Robinson, Uniqueness of the Kerr black hole, Phys. Rev. Lett. 34, 905 (1975).
  15. P. O. Mazur, Proof of uniqueness of the Kerr-Newman black hole solution, J. Phys. A 15, 3173 (1982).
  16. B. Carter, Global structure of the Kerr family of gravitational fields, Phys. Rev. 174, 1559 (1968).
  17. R. Penrose, Gravitational collapse: The role of general relativity, Riv. Nuovo Cimento 1, 252 (1969).
  18. R. Penrose and R. M. Floyd, Extraction of rotational energy from a black hole, Nat. Phys. Sci. 229, 177 (1971).
  19. J. M. Bardeen, B. Carter, and S. W. Hawking, The four laws of black hole mechanics, Commun. Math. Phys. 31, 161 (1973).
  20. M. Schmidt, 3C 273: A star-like object with large red-shift, Nature (London) 197, 1040 (1963).
  21. M. Dafermos, G. Holzegel, and I. Rodnianski, The linear stability of the Schwarzschild solution to gravitational perturbations, Acta Math. 222, 1 (2019).
  22. R. Teixeira da Costa, Mode stability for the Teukolsky equation on extremal and subextremal Kerr spacetimes, Commun. Math. Phys. 378, 705 (2020).
  23. S. Klainerman and J. Szeftel, Kerr stability for small angular momentum, Pure Appl. Math. Q. 19, 791 (2023).
  24. M. Dafermos, G. Holzegel, I. Rodnianski, and M. Taylor, The non-linear stability of the Schwarzschild family of black holes, arXiv:2104.08222.
  25. S. W. Hawking and R. Penrose, The singularities of gravitational collapse and cosmology, Proc. R. Soc. A 314, 529 (1970).
  26. A. Almheiri, T. Hartman, J. Maldacena, E. Shaghoulian, and A. Tajdini, The entropy of Hawking radiation, Rev. Mod. Phys. 93, 035002 (2021).
  27. S. Raju, Lessons from the information paradox, Phys. Rep. 943, 1 (2022).
  28. C. M. Will, The confrontation between general relativity and experiment, Living Rev. Relativity 17, 4 (2014).
  29. E. Berti et al., Testing general relativity with present and future astrophysical observations, Classical Quantum Gravity 32, 243001 (2015).
  30. N. Yunes, X. Siemens, and K. Yagi, Gravitational-wave tests of general relativity with ground-based detectors and pulsar-timing arrays, Living Rev. Relativity 28, 3 (2025).
  31. A. G. Abac et al. (LIGO Scientific, Virgo, and KAGRA Collaborations), GWTC-4.0: An introduction to version 4.0 of the gravitational-wave transient catalog, arXiv:2508.18080.
  32. A. G. Abac et al. (LIGO Scientific, Virgo, and KAGRA Collaborations), GWTC-4.0: Updating the gravitational-wave transient catalog with observations from the first part of the fourth LIGO-Virgo-KAGRA observing run, arXiv:2508.18082.
  33. L. Blanchet and B. S. Sathyaprakash, Detecting a tail effect in gravitational-wave experiments, Phys. Rev. Lett. 74, 1067 (1995).
  34. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Observation of gravitational waves from a binary black hole merger, Phys. Rev. Lett. 116, 061102 (2016).
  35. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Tests of general relativity with GW150914, Phys. Rev. Lett. 116, 221101 (2016); 121, 129902(E) (2018).
  36. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), GWTC-1: A gravitational-wave transient catalog of compact binary mergers observed by LIGO and Virgo during the first and second observing runs, Phys. Rev. X 9, 031040 (2019).
  37. R. Abbott et al. (LIGO Scientific and Virgo Collaborations), GWTC-2: Compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run, Phys. Rev. X 11, 021053 (2021).
  38. R. Abbott et al. (LIGO Scientific and Virgo Collaborations), GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run, Phys. Rev. D 109, 022001 (2024).
  39. R. Abbott et al. (KAGRA, Virgo, and LIGO Scientific Collaborations), GWTC-3: Compact binary coalescences observed by LIGO and Virgo during the second part of the third observing run, Phys. Rev. X 13, 041039 (2023).
  40. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Tests of general relativity with GW170817, Phys. Rev. Lett. 123, 011102 (2019).
  41. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Tests of general relativity with the binary black hole signals from the LIGO-Virgo catalog GWTC-1, Phys. Rev. D 100, 104036 (2019).
  42. R. Abbott et al. (LIGO Scientific and Virgo Collaborations), Tests of general relativity with binary black holes from the second LIGO-Virgo gravitational-wave transient catalog, Phys. Rev. D 103, 122002 (2021).
  43. R. Abbott et al. (LIGO Scientific,, and KAGRA Collaborations), Tests of general relativity with GWTC-3, Phys. Rev. D 112, 084080 (2025).
  44. P. C. C. Freire, N. Wex, G. Esposito-Farese, J. P. W. Verbiest, M. Bailes, B. A. Jacoby, M. Kramer, I. H. Stairs, J. Antoniadis, and G. H. Janssen, The relativistic pulsar-white dwarf binary PSR J1738+0333 II. The most stringent test of scalar-tensor gravity, Mon. Not. R. Astron. Soc. 423, 3328 (2012).
