Open Data from the Third Observing Run of LIGO, Virgo, KAGRA, and GEO
R. Abbott(California Institute of Technology), Haruka Abe(Tokyo Institute of Technology), F. Acernese(University of Salerno), K. Ackley(ARC Centre of Excellence for Gravitational Wave Discovery), S. Adhicary(Pennsylvania State University), N. Adhikari(University of Wisconsin–Milwaukee), R. X. Adhikari(California Institute of Technology), V. K. Adkins(Louisiana State University), V. B. Adya(Australian National University), C. Affeldt(Leibniz University Hannover), D. Agarwal(Inter-University Centre for Astronomy and Astrophysics), M. Agathos(University of Cambridge), O. D. Aguiar(Instituto Nacional de Pesquisas Espaciais), L. Aiello(Cardiff University), A. Ain(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), P. Ajith(Tata Institute of Fundamental Research), T. Akutsu(National Astronomical Observatory of Japan), S. Albanesi(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), R. A. Alfaidi(University of Glasgow), Ammar Al-Jodah(The University of Western Australia), C. Alléné(Centre National de la Recherche Scientifique), A. Allocca(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), M. Almualla(University of Minnesota), P. A. Altin(Australian National University), A. Amato(Maastricht University), L. Amez-Droz(Université Libre de Bruxelles), A. Amorosi(Université Libre de Bruxelles), Shreya Anand(California Institute of Technology), A. Ananyeva(California Institute of Technology), R. Andersen(University of California, Riverside), S. B. Anderson(California Institute of Technology), W. G. Anderson(California Institute of Technology), M. Andia(Centre National de la Recherche Scientifique), Masaki Ando(The University of Tokyo), Tomás Andrade(Universitat de Barcelona), N. Andres(Centre National de la Recherche Scientifique), M. Andrés‐Carcasona(Institució Catalana de Recerca i Estudis Avançats), T. Andrić(Gran Sasso Science Institute), S. Ansoldi(University of Udine), Javier M. Antelis(Embry–Riddle Aeronautical University), S. Antier(Centre National de la Recherche Scientifique), M. Aoumi(The University of Tokyo), Theocharis A. Apostolatos(National and Kapodistrian University of Athens), E. Z. Appavuravther(Università di Camerino), S. Appert(California Institute of Technology), S. K. Apple(American University), K. Arai(California Institute of Technology), A. Araya(The University of Tokyo), M. C. Araya(California Institute of Technology), J. S. Areeda(California State University, Fullerton), M. Arène(Centre National de la Recherche Scientifique), N. Aritomi(National Astronomical Observatory of Japan), N. Arnaud(Centre National de la Recherche Scientifique), M. Arogeti(Georgia Institute of Technology), S. M. Aronson(Louisiana State University), K. G. Arun(Chennai Mathematical Institute), Hideki Asada(Hirosaki University), G. Ashton(Royal Holloway University of London), Yusuke Aso(The Graduate University for Advanced Studies, SOKENDAI), M. Assiduo(University of Urbino), S. Assis de Souza Melo(European Gravitational Observatory), S. M. Aston(LIGO Scientific Collaboration), P. Astone(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), F. Aubin(Istituto Nazionale di Fisica Nucleare, Sezione di Firenze), K. AultONeal(Embry–Riddle Aeronautical University), S. Babak(Centre National de la Recherche Scientifique), A. Badalyan(Andrews University), F. Badaracco(UCLouvain), C. Badger(University of London), S. Bae(Korea Institute of Science & Technology Information), S. Bagnasco(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), Y. Bai(California Institute of Technology), J. G. Baier(Kenyon College), Luca Baiotti(Osaka International University), J. Baird(Centre National de la Recherche Scientifique), R. Bajpai(The Graduate University for Advanced Studies, SOKENDAI), T. Baka(Utrecht University), M. Ball(University of Oregon), G. Ballardin(European Gravitational Observatory), S. Ballmer(Syracuse University), G. Baltus(University of Liège), S. Banagiri(Northwestern University), B. Banerjee(Gran Sasso Science Institute), D. Bankar(Inter-University Centre for Astronomy and Astrophysics), Pratyusava Baral(University of Wisconsin–Milwaukee), J. C. Barayoga(California Institute of Technology), Jordan Barber(Cardiff University), B. C. Barish(California Institute of Technology), D. Barker, P. Barneo(Universitat de Barcelona), F. Barone(University of Salerno), B. Barr(University of Glasgow), L. Barsotti(Massachusetts Institute of Technology), M. Barsuglia(Centre National de la Recherche Scientifique), D. Barta(HUN-REN Wigner Research Centre for Physics), S. D. Barthelmy(Goddard Space Flight Center), M. A. Barton(University of Glasgow), I. Bartos(University of Florida), S. Basak(Tata Institute of Fundamental Research), A. Basalaev(Universität Hamburg), R. Bassiri(Stanford University), A. Basti(University of Pisa), M. Bawaj(University of Perugia), J. C. Bayley(University of Glasgow), A. C. Baylor(University of Wisconsin–Milwaukee), M. Bazzan(University of Padua), B. Bécsy(Montana State University), V. M. Bedakihale(Institute for Plasma Research), F. Beirnaert(Ghent University), M. Bejger(Nicolaus Copernicus Astronomical Center), A. S. Bell(University of Glasgow), V. Benedetto(University of Sannio), D. Beniwal(ARC Centre of Excellence for Gravitational Wave Discovery), William Benoit(University of Minnesota), J. D. Bentley(Universität Hamburg), M. Ben Yaala(University of Strathclyde), Sayantani Bera(Universitat de les Illes Balears), M. Berbel(Universitat Autònoma de Barcelona), F. Bergamin(Leibniz University Hannover), B. K. Berger(Stanford University), Sebastiano Bernuzzi(Friedrich Schiller University Jena), M. Beroiz(California Institute of Technology), C. P. L. Berry(University of Glasgow), D. Bersanetti(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), A. Bertolini(National Institute for Subatomic Physics), J. Betzwieser(LIGO Scientific Collaboration), D. Beveridge(The University of Western Australia), N. Bevins(Villanova University), R. Bhandare(Raja Ramanna Centre for Advanced Technology), A. V. Bhandari(Inter-University Centre for Astronomy and Astrophysics), U. Bhardwaj(National Institute for Subatomic Physics), R. Bhatt(California Institute of Technology), D. Bhattacharjee(Kenyon College), S. Bhaumik(University of Florida), A. Bianchi(National Institute for Subatomic Physics), I. A. Bilenko(Lomonosov Moscow State University), Maciej Bilicki(Center for Theoretical Physics), G. Billingsley(California Institute of Technology), S. Bini(University of Trento), O. Birnholtz(Bar-Ilan University), S. Biscans(California Institute of Technology), M. Bischi(University of Urbino), S. Biscoveanu(Massachusetts Institute of Technology), A. Bisht(Leibniz University Hannover), B. Biswas(Inter-University Centre for Astronomy and Astrophysics), M. Bitossi(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), M. A. Bizouard(Centre National de la Recherche Scientifique), K. Blackburn(California Institute of Technology), C. D. Blair(The University of Western Australia), D. G. Blair(The University of Western Australia), R. M. Blair, F. Bobba(University of Salerno), N. Bode(Leibniz University Hannover), M. Boër(Centre National de la Recherche Scientifique), G. Bogaert(Centre National de la Recherche Scientifique), Guillaume Boileau(Centre National de la Recherche Scientifique), M. Boldrini(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), G. N. Bolingbroke(ARC Centre of Excellence for Gravitational Wave Discovery), L. D. Bonavena(University of Padua), R. Bondarescu(Universitat de Barcelona), F. Bondu(Centre National de la Recherche Scientifique), E. Bonilla(Stanford University), G. S. Bonilla(California State University, Fullerton), R. Bonnand(Centre National de la Recherche Scientifique), P. Booker(Leibniz University Hannover), R. Bork(California Institute of Technology), V. Boschi(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), N. Bose(Indian Institute of Technology Bombay), S. Bose(Inter-University Centre for Astronomy and Astrophysics), V. Bossilkov(The University of Western Australia), V. Boudart(University of Liège), Y. Bouffanais(University of Padua), A. Bozzi(European Gravitational Observatory), C. Bradaschia(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), P. R. Brady(University of Wisconsin–Milwaukee), Matteo Braglia(Universidad Autónoma de Madrid), A. Branch(LIGO Scientific Collaboration), M. Branchesi(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), J. E. Brau(University of Oregon), M. Breschi(Friedrich Schiller University Jena), T. Briant(Centre National de la Recherche Scientifique), A. Brillet(Centre National de la Recherche Scientifique), M. Brinkmann(Leibniz University Hannover), P. Brockill(University of Wisconsin–Milwaukee), A. F. Brooks(California Institute of Technology), J. Brooks(European Gravitational Observatory), D. Brown(ARC Centre of Excellence for Gravitational Wave Discovery), S. Brunett(California Institute of Technology), G. Bruno(UCLouvain), R. Bruntz(Christopher Newport University), John Bryant(University of Birmingham), F. Bucci(Istituto Nazionale di Fisica Nucleare, Sezione di Firenze), J. Buchanan(Christopher Newport University), O. M. Bulashenko(Universitat de Barcelona), T. Bulik(University of Warsaw), H. J. Bulten(National Institute for Subatomic Physics), Alessandra Buonanno(Max Planck Institute for Gravitational Physics), K. Burtnyk, R. Buscicchio(Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca), D. Buskulic(Centre National de la Recherche Scientifique), C. Buy(Centre National de la Recherche Scientifique), R. L. Byer(Stanford University), G. S. Davies(University of Portsmouth), G. Cabras(University of Udine), R. Cabrita(UCLouvain), L. Cadonati(Georgia Institute of Technology), S. Caesar(Cardiff University), G. Cagnoli(Université Claude Bernard Lyon 1), C. Cahillane, J. Calderón Bustillo(Universidade de Santiago de Compostela), J. D. Callaghan(University of Glasgow), T. A. Callister(Flatiron Health (United States)), E. Calloni(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), J. B. Camp(Goddard