  45. M. Kramer et al., Strong-field gravity tests with the double pulsar, Phys. Rev. X 11, 041050 (2021).
  46. R. Abuter et al. (GRAVITY Collaboration), Detection of the gravitational redshift in the orbit of the star S2 near the Galactic centre massive black hole, Astron. Astrophys. 615, L15 (2018).
  47. T. Do et al., Relativistic redshift of the star S0-2 orbiting the Galactic center supermassive black hole, Science 365, 664 (2019).
  48. K. Akiyama et al. (Event Horizon Telescope Collaboration), First M87 Event Horizon Telescope results. I. The shadow of the supermassive black hole, Astrophys. J. Lett. 875, L1 (2019).
  49. T. Clifton, P. G. Ferreira, A. Padilla, and C. Skordis, Modified gravity and cosmology, Phys. Rep. 513, 1 (2012).
  50. A. Einstein, Über Gravitationswellen, Sitzungsber. Preuss. Akad. Wiss. Berlin (Math. Phys.) 1918, 154 (1918), https://ui.adsabs.harvard.edu/abs/1918SPAW.......154E/abstract.
  51. F. Pretorius, Evolution of binary black hole spacetimes, Phys. Rev. Lett. 95, 121101 (2005).
  52. M. Campanelli, C. O. Lousto, Y. Zlochower, B. Krishnan, and D. Merritt, Spin flips and precession in black-hole-binary mergers, Phys. Rev. D 75, 064030 (2007).
  53. J. G. Baker, J. Centrella, D.-I. Choi, M. Koppitz, and J. van Meter, Gravitational wave extraction from an inspiraling configuration of merging black holes, Phys. Rev. Lett. 96, 111102 (2006).
  54. C. V. Vishveshwara, Scattering of gravitational radiation by a Schwarzschild black-hole, Nature (London) 227, 936 (1970).
  55. W. H. Press, Long wave trains of gravitational waves from a vibrating black hole, Astrophys. J. 170, L105 (1971).
  56. T. Regge, Stability of a Schwarzschild singularity, Phys. Rev. 108, 1063 (1957).
  57. F. J. Zerilli, Effective potential for even parity Regge-Wheeler gravitational perturbation equations, Phys. Rev. Lett. 24, 737 (1970).
  58. S. A. Teukolsky, Perturbations of a rotating black hole. 1. Fundamental equations for gravitational electromagnetic and neutrino field perturbations, Astrophys. J. 185, 635 (1973).
  59. S. Chandrasekhar and S. L. Detweiler, The quasi-normal modes of the Schwarzschild black hole, Proc. R. Soc. A 344, 441 (1975).
  60. S. L. Detweiler, Resonant oscillations of a rapidly rotating black hole, Proc. R. Soc. A 352, 381 (1977).
  61. S. L. Detweiler, Black holes and gravitational waves. III. The resonant frequencies of rotating holes, Astrophys. J. 239, 292 (1980).
  62. E. W. Leaver, An analytic representation for the quasi-normal modes of Kerr black holes, Proc. R. Soc. A 402, 285 (1985).
  63. R. H. Price, Nonspherical perturbations of relativistic gravitational collapse. 1. Scalar and gravitational perturbations, Phys. Rev. D 5, 2419 (1972).
  64. R. H. Price, Nonspherical perturbations of relativistic gravitational collapse. II. Integer-spin, zero-rest-mass fields, Phys. Rev. D 5, 2439 (1972).
  65. H.-P. Nollert, Topical review: Quasinormal modes: The characteristic “sound” of black holes and neutron stars, Classical Quantum Gravity 16, R159 (1999).
  66. K. D. Kokkotas and B. G. Schmidt, Quasinormal modes of stars and black holes, Living Rev. Relativity 2, 2 (1999).
  67. O. Dreyer, B. J. Kelly, B. Krishnan, L. S. Finn, D. Garrison, and R. Lopez-Aleman, Black hole spectroscopy: Testing general relativity through gravitational wave observations, Classical Quantum Gravity 21, 787 (2004).
  68. E. Berti, V. Cardoso, and C. M. Will, On gravitational-wave spectroscopy of massive black holes with the space interferometer LISA, Phys. Rev. D 73, 064030 (2006).
  69. E. Berti, V. Cardoso, and A. O. Starinets, Quasinormal modes of black holes and black branes, Classical Quantum Gravity 26, 163001 (2009).
  70. S. Gossan, J. Veitch, and B. S. Sathyaprakash, Bayesian model selection for testing the no-hair theorem with black hole ringdowns, Phys. Rev. D 85, 124056 (2012).
  71. J. Meidam, M. Agathos, C. Van Den Broeck, J. Veitch, and B. S. Sathyaprakash, Testing the no-hair theorem with black hole ringdowns using TIGER, Phys. Rev. D 90, 064009 (2014).