Space Flight Center), M. Canepa(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), G. Caneva Santoro(Institució Catalana de Recerca i Estudis Avançats), M. Cannavacciuolo(University of Salerno), K. C. Cannon(The University of Tokyo), H. Cao(ARC Centre of Excellence for Gravitational Wave Discovery), Z. Cao(Beijing Normal University), L. A. Capistran(Texas A&M University), E. Capocasa(Centre National de la Recherche Scientifique), E. Capote(Syracuse University), G. Carapella(University of Salerno), F. Carbognani(European Gravitational Observatory), M Carlassara(Leibniz University Hannover), J. B. Carlin(The University of Melbourne), M. Carpinelli(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud), J. J. Carter(Leibniz University Hannover), G. Carullo(University of Pisa), J. Casanueva Diaz(European Gravitational Observatory), C. Casentini(University of Rome Tor Vergata), Giuseppe Castaldi(University of Sannio), S. Y. Castro-Lucas(Colorado State University), S. Caudill(Utrecht University), M. Cavaglià(Missouri University of Science and Technology), R. Cavalieri(European Gravitational Observatory), G. Cella(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), P. Cerdá–Durán(Universitat de València), E. Cesarini(Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata), W. Chaibi(Centre National de la Recherche Scientifique), W. Chakalis(Flatiron Health (United States)), S. Chalathadka Subrahmanya(Universität Hamburg), E. Champion(Rochester Institute of Technology), C. Chan(The University of Tokyo), C. Chan(Chinese University of Hong Kong), Koustav Chandra(Indian Institute of Technology Bombay), I. P. Chang(National Tsing Hua University), W. C. Chang(National Tsing Hua University), P. Chanial(Centre National de la Recherche Scientifique), S. Chao(National Tsing Hua University), C. Chapman-Bird(University of Glasgow), E. L. Charlton(Christopher Newport University), P. Charlton(Charles Sturt University), E. Chassande‐Mottin(Centre National de la Recherche Scientifique), L. Chastain(ARC Centre of Excellence for Gravitational Wave Discovery), C. Chatterjee(The University of Western Australia), Debarati Chatterjee(Inter-University Centre for Astronomy and Astrophysics), Deep Chatterjee(University of Wisconsin–Milwaukee), M. Chaturvedi(Raja Ramanna Centre for Advanced Technology), S. Chaty(Centre National de la Recherche Scientifique), Katerina Chatziioannou(California Institute of Technology), D. Chen(National Astronomical Observatory of Japan), Yu‐Hung Chen(National Tsing Hua University), Yu‐Hung Chen(Massachusetts Institute of Technology), Junxin Chen(Massachusetts Institute of Technology), Kuei‐Hsien Chen(National Central University), X. Chen(The University of Western Australia), Y.-R. Chen(National Tsing Hua University), Yu‐Hung Chen(California Institute of Technology), H.-P. Cheng(University of Florida), P. Chessa(University of Pisa), H. Y. Cheung(Chinese University of Hong Kong), H. Y. Chia(University of Florida), F. Chiadini(University of Salerno), C-I. Chiang(Institute of Physics, Academia Sinica), C. Chiang(National Central University), G. Chiarini(Istituto Nazionale di Fisica Nucleare, Sezione di Padova), A. Chiba(University of Toyama), R. Chiba(The University of Tokyo), R. Chierici(Université Claude Bernard Lyon 1), A. Chincarini(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), Maria Luisa Chiofalo(University of Pisa), A. Chiummo(European Gravitational Observatory), S. Choudhary(Inter-University Centre for Astronomy and Astrophysics), N. Christensen(Centre National de la Recherche Scientifique), S. Chua(Australian National University), K. W. Chung(University of London), G. Ciani(University of Padua), P. Ciecieląg(Nicolaus Copernicus Astronomical Center), M. Cieślar(Nicolaus Copernicus Astronomical Center), M. Cifaldi(University of Rome Tor Vergata), A. A. Ciobanu(ARC Centre of Excellence for Gravitational Wave Discovery), R. Ciolfi(Istituto Nazionale di Fisica Nucleare, Sezione di Padova), F. Clara, J. A. Clark(California Institute of Technology), Teagan A. Clarke(ARC Centre of Excellence for Gravitational Wave Discovery), P. Clearwater(ARC Centre of Excellence for Gravitational Wave Discovery), S. Clesse(Université Libre de Bruxelles), F. Cleva(Centre National de la Recherche Scientifique), E. Coccia(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), E. Codazzo(Gran Sasso Science Institute), P.-F. Cohadon(Centre National de la Recherche Scientifique), M. Colleoni(Universitat de les Illes Balears), Christophe Collette(Université Libre de Bruxelles), A. Colombo(Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca), M. Colpi(Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca), C. M. Compton, L. Conti(Istituto Nazionale di Fisica Nucleare, Sezione di Padova), S. J. Cooper(University of Birmingham), P. Corban(LIGO Scientific Collaboration), T. R. Corbitt(Louisiana State University), I. Cordero-Carrión(Universitat de València), S. Corezzi(University of Perugia), Neil J. Cornish(Montana State University), A. Corsi(Texas Tech University), S. Cortese(European Gravitational Observatory), A. C. Coschizza(University of British Columbia), R. Cottingham(LIGO Scientific Collaboration), M. W. Coughlin(University of Minnesota), J.-P. Coulon(Centre National de la Recherche Scientifique), S. T. Countryman(Columbia University), J.-F. Coupechoux(Université Claude Bernard Lyon 1), B. Cousins(Pennsylvania State University), P. Couvares(California Institute of Technology), D. M. Coward(The University of Western Australia), M. J. Cowart(LIGO Scientific Collaboration), B. D. Cowburn(Rochester Institute of Technology), D. C. Coyne(California Institute of Technology), R. Coyne(University of Rhode Island), K. Craig(University of Strathclyde), J. D. E. Creighton(University of Wisconsin–Milwaukee), J. D. E. Creighton(The University of Texas Rio Grande Valley), A. W. Criswell(University of Minnesota), J. C. G. Crockett-Gray(Louisiana State University), M. Croquette(Centre National de la Recherche Scientifique), S. G. Crowder(Bellevue College), J. R. Cudell(University of Liège), T. J. Cullen(California Institute of Technology), A. Cumming(University of Glasgow), R. Cummings(University of Glasgow), E. Cuoco(Scuola Normale Superiore), M. Curyło(University of Warsaw), P. Dabadie(Université Claude Bernard Lyon 1), T. Dal Canton(Centre National de la Recherche Scientifique), S. Dall’Osso(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), G. Dálya(Ghent University), B. D’Angelo(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), S. L. Danilishin(Maastricht University), S. D’Antonio(Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata), K. Danzmann(Leibniz University Hannover), K. E. Darroch(Christopher Newport University), C. Darsow-Fromm(Universität Hamburg), Arnab Dasgupta(Institute for Plasma Research), L. E. H. Datrier(University of Glasgow), Sayantani Datta(Chennai Mathematical Institute), V. Dattilo(European Gravitational Observatory), I. Dave(Raja Ramanna Centre for Advanced Technology), A. Davenport(Colorado State University), M. Davier(Centre National de la Recherche Scientifique), D. Davis(California Institute of Technology), M. C. Davis(Villanova University), E. J. Daw(University of Sheffield), Maximilian Dax(Max Planck Institute for Gravitational Physics), D. DeBra(Stanford University), M. Deenadayalan(Inter-University Centre for Astronomy and Astrophysics), J. Degallaix(Université Claude Bernard Lyon 1), M. De Laurentis(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), S. Deléglise(Centre National de la Recherche Scientifique), V. Del Favero(Rochester Institute of Technology), F. De Lillo(UCLouvain), N. De Lillo(University of Glasgow), D. Dell’Aquila(University of Sassari), W. Del Pozzo(University of Pisa), F. De Matteis(University of Rome Tor Vergata), V. D’Emilio(Cardiff University), N. Demos(Massachusetts Institute of Technology), T. Dent(Universidade de Santiago de Compostela), A. Depasse(UCLouvain), R. De Pietri(University of Parma), R. De Rosa(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), C. De Rossi(European Gravitational Observatory), R. DeSalvo(University of Sannio), R. De Simone(University of Salerno), S. Dhurandhar(Inter-University Centre for Astronomy and Astrophysics), R. Diab(University of Florida), P. Z. Diamond(Kenyon College), M. C. Díaz(The University of Texas Rio Grande Valley), N. A. Didio(Syracuse University), Tim Dietrich(Max Planck Institute for Gravitational Physics), L. Di Fiore(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), C. Di Fronzo(Université Libre de Bruxelles), C. Di Giorgio(University of Salerno), F. Di Giovanni(Universitat de València), M. Di Giovanni(Gran Sasso Science Institute), T. Di Girolamo(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), D. Diksha(Maastricht University), A. Di Lieto(University of Pisa), Alessandro Di Michele(University of Perugia), S. Di Pace(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), I. Di Palma(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), F. Di Renzo(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), Divyajyoti(Indian Institute of Technology Madras), A. Dmitriev(University of Birmingham), Z. Doctor(Northwestern University), E. Dohmen, P. P. Doleva(Christopher Newport University), L. Donahue(Carleton College), L. D’Onofrio(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), F. Donovan(Massachusetts Institute of Technology), K. L. Dooley(Cardiff University), T. Dooney(Utrecht University), S. Doravari(Inter-University Centre for Astronomy and Astrophysics), O. Dorosh(National Centre for Nuclear Research), M. Drago(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), J. C. Driggers, Y. Drori(California Institute of Technology), J.-G. Ducoin(Centre National de la Recherche Scientifique), L. Dunn(The University of Melbourne), U. Dupletsa(Gran Sasso Science Institute), O. Durante(University of Salerno), D. D’Urso(University of Sassari), P.