  72. E. Berti, V. Cardoso, G. Carullo et al., Black hole spectroscopy: From theory to experiment, arXiv:2505.23895.
  73. R. Penrose, “Golden Oldie”: Gravitational collapse: The role of general relativity, Gen. Relativ. Gravit. 34, 1141 (2002).
  74. S. Klainerman, Mathematical challenges of general relativity, in The Ninth Marcel Grossmann Meeting, edited by V. G. Gurzadyan, R. T. Jantzen, and R. Ruffini (2002), pp. 28–43.
  75. P. T. Chruściel, J. Lopes Costa, and M. Heusler, Stationary black holes: Uniqueness and beyond, Living Rev. Relativity 15, 7 (2012).
  76. G. W. Gibbons, Vacuum polarization and the spontaneous loss of charge by black holes, Commun. Math. Phys. 44, 245 (1975).
  77. R. D. Blandford and R. L. Znajek, Electromagnetic extractions of energy from Kerr black holes, Mon. Not. R. Astron. Soc. 179, 433 (1977).
  78. R. S. Hanni, Limits on the charge of a collapsed object, Phys. Rev. D 25, 2509 (1982).
  79. G. Carullo, D. Laghi, N. K. Johnson-McDaniel, W. Del Pozzo, O. J. C. Dias, M. Godazgar, and J. E. Santos, Constraints on Kerr-Newman black holes from merger-ringdown gravitational-wave observations, Phys. Rev. D 105, 062009 (2022).
  80. G. Carullo, W. Del Pozzo, and J. Veitch, Observational black hole spectroscopy: A time-domain multimode analysis of GW150914, Phys. Rev. D 99, 123029 (2019); 100, 089903(E) (2019).
  81. M. Isi, M. Giesler, W. M. Farr, M. A. Scheel, and S. A. Teukolsky, Testing the no-hair theorem with GW150914, Phys. Rev. Lett. 123, 111102 (2019).
  82. C. D. Capano, M. Cabero, J. Westerweck, J. Abedi, S. Kastha, A. H. Nitz, A. B. Nielsen, and B. Krishnan, Observation of a multimode quasi-normal spectrum from a perturbed black hole, Phys. Rev. Lett. 131, 221402 (2023).
  83. R. Cotesta, G. Carullo, E. Berti, and V. Cardoso, Analysis of ringdown overtones in GW150914, Phys. Rev. Lett. 129, 111102 (2022).
  84. H. Siegel, M. Isi, and W. M. Farr, Ringdown of GW190521: Hints of multiple quasinormal modes with a precessional interpretation, Phys. Rev. D 108, 064008 (2023).
  85. V. Gennari, G. Carullo, and W. Del Pozzo, Searching for ringdown higher modes with a numerical relativity-informed post-merger model, Eur. Phys. J. C 84, 233 (2024).
  86. V. Varma, S. E. Field, M. A. Scheel, J. Blackman, D. Gerosa, L. C. Stein, L. E. Kidder, and H. P. Pfeiffer, Surrogate models for precessing binary black hole simulations with unequal masses, Phys. Rev. Res. 1, 033015 (2019).
  87. A. Gamboa et al., Accurate waveforms for eccentric, aligned-spin binary black holes: The multipolar effective-one-body model seobnrv5ehm, Phys. Rev. D 112, 044038 (2025).
  88. A. Nagar, R. Gamba, P. Rettegno, V. Fantini, and S. Bernuzzi, Effective-one-body waveform model for noncircularized, planar, coalescing black hole binaries: The importance of radiation reaction, Phys. Rev. D 110, 084001 (2024).
  89. E. W. Leaver, Spectral decomposition of the perturbation response of the Schwarzschild geometry, Phys. Rev. D 34, 384 (1986).
  90. N. Andersson, Evolving test fields in a black hole geometry, Phys. Rev. D 55, 468 (1997).
  91. H. Zhu et al., Imprints of changing mass and spin on black hole ringdown, Phys. Rev. D 110, 124028 (2024).
  92. A. Chavda, M. Lagos, and L. Hui, The impact of initial conditions on quasi-normal modes, J. Cosmol. Astropart. Phys. 07 (2025) 084.
  93. M. De Amicis, E. Cannizzaro, G. Carullo, and L. Sberna, Dynamical quasinormal mode excitation, arXiv:2506.21668.
  94. L. London, D. Shoemaker, and J. Healy, Modeling ringdown: Beyond the fundamental quasinormal modes, Phys. Rev. D 90, 124032 (2014); 94, 069902(E) (2016).
  95. K. Mitman et al., Nonlinearities in black hole ringdowns, Phys. Rev. Lett. 130, 081402 (2023).
  96. M. H.-Y. Cheung et al., Nonlinear effects in black hole ringdown, Phys. Rev. Lett. 130, 081401 (2023).
  97. S. Ma and H. Yang, Excitation of quadratic quasinormal modes for Kerr black holes, Phys. Rev. D 109, 104070 (2024).
  98. A. Buonanno, G. B. Cook, and F. Pretorius, Inspiral, merger and ring-down of equal-mass black-hole binaries, Phys. Rev. D 75, 124018 (2007).