-A. Duverne(Centre National de la Recherche Scientifique), S. E. Dwyer, C. Eassa, P. J. Easter(ARC Centre of Excellence for Gravitational Wave Discovery), M. Ebersold(University of Zurich), T. Eckhardt(Universität Hamburg), G. Eddolls(University of Glasgow), B. Edelman(University of Oregon), T. B. Edo(California Institute of Technology), O. Edy(University of Portsmouth), A. Effler(LIGO Scientific Collaboration), J. Eichholz(Australian National University), M. Eisenmann(National Astronomical Observatory of Japan), R. A. Eisenstein(Massachusetts Institute of Technology), A. Ejlli(Cardiff University), E. Engelby(California State University, Fullerton), A. J. Engl(Stanford University), L. Errico(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), R. C. Essick(Perimeter Institute), H. Estellés(Max Planck Institute for Gravitational Physics), D. Estevez(Centre National de la Recherche Scientifique), T. Etzel(California Institute of Technology), Christopher Evans(Cardiff University), M. Evans(Massachusetts Institute of Technology), T. M. Evans(LIGO Scientific Collaboration), Tamara Evstafyeva(University of Cambridge), B. E. Ewing(Pennsylvania State University), F. Fabrizi(University of Urbino), F. Faedi(Istituto Nazionale di Fisica Nucleare, Sezione di Firenze), V. Fafone(University of Rome Tor Vergata), H. Fair(Syracuse University), S. Fairhurst(Cardiff University), P. C. Fan(Carleton College), X. Fan(Wuhan University), A. M. Farah(University of Chicago), B. Farr(University of Oregon), Will M. Farr(Flatiron Health (United States)), E. J. Fauchon-Jones(Cardiff University), G. Favaro(University of Padua), M. Favata(Montclair State University), M. Fays(University of Liège), J. Feicht(California Institute of Technology), M. M. Fejer(Stanford University), E. Fenyvesi(HUN-REN Institute for Nuclear Research), D. L. Ferguson(The University of Texas at Austin), A. Fernandez-Galiana(Massachusetts Institute of Technology), I. Ferrante(University of Pisa), T. A. Ferreira(Instituto Nacional de Pesquisas Espaciais), F. Fidecaro(University of Pisa), P. Figura(University of Warsaw), A. Fiori(University of Pisa), I. Fiori(European Gravitational Observatory), M. Fishbach(Northwestern University), R. P. Fisher(Christopher Newport University), R. Fittipaldi(Superconducting and other Innovative Materials and Devices Institute), V. Fiumara(University of Basilicata), R. Flaminio(Centre National de la Recherche Scientifique), S. M. Fleischer(Western Washington University), L. S. Fleming(University of the West of Scotland), E. Floden(University of Minnesota), H. K. Fong(The University of Tokyo), José A. Font(Universitat de València), Bartosz Fornal(University of Utah), P. W. F. Forsyth(Australian National University), A. Franke(Universität Hamburg), S. Frasca(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), F. Frasconi(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), J. P. Freed(Embry–Riddle Aeronautical University), Z. Frei(Eötvös Loránd University), A. Freise(National Institute for Subatomic Physics), O. Freitas(University of Minho), R. Frey(University of Oregon), P. Fritschel(Massachusetts Institute of Technology), V. V. Frolov(LIGO Scientific Collaboration), G. G. Fronzé(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), Yumiko Fujimoto(Osaka City University), I. Fukunaga(Osaka Metropolitan University), P. Fulda(University of Florida), M. Fyffe(LIGO Scientific Collaboration), H. A. Gabbard(University of Glasgow), W. Gabella(Vanderbilt University), B. U. Gadre(Utrecht University), K. Gaglani(Embry–Riddle Aeronautical University), J. R. Gair(Max Planck Institute for Gravitational Physics), J. Gais(Chinese University of Hong Kong), S. Galaudage(ARC Centre of Excellence for Gravitational Wave Discovery), S. Gallardo(California State University Los Angeles), Rossella Gamba(Friedrich Schiller University Jena), D. Ganapathy(Massachusetts Institute of Technology), A. Ganguly(Inter-University Centre for Astronomy and Astrophysics), D. Gao(Stanford University), S. G. Gaonkar(Inter-University Centre for Astronomy and Astrophysics), B. Garaventa(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), J. García-Bellido(Universidad Autónoma de Madrid), C. García‐Núñez(University of the West of Scotland), C. García-Quirós(Universitat de les Illes Balears), K. A. Gardner(University of British Columbia), J. Gargiulo(European Gravitational Observatory), F. Garufi(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), C. Gasbarra(University of Rome Tor Vergata), B. Gateley, V. Gayathri(University of Florida), G. Gemme(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), A. Gennai(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), J. George(Raja Ramanna Centre for Advanced Technology), Oliver Gerberding(Universität Hamburg), L. Gergely(University of Szeged), S. Ghonge(Georgia Institute of Technology), Abhirup Ghosh(Max Planck Institute for Gravitational Physics), Archisman Ghosh(Ghent University), Shaon Ghosh(Montclair State University), Shrobana Ghosh(Cardiff University), Tathagata Ghosh(Inter-University Centre for Astronomy and