  99. E. Berti, V. Cardoso, J. A. Gonzalez, U. Sperhake, M. Hannam, S. Husa, and B. Brügmann, Inspiral, merger and ringdown of unequal mass black hole binaries: A multipolar analysis, Phys. Rev. D 76, 064034 (2007).
  100. E. S. C. Ching, P. T. Leung, W. M. Suen, and K. Young, Wave propagation in gravitational systems: Late time behavior, Phys. Rev. D 52, 2118 (1995).
  101. S. Ma, M. A. Scheel, J. Moxon, K. C. Nelli, N. Deppe, L. E. Kidder, W. Throwe, and N. L. Vu, Merging black holes with Cauchy-characteristic matching: Computation of late-time tails, Phys. Rev. D 112, 024003 (2025).
  102. M. De Amicis, S. Albanesi, and G. Carullo, Inspiral-inherited ringdown tails, Phys. Rev. D 110, 104005 (2024).
  103. M. De Amicis et al., Late-time tails in nonlinear evolutions of merging black holes, Phys. Rev. Lett. 135, 171401 (2025).
  104. I. Kamaretsos, M. Hannam, and B. Sathyaprakash, Is black-hole ringdown a memory of its progenitor?, Phys. Rev. Lett. 109, 141102 (2012).
  105. L. T. London, Modeling ringdown. II. Aligned-spin binary black holes, implications for data analysis and fundamental theory, Phys. Rev. D 102, 084052 (2020).
  106. X. Jiménez Forteza, S. Bhagwat, P. Pani, and V. Ferrari, Spectroscopy of binary black hole ringdown using overtones and angular modes, Phys. Rev. D 102, 044053 (2020).
  107. M. H.-Y. Cheung, E. Berti, V. Baibhav, and R. Cotesta, Extracting linear and nonlinear quasinormal modes from black hole merger simulations, Phys. Rev. D 109, 044069 (2024); 110, 049902(E) (2024).
  108. L. Magaña Zertuche et al., High-precision ringdown surrogate model for non-precessing binary black holes, Phys. Rev. D 112, 024077 (2025).
  109. F. Nobili, S. Bhagwat, C. Pacilio, and D. Gerosa, Ringdown mode amplitudes of precessing binary black holes, Phys. Rev. D 112, 044058 (2025).
  110. M. Isi and W. M. Farr, Analyzing black-hole ringdowns, arXiv:2107.05609.
  111. A. Dhani, Importance of mirror modes in binary black hole ringdown waveform, Phys. Rev. D 103, 104048 (2021).
  112. X. Li, L. Sun, R. K. L. Lo, E. Payne, and Y. Chen, Angular emission patterns of remnant black holes, Phys. Rev. D 105, 024016 (2022).
  113. G. Carullo, W. Del Pozzo, and J. Veitch, pyring: A time-domain ringdown analysis python package, https://git.ligo.org/lscsoft/pyring (2023).
  114. G. Carullo et al., Empirical tests of the black hole no-hair conjecture using gravitational-wave observations, Phys. Rev. D 98, 104020 (2018).
  115. See Supplemental Material at http://link.aps.org/supplemental/10.1103/6c61-fm1n for additional details regarding the assumptions and analyses that have been presented.
  116. M. Giesler et al., Overtones and nonlinearities in binary black hole ringdowns, Phys. Rev. D 111, 084041 (2025).
  117. M. Isi, K. Chatziioannou, and W. M. Farr, Hierarchical test of general relativity with gravitational waves, Phys. Rev. Lett. 123, 121101 (2019).
  118. S. Ma, K. Mitman, L. Sun, N. Deppe, F. Hébert, L. E. Kidder, J. Moxon, W. Throwe, N. L. Vu, and Y. Chen, Quasinormal-mode filters: A new approach to analyze the gravitational-wave ringdown of binary black-hole mergers, Phys. Rev. D 106, 084036 (2022).
  119. S. Ma, L. Sun, and Y. Chen, Black hole spectroscopy by mode cleaning, Phys. Rev. Lett. 130, 141401 (2023).
  120. S. Ma, L. Sun, and Y. Chen, Using rational filters to uncover the first ringdown overtone in GW150914, Phys. Rev. D 107, 084010 (2023).
  121. N. Lu, S. Ma, O. J. Piccinni, L. Sun, and E. Finch, Statistical identification of ringdown modes with rational filters, Phys. Rev. D 112, 064047 (2025).
  122. R. Brito, A. Buonanno, and V. Raymond, Black-hole spectroscopy by making full use of gravitational-wave modeling, Phys. Rev. D 98, 084038 (2018).
  123. L. Pompili, E. Maggio, H. O. Silva, and A. Buonanno, Parametrized spin-precessing inspiral-merger-ringdown waveform model for tests of general relativity, Phys. Rev. D 111, 124040 (2025).
  124. E. Maggio, H. O. Silva, A. Buonanno, and A. Ghosh, Tests of general relativity in the nonlinear regime: A parametrized plunge-merger-ringdown gravitational waveform model, Phys. Rev. D 108, 024043 (2023).
  125. A. Ghosh, R. Brito, and A. Buonanno, Constraints on quasinormal-mode frequencies with LIGO-Virgo binary–black-hole observations, Phys. Rev. D 103, 124041 (2021).
  126. A. Ramos-Buades, A. Buonanno, H. Estellés, M. Khalil, D. P. Mihaylov, S. Ossokine, L. Pompili, and M. Shiferaw, Next generation of accurate and efficient multipolar precessing-spin effective-one-body waveforms for binary black holes, Phys. Rev. D 108, 124037 (2023).
  127. L. Pompili et al., Laying the foundation of the effective-one-body waveform models seobnrv5: Improved accuracy and efficiency for spinning nonprecessing binary black holes, Phys. Rev. D 108, 124035 (2023).
  128. X. Jiménez-Forteza, D. Keitel, S. Husa, M. Hannam, S. Khan, and M. Pürrer, Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy, Phys. Rev. D 95, 064024 (2017).
  129. F. Hofmann, E. Barausse, and L. Rezzolla, The final spin from binary black holes in quasi-circular orbits, Astrophys. J. Lett. 825, L19 (2016).
  130. J. G. Baker, W. D. Boggs, J. Centrella, B. J. Kelly, S. T. McWilliams, and J. R. van Meter, Mergers of non-spinning black-hole binaries: Gravitational radiation characteristics, Phys. Rev. D 78, 044046 (2008).
  131. T. Damour and A. Nagar, A new analytic representation of the ringdown waveform of coalescing spinning black hole binaries, Phys. Rev. D 90, 024054 (2014).
  132. L. Blanchet, Post-Newtonian theory for gravitational waves, Living Rev. Relativity 27, 4 (2024).
  133. R. Cotesta, A. Buonanno, A. Bohé, A. Taracchini, I. Hinder, and S. Ossokine, Enriching the symphony of gravitational waves from binary black holes by tuning higher harmonics, Phys. Rev. D 98, 084028 (2018).
  134. C. Mills and S. Fairhurst, Measuring gravitational-wave higher-order multipoles, Phys. Rev. D 103, 024042 (2021).
  135. H. Zhong, M. Isi, K. Chatziioannou, and W. M. Farr, Multidimensional hierarchical tests of general relativity with gravitational waves, Phys. Rev. D 110, 044053 (2024).
  136. A. G. Abac et al., GWTC-4.0: Tests of general relativity, arXiv:2509.0000.
  137. E. Payne, M. Isi, K. Chatziioannou, and W. M. Farr, Fortifying gravitational-wave tests of general relativity against astrophysical assumptions, Phys. Rev. D 108, 124060 (2023).
  138. C. Pacilio, D. Gerosa, and S. Bhagwat, Catalog variance of testing general relativity with gravitational-wave data, Phys. Rev. D 109, L081302 (2024).
  139. W. Del Pozzo and A. Nagar, Analytic family of post-merger template waveforms, Phys. Rev. D 95, 124034 (2017).
  140. A. Nagar, G. Riemenschneider, G. Pratten, P. Rettegno, and F. Messina, Multipolar effective one body waveform model for spin-aligned black hole binaries, Phys. Rev. D 102, 024077 (2020).
  141. N. Yunes, K. Yagi, and F. Pretorius, Theoretical physics implications of the binary black-hole mergers GW150914 and GW151226, Phys. Rev. D 94, 084002 (2016).
  142. A. Maselli, P. Pani, L. Gualtieri, and E. Berti, Parametrized ringdown spin expansion coefficients: A data-analysis framework for black-hole spectroscopy with multiple events, Phys. Rev. D 101, 024043 (2020).
  143. H. O. Silva, A. Ghosh, and A. Buonanno, Black-hole ringdown as a probe of higher-curvature gravity theories, Phys. Rev. D 107, 044030 (2023).
  144. E. M. Sänger et al., Tests of general relativity with GW230529: A neutron star merging with a lower mass-gap compact object, arXiv:2406.03568.
  145. A. K.-W. Chung and N. Yunes, Probing quadratic gravity with black-hole ringdown gravitational waves measured by LIGO-Virgo-KAGRA detectors, arXiv:2506.14695.
  146. V. Cardoso, S. Hopper, C. F. B. Macedo, C. Palenzuela, and P. Pani, Gravitational-wave signatures of exotic compact objects and of quantum corrections at the horizon scale, Phys. Rev. D 94, 084031 (2016).
  147. E. Maggio, L. Buoninfante, A. Mazumdar, and P. Pani, How does a dark compact object ringdown?, Phys. Rev. D 102, 064053 (2020).
  148. S. Alexander and N. Yunes, Chern-Simons modified general relativity, Phys. Rep. 480, 1 (2009).
  149. A. K.-W. Chung, K. K.-H. Lam, and N. Yunes, Quasinormal mode frequencies and gravitational perturbations of spinning black holes in modified gravity through METRICS: The dynamical Chern-Simons gravity case, Phys. Rev. D 111, 124052 (2025).
  150. L. Blanchet, Gravitational radiation from post-Newtonian sources and inspiralling compact binaries, Living Rev. Relativity 17, 2 (2014).