Astrophysics), L. Giacoppo(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), J. A. Giaime(Louisiana State University), K. D. Giardina(LIGO Scientific Collaboration), Des Gibson(University of the West of Scotland), C. Gier(University of Strathclyde), P. Giri(University of Pisa), F. Gissi(University of Sannio), S. Gkaitatzis(European Gravitational Observatory), J. Glanzer(Louisiana State University), A. E. Gleckl(California State University, Fullerton), F Glotin(Centre National de la Recherche Scientifique), J. Godfrey(University of Oregon), P. Godwin(California Institute of Technology), E. Goetz(University of British Columbia), R. Goetz(University of Florida), Jacob Golomb(California Institute of Technology), B. Goncharov(Gran Sasso Science Institute), G. González(Louisiana State University), M. Gosselin(European Gravitational Observatory), R. Gouaty(Centre National de la Recherche Scientifique), D. W. Gould(Australian National University), Srashti Goyal(Tata Institute of Fundamental Research), B. Grace(Australian National University), A. Grado(Astronomical Observatory of Capodimonte), V. Graham(University of Glasgow), M. Granata(Université Claude Bernard Lyon 1), V. Granata(University of Salerno), S. Gras(Massachusetts Institute of Technology), P. Grassia(California Institute of Technology), C. Gray, R. Gray(Queen Mary University of London), G. Greco(Istituto Nazionale di Fisica Nucleare, Sezione di Perugia), A. C. Green(University of Florida), R. Green(Cardiff University), S.M Green(University of Portsmouth), Stephen Green(Max Planck Institute for Gravitational Physics), A. M. Gretarsson(Embry–Riddle Aeronautical University), E. M. Gretarsson(Embry–Riddle Aeronautical University), D. Griffith(California Institute of Technology), W. L. Griffiths(Cardiff University), H. L. Griggs(Georgia Institute of Technology), G. Grignani(University of Perugia), A. Grimaldi(University of Trento), H. Grote(Cardiff University), A. S. Gruson(California State University, Fullerton), D. Guerra(Universitat de València), D. Guetta(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), G. M. Guidi(University of Urbino), A. R. Guimaraes(Louisiana State University), H. K. Gulati(Institute for Plasma Research), F. Gulminelli(Centre National de la Recherche Scientifique), A. M. Gunny(Massachusetts Institute of Technology), Huai-Ke Guo(University of Utah), Y. Guo(National Institute for Subatomic Physics), Anchal Gupta(California Institute of Technology), Anuradha Gupta(University of Mississippi), Ish Gupta(Pennsylvania State University), N. C. Gupta(Institute for Plasma Research), Anchal Gupta(Utrecht University), Sonam Gupta(Indian Institute of Technology Bombay), J. Gurs(Universität Hamburg), Y. Gushima(Fukuoka University), E. K. Gustafson(California Institute of Technology), N. Gutierrez(Université Claude Bernard Lyon 1), Felipe Guzmán(Texas A&M University), L. Haegel(Centre National de la Recherche Scientifique), G. Hain(Christopher Newport University), S. Haino(Institute of Physics, Academia Sinica), O. Halim(University of Trieste), E. D. Hall(Massachusetts Institute of Technology), E. Z. Hamilton(University of Zurich), G. Hammond(University of Glasgow), Wen-Biao Han(Shanghai Astronomical Observatory), M. Haney(University of Zurich), J. Hanks, C. Hanna(Pennsylvania State University), M. D. Hannam(Cardiff University), O. A. Hannuksela(Chinese University of Hong Kong), H. Hansen, J. Hanson(LIGO Scientific Collaboration), Reiko Harada(The University of Tokyo), T. Harder(Centre National de la Recherche Scientifique), K. Haris(Utrecht University), Troels Harmark, J. Harms(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), G. M. Harry(American University), I. W. Harry(University of Portsmouth), D. Hartwig(Universität Hamburg), B. Haskell(Nicolaus Copernicus Astronomical Center), C.‐J. Haster(Massachusetts Institute of Technology), J. S. Hathaway(Rochester Institute of Technology), K. Haughian(University of Glasgow), Hisashi Hayakawa(The University of Tokyo), K. Hayama(Fukuoka University), F. J. Hayes(University of Glasgow), James Healy(Rochester Institute of Technology), Anna Heffernan(Universitat de les Illes Balears), A. Heidmann(Centre National de la Recherche Scientifique), M. C. Heintze(LIGO Scientific Collaboration), J. Heinze(Leibniz University Hannover), J. Heinzel(Massachusetts Institute of Technology), H. Heitmann(Centre National de la Recherche Scientifique), F. Hellman(University of California, Berkeley), P. Hello(Centre National de la Recherche Scientifique), A. F. Helmling-Cornell(University of Oregon), G. Hemming(European Gravitational Observatory), M. Hendry(University of Glasgow), I. S. Heng(University of Glasgow), E. Hennes(National Institute for Subatomic Physics), J.