  151. L. Blanchet and B. S. Sathyaprakash, Detecting the tail effect in gravitational wave experiments, Phys. Rev. Lett. 74, 1067 (1995).
  152. L. Blanchet and B. S. Sathyaprakash, Signal analysis of gravitational wave tails, Classical Quantum Gravity 11, 2807 (1994).
  153. K. G. Arun, B. R. Iyer, M. S. S. Qusailah, and B. S. Sathyaprakash, Probing the non-linear structure of general relativity with black hole binaries, Phys. Rev. D 74, 024006 (2006).
  154. N. Yunes and F. Pretorius, Fundamental theoretical bias in gravitational wave astrophysics and the parameterized post-Einsteinian framework, Phys. Rev. D 80, 122003 (2009).
  155. C. K. Mishra, K. G. Arun, B. R. Iyer, and B. S. Sathyaprakash, Parametrized tests of post-Newtonian theory using Advanced LIGO and Einstein Telescope, Phys. Rev. D 82, 064010 (2010).
  156. T. G. F. Li, W. Del Pozzo, S. Vitale, C. Van Den Broeck, M. Agathos, J. Veitch, K. Grover, T. Sidery, R. Sturani, and A. Vecchio, Towards a generic test of the strong field dynamics of general relativity using compact binary coalescence, Phys. Rev. D 85, 082003 (2012).
  157. M. Agathos, W. Del Pozzo, T. G. F. Li, C. Van Den Broeck, J. Veitch, and S. Vitale, TIGER: A data analysis pipeline for testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing compact binaries, Phys. Rev. D 89, 082001 (2014).
  158. A. K. Mehta, A. Buonanno, R. Cotesta, A. Ghosh, N. Sennett, and J. Steinhoff, Tests of general relativity with gravitational-wave observations using a flexible theory-independent method, Phys. Rev. D 107, 044020 (2023).
  159. M. Agathos, W. Del Pozzo, T. G. F. Li, C. Van Den Broeck, J. Veitch, and S. Vitale, TIGER: A data analysis pipeline for testing the strong-field dynamics of general relativity with gravitational wave signals from coalescing compact binaries, Phys. Rev. D 89, 082001 (2014).
  160. J. Meidam et al., Parametrized tests of the strong-field dynamics of general relativity using gravitational wave signals from coalescing binary black holes: Fast likelihood calculations and sensitivity of the method, Phys. Rev. D 97, 044033 (2018).
  161. S. Roy, M. Haney, G. Pratten, P. T. H. Pang, and C. Van Den Broeck, An improved parametrized test of general relativity using the imrphenomx waveform family: Including higher harmonics and precession, arXiv:2504.21147.
  162. G. Pratten et al., Computationally efficient models for the dominant and subdominant harmonic modes of precessing binary black holes, Phys. Rev. D 103, 104056 (2021).
  163. M. Colleoni, F. A. R. Vidal, C. García-Quirós, S. Akçay, and S. Bera, Fast frequency-domain gravitational waveforms for precessing binaries with a new twist, Phys. Rev. D 111, 104019 (2025).
  164. A. Pai and K. G. Arun, Singular value decomposition in parametrised tests of post-Newtonian theory, Classical Quantum Gravity 30, 025011 (2013).
  165. A. A. Shoom, P. K. Gupta, B. Krishnan, A. B. Nielsen, and C. D. Capano, Testing the post-Newtonian expansion with GW170817, Gen. Relativ. Gravit. 55, 55 (2023).
  166. M. Saleem, S. Datta, K. G. Arun, and B. S. Sathyaprakash, Parametrized tests of post-Newtonian theory using principal component analysis, Phys. Rev. D 105, 084062 (2022).
  167. P. Mahapatra et al., Confronting general relativity with principal component analysis: Simulations and results from GWTC-3 events, Phys. Rev. D 112, 104007 (2025).
  168. S. A. Hughes and K. Menou, Golden binaries for LISA: Robust probes of strong-field gravity, Astrophys. J. 623, 689 (2005).
  169. A. Ghosh et al., Testing general relativity using golden black-hole binaries, Phys. Rev. D 94, 021101(R) (2016).
  170. A. Ghosh, N. K. Johnson-McDaniel, A. Ghosh, C. K. Mishra, P. Ajith, W. Del Pozzo, C. P. L. Berry, A. B. Nielsen, and L. London, Testing general relativity using gravitational wave signals from the inspiral, merger and ringdown of binary black holes, Classical Quantum Gravity 35, 014002 (2018).
  171. J. M. Bardeen, W. H. Press, and S. A. Teukolsky, Rotating black holes: Locally nonrotating frames, energy extraction, and scalar synchrotron radiation, Astrophys. J. 178, 347 (1972).
  172. J. Healy and C. O. Lousto, Remnant of binary black-hole mergers: New simulations and peak luminosity studies, Phys. Rev. D 95, 024037 (2017).
  173. X. Jiménez-Forteza, D. Keitel, S. Husa, M. Hannam, S. Khan, and M. Pürrer, Hierarchical data-driven approach to fitting numerical relativity data for nonprecessing binary black holes with an application to final spin and radiated energy, Phys. Rev. D 95, 064024 (2017).
  174. S. W. Hawking, Gravitational radiation from colliding black holes, Phys. Rev. Lett. 26, 1344 (1971).
  175. N. Cornish, L. Sampson, N. Yunes, and F. Pretorius, Gravitational wave tests of general relativity with the parameterized post-Einsteinian framework, Phys. Rev. D 84, 062003 (2011).
  176. M. Vallisneri, Testing general relativity with gravitational waves: A reality check, Phys. Rev. D 86, 082001 (2012).
  177. W. Jia et al. (Members of the LIGO Scientific Collaboration), Squeezing the quantum noise of a gravitational-wave detector below the standard quantum limit, Science 385, 1318 (2024).
  178. D. Ganapathy, V. Xu, W. Jia, C. Whittle, M. Tse, L. Barsotti, M. Evans, and L. McCuller, Probing squeezing for gravitational-wave detectors with an audio-band field, Phys. Rev. D 105, 122005 (2022).
  179. E. Capote et al., Advanced LIGO detector performance in the fourth observing run, Phys. Rev. D 111, 062002 (2025).
  180. LIGO Scientific, Virgo, and KAGRA Collaborations, GWTC-4.0: Population properties of merging compact binaries, arXiv:2508.18083.
  181. B. P. Abbott et al. (LIGO Scientific and Virgo Collaborations), Observation of gravitational waves from a binary black hole merger, Phys. Rev. Lett. 116, 061102 (2016).
  182. B. P. Abbott et al. (KAGRA, LIGO Scientific, and Virgo Collaborations), Prospects for observing and localizing gravitational-wave transients with Advanced LIGO, Advanced Virgo and KAGRA, Living Rev. Relativity 23, 3 (2020).
  183. LIGO Scientific, Virgo, and KAGRA Collaborations, GW250114 GWOSC page (2025), https://gwosc.org/eventapi/html/O4_Discovery_Papers/GW250114_082203/v1/.
  184. LIGO Scientific, Virgo, and KAGRA Collaborations, Black hole spectroscopy and tests of general relativity with GW250114: Data release (2025), https://zenodo.org/records/17018009.
  185. R. Kumar, C. Carroll, A. Hartikainen, and O. Martin, arviz a unified library for exploratory analysis of Bayesian models in python, J. Open Source Software 4, 1143 (2019).
  186. D. Williams, J. Veitch, M. L. Chiofalo, P. Schmidt, R. P. Udall, A. Vajpeji, and C. Hoy, asimov: A framework for coordinating parameter estimation workflows, J. Open Source Software 8, 4170 (2023).
  187. T. P. Robitaille et al. (Astropy Collaboration), astropy: A community python package for astronomy, Astron. Astrophys. 558, A33 (2013).
  188. A. M. Price-Whelan et al. (Astropy Collaboration), The astropy project: Building an open-science project and status of the v2.0 core package, Astron. J. 156, 123 (2018).
  189. A. M. Price-Whelan et al. (Astropy Collaboration), The astropy project: Sustaining and growing a community-oriented open-source project and the latest major release (v5.0) of the core package, Astrophys. J. 935, 167 (2022).
  190. N. J. Cornish, T. B. Littenberg, B. Bécsy, K. Chatziioannou, J. A. Clark, S. Ghonge, and M. Millhouse, bayeswave analysis pipeline in the era of gravitational wave observations, Phys. Rev. D 103, 044006 (2021).
  191. G. Ashton et al., bilby: A user-friendly Bayesian inference library for gravitational-wave astronomy, Astrophys. J. Suppl. Ser. 241, 27 (2019).
  192. I. M. Romero-Shaw et al., Bayesian inference for compact binary coalescences with bilby: Validation and application to the first LIGO–Virgo gravitational-wave transient catalogue, Mon. Not. R. Astron. Soc. 499, 3295 (2020).
  193. G. Ashton, C. Talbot, S. Roy, G. Pratten, T.-H. Pang, M. Agathos, T. Baka, E. Sänger, A. Mehta, J. Steinhoff, E. Maggio, A. Ghosh, A. Vijaykumar, R. Enficiaud, and L. Pompili, bilby_tgr (2025), https://zenodo.org/records/15676285.
  194. W. Del Pozzo and J. Veitch, cpnest: An efficient python parallelizable nested sampling algorithm, https://github.com/johnveitch/cpnest (2025).
  195. J. S. Speagle, dynesty: A dynamic nested sampling package for estimating Bayesian posteriors and evidences, Mon. Not. R. Astron. Soc. 493, 3132 (2020).
  196. D. M. Macleod, J. S. Areeda, S. B. Coughlin, T. J. Massinger, and A. L. Urban, gwpy: A python package for gravitational-wave astrophysics, SoftwareX 13, 100657 (2021).
  197. D. Macleod, S. Coughlin, A. Southgate, D. Davis, M. Pitkin, J. Areeda, R. N. George, P. Altin, P. Godwin, L. Singer et al., gwpy/gwpy: gwpy 3.0.9 (2024), https://zenodo.org/records/12734623.