-S. Hennig(Maastricht University), M Hennig(Maastricht University), C. Henshaw(Georgia Institute of Technology), F. Hernandez Vivanco(ARC Centre of Excellence for Gravitational Wave Discovery), M. Heurs(Leibniz University Hannover), A. Hewitt(University of Cambridge), S. Higginbotham(Cardiff University), S. Hild(Maastricht University), P. Hill(University of Strathclyde), Y. Himemoto(Nihon University), A. S. Hines(Texas A&M University), N. Hirata(National Astronomical Observatory of Japan), C. Hirose(Niigata University), J. Ho(National Central University), S. Hochheim(Leibniz University Hannover), D. Hofman(Université Claude Bernard Lyon 1), J. N. Hohmann(Universität Hamburg), D. G. Holcomb(Villanova University), N. A. Holland(National Institute for Subatomic Physics), Kelly Holley‐Bockelmann(Vanderbilt University), I. J. Hollows(University of Sheffield), Z. J. Holmes(ARC Centre of Excellence for Gravitational Wave Discovery), K. Holt(LIGO Scientific Collaboration), D. E. Holz(University of Chicago), Qi‐Jun Hong(National Tsing Hua University), J. Hornung(University of Oregon), S. Hoshino(Niigata University), J. Hough(University of Glasgow), S. Hourihane(California Institute of Technology), D. A. Howell(Flatiron Health (United States)), E. J. Howell(The University of Western Australia), C. G. Hoy(University of Portsmouth), D. Hoyland(University of Birmingham), B. H. Hsieh(The University of Tokyo), H-F. Hsieh(National Tsing Hua University), C Hsiung(Tamkang University), Han Hsu(National Central University), P. Hu(Vanderbilt University), Qian Hu(University of Glasgow), H. Y. Huang(National Central University), Y.-J. Huang(Pennsylvania State University), Y.-J. Huang(Massachusetts Institute of Technology), Y. T. Huang(University of Washington), M. T. Hübner(The University of Melbourne), A. D. Huddart(Rutherford Appleton Laboratory), B. Hughey(Embry–Riddle Aeronautical University), C. Y. Hui(Chungnam National University), V. Hui(Centre National de la Recherche Scientifique), S. Husa(Universitat de les Illes Balears), S. H. Huttner(University of Glasgow), R. Huxford(Pennsylvania State University), T. Huynh–Dinh(LIGO Scientific Collaboration), J. Hyland(University of Glasgow), A. Iakovlev(Institute of Applied Physics), G.A Iandolo(Maastricht University), B. Idźkowski(University of Warsaw), A. Iess(Scuola Normale Superiore), Kohei Inayoshi(Peking University), Yuki Inoue(National Central University), Giuliano Iorio(University of Padua), P. Iosif(Aristotle University of Thessaloniki), J. Irwin(University of Glasgow), M. Isi(Flatiron Health (United States)), M. A. Ismail(National Central University), Y. Itoh(Osaka City University), B. R. Iyer(Tata Institute of Fundamental Research), V. JaberianHamedan(The University of Western Australia), T. Jacqmin(Centre National de la Recherche Scientifique), P.-E. Jacquet(Centre National de la Recherche Scientifique), S. J. Jadhav(Research & Development Establishment (Engrs.)), S. J. Jadhav(Inter-University Centre for Astronomy and Astrophysics), Devansh Jain(ARC Centre of Excellence for Gravitational Wave Discovery), Tamanna Jain(University of Cambridge), A. L. James(Cardiff University), A. Z. Jan(The University of Texas at Austin), K. Jani(Vanderbilt University), L. Janiurek(University of Glasgow), Justin Janquart(Utrecht University), K. Janssens(Centre National de la Recherche Scientifique), N. N. Janthalur(Research & Development Establishment (Engrs.)), Santiago Jaraba(Universidad Autónoma de Madrid), P. Jaranowski(University of Białystok), S. Jarov(University of British Columbia), P. Jasal(Universitat de Barcelona), R. Jaume(Universitat de les Illes Balears), W. Javed(Cardiff University), A. C. Jenkins(University of London), K. Jenner(ARC Centre of Excellence for Gravitational Wave Discovery), A. Jennings, W. Jia(Massachusetts Institute of Technology), Jun Jiang(University of Florida), J. Liu(The University of Western Australia), H.-B. Jin(National Astronomical Observatories), K. Johansmeyer(Montclair State University), G. R. Johns(Christopher Newport University), N. A. Johnson(University of Florida), Ron Johnston(University of Glasgow), N. Johny(Leibniz University Hannover), A. W. Jones(The University of Western Australia), D. H. Jones(Australian National University), D. I. Jones(University of Southampton), P. Jones(University of Birmingham), R. W. L. Jones(University of Glasgow), Prasanna Joshi(Pennsylvania State University), L. Ju(The University of Western Australia), K. Jung(Ulsan National Institute of Science and Technology), J. Junker(Leibniz University Hannover), V. Juste(Centre National de la Recherche Scientifique), T. Kajita(The University of Tokyo), C. V. Kalaghatgi(Utrecht University), V. Kalogera(Northwestern University), B. Kamai(California Institute of Technology), M. Kamiizumi(The University of Tokyo), Nobuyuki Kanda(Osaka City University), S. Kandhasamy(Inter-University Centre for Astronomy and Astrophysics), G. Kang(Chung-Ang University), J. B. Kanner(California Institute of Technology), S. J. Kapadia(Tata Institute of Fundamental Research), D. P. Kapasi(Australian National University), S. Karat(California Institute of Technology), Christos Karathanasis(Institució Catalana de Recerca i Estudis Avançats), S. Karki(Missouri University of Science and Technology), D. Kasamatsu(University of Toyama), Y. A. Kas-danouche(Andrews