  198. A. Collette, python and hdf5 (O’Reilly, 2013), https://www.oreilly.com/library/view/python-and-hdf5/9781491944981/.
  199. F. Perez and B. E. Granger, ipython: A system for interactive scientific computing, Comput. Sci. Eng. 9, 21 (2007).
  200. T. Kluyver et al. (Jupyter Development Team), jupyter notebooks—A Publishing Format for Reproducible Computational Workflows (IOS Press, 2016), pp. 87–90, https://ebooks.iospress.nl/publication/42900.
  201. M. Beg, J. Taka, T. Kluyver, A. Konovalov, M. Ragan-Kelley, N. M. Thiéry, and H. Fangohr, Using jupyter for reproducible scientific workflows, Comput. Sci. Eng. 23, 36 (2021).
  202. LIGO Scientific, Virgo, and KAGRA Collaborations, LVK Algorithm Library—lalsuite, Free software (GPL) (2018), https://git.ligo.org/lscsoft/lalsuite.
  203. K. Wette, swiglal: python and octave interfaces to the lalsuite gravitational-wave data analysis libraries, SoftwareX 12, 100634 (2020).
  204. T. A. Caswell, E. S. de Andrade, A. Lee, M. Droettboom, T. Hoffmann, J. Klymak, J. Hunter, E. Firing, D. Stansby, N. Varoquaux et al., matplotlib/matplotlib: Rel: v3.7.3 (2023), https://zenodo.org/records/8336761.
  205. J. D. Hunter, matplotlib: A 2d graphics environment, Comput. Sci. Eng. 9, 90 (2007).
  206. C. R. Harris, K. J. Millman, S. J. van der Walt, R. Gommers, P. Virtanen, D. Cournapeau, E. Wieser, J. Taylor, S. Berg, N. J. Smith et al., Array programming with numpy, Nature (London) 585, 357 (2020).
  207. W. McKinney, Data structures for statistical computing in python, in Proceedings of the 9th python in Science Conference, edited by Stéfan van der Walt and Jarrod Millman (2010), pp. 56–61.
  208. The Pandas Development Team, pandas-dev/pandas: pandas (2024), https://zenodo.org/records/13819579.
  209. C. Hoy and V. Raymond, pesummary: The code agnostic parameter estimation summary page builder, SoftwareX 15, 100765 (2021).
  210. D. P. Mihaylov, S. Ossokine, A. Buonanno, H. Estelles, L. Pompili, M. Pürrer, and A. Ramos-Buades, pyseobnr: A software package for the next generation of effective-one-body multipolar waveform models, SoftwareX 30, 102080 (2025).
  211. G. Van Rossum and F. L. Drake, python 3 Reference Manual (CreateSpace, Scotts Valley, CA, 2009).
  212. L. C. Stein, qnm: A python package for calculating Kerr quasinormal modes, separation constants, and spherical-spheroidal mixing coefficients, J. Open Source Software 4, 1683 (2019).
  213. M. Isi and W. M. Farr, ringdown package, https://ringdown.readthedocs.io/en/latest/ (2024).
  214. P. Virtanen et al. (SciPy 1.0 Contributors), scipy 1.0: Fundamental algorithms for scientific computing in python, Nat. Methods 17, 261 (2020).
  215. R. Gommers, P. Virtanen, M. Haberland, E. Burovski, W. Weckesser, T. Reddy, T. E. Oliphant, D. Cournapeau, A. Nelson et al., scipy/scipy: scipy 1.12.0 (2024), https://zenodo.org/records/10543017.
  216. M. L. Waskom, seaborn: Statistical data visualization, J. Open Source Software 6, 3021 (2021).
  217. M. Khalil, A. Buonanno, H. Estelles, D. P. Mihaylov, S. Ossokine, L. Pompili, and A. Ramos-Buades, Theoretical groundwork supporting the precessing-spin two-body dynamics of the effective-one-body waveform models seobnrv5, Phys. Rev. D 108, 124036 (2023).
  218. M. van de Meent, A. Buonanno, D. P. Mihaylov, S. Ossokine, L. Pompili, N. Warburton, A. Pound, B. Wardell, L. Durkan, and J. Miller, Enhancing the seobnrv5 effective-one-body waveform model with second-order gravitational self-force fluxes, Phys. Rev. D 108, 124038 (2023).
  219. M. Boyle, K. Mitman, M. Scheel, and L. Stein, The sxs package (2025), https://zenodo.org/records/16277847.
  220. C. da Costa-Luis, S. K. Larroque, K. Altendorf, H. Mary, R. Sheridan, M. Korobov, N. Yorav-Raphael, I. Ivanov, M. Bargull, N. Rodrigues et al., tqdm: A fast, extensible progress bar for python and cli (2024), https://zenodo.org/records/14002015.
  221. C. Talbot et al., Inference with finite time series II: The window strikes back, arXiv:2508.11091.
  222. A. G. Abac et al. (LIGO Scientific, Virgo, and KAGRA Collaborations), GWTC-4.0: Methods for identifying and characterizing gravitational-wave transients, arXiv:2508.18081.

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