University), Rahul Kashyap(Pennsylvania State University), M. Kasprzack(California Institute of Technology), W. Kastaun(Leibniz University Hannover), J. Kato(University of Toyama), S. Katsanevas(European Gravitational Observatory), E. Katsavounidis(Massachusetts Institute of Technology), J. K. Katsuren(Andrews University), W. Katzman(LIGO Scientific Collaboration), T. Kaur(The University of Western Australia), K. Kawabe, K. Kawazoe(Fukuoka University), F. Kéfélian(Centre National de la Recherche Scientifique), D. Keitel(Universitat de les Illes Balears), I. Kellard(Cardiff University), J. Kelley-Derzon(University of Florida), James Kennington(Pennsylvania State University), J. S. Key(University of Washington Bothell), S. Khadka(Stanford University), F. Y. Khalili(Lomonosov Moscow State University), S. Khan(Cardiff University), T. Khanam(Texas Tech University), Е. А. Хазанов(Institute of Applied Physics), M. Khursheed(Raja Ramanna Centre for Advanced Technology), N. Kijbunchoo(Australian National University), Chunglee Kim(Ewha Womans University), J. C. Kim(Inje University), Kyungmin Kim(Ewha Womans University), M. H. Kim(Sungkyunkwan University), P. Kim(Sungkyunkwan University), S. Kim(Chungnam National University), W. S. Kim(National Institute for Mathematical Sciences), Y.-M. Kim(Ulsan National Institute of Science and Technology), C. Kimball(Northwestern University), N. Kimura(The University of Tokyo), M. Kinley-Hanlon(University of Glasgow), R. Kirchhoff(Leibniz University Hannover), J. S. Kissel, T. Kiyota(Osaka Metropolitan University), S. Klimenko(University of Florida), T. Klinger(Cardiff University), A. M. Knee(University of British Columbia), N. Knust(Leibniz University Hannover), Y. Kobayashi(Osaka City University), Patrick M. Koch(Leibniz University Hannover), S. M. Koehlenbeck(Leibniz University Hannover), G. Koekoek(Maastricht University), Kazunori Kohri(High Energy Accelerator Research Organization), K. Kokeyama(Cardiff University), S. Koley(Gran Sasso Science Institute), N. D. Koliadko(Andrews University), P. Kolitsidou(Cardiff University), M. Kolstein(Institució Catalana de Recerca i Estudis Avançats), V. Kondrashov(California Institute of Technology), A. K. H. Kong(National Tsing Hua University), A. Kontos(Bard College), M. Korobko(Universität Hamburg), R. V. Kossak(Leibniz University Hannover), N. Kouvatsos(University of London), M. Kovalam(The University of Western Australia), Naoki Koyama(Niigata University), D. B. Kozak(California Institute of Technology), L. Kranzhoff(Leibniz University Hannover), S. L. Kranzhoff(Maastricht University), V. Kringel(Leibniz University Hannover), N. V. Krishnendu(Leibniz University Hannover), A. Królak(National Centre for Nuclear Research), A. Królak(Leibniz University Hannover), P. G. Kuijer(National Institute for Subatomic Physics), M. Kukihara(Fukuoka University), Sumeet Kulkarni(University of Mississippi), A. Kumar(Research & Development Establishment (Engrs.)), Praveen Kumar(Universidade de Santiago de Compostela), P. Kumar(Tata Institute of Fundamental Research), Rahul Kumar, Rakesh Kumar(Institute for Plasma Research), J. Kume(The University of Tokyo), K. Kuns(Massachusetts Institute of Technology), Sachiko Kuroyanagi(Nagoya University), S. Kuwahara(The University of Tokyo), K. Kwak(Ulsan National Institute of Science and Technology), G. Lacaille(University of Glasgow), P. Lagabbe(Centre National de la Recherche Scientifique), D. Laghi(Centre National de la Recherche Scientifique), M. H. Lakkis(Université Libre de Bruxelles), É. Lalande(Polytechnique Montréal), M Lalleman(University of Antwerp), A. Lamberts(Centre National de la Recherche Scientifique), M. Landry, B. B. Lane(Massachusetts Institute of Technology), R. N. Lang(Massachusetts Institute of Technology), J. Lange(The University of Texas at Austin), B. Lantz(Stanford University), Adele La Rana(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), I. La Rosa(Centre National de la Recherche Scientifique), A. Lartaux-Vollard(Centre National de la Recherche Scientifique), P. D. Lasky(ARC Centre of Excellence for Gravitational Wave Discovery), Jack Lawrence(Texas Tech University), M. Laxen(LIGO Scientific Collaboration), A. Lazzarini(California Institute of Technology), C. Lazzaro(University of Padua), P. Leaci(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), S. Leavey(Leibniz University Hannover), S. LeBohec(University of Utah), Y. K. Lecoeuche(University of British Columbia), Hyung Mok Lee(The University of Tokyo), Hyung Mok Lee(Seoul National University), H. W. Lee(Inje University), H. K. Lee(Sungkyunkwan University), R.-L. Lee(Massachusetts Institute of Technology), R. Lee(Massachusetts Institute of Technology), S. Lee(Korea Astronomy and Space Science Institute), Isaac Legred(California Institute of Technology), J. Lehmann(Leibniz University Hannover), Luis Lehner(Perimeter Institute), A. Lemaître(Centre National de la Recherche Scientifique), M. Lenti(Istituto Nazionale di Fisica Nucleare, Sezione di Firenze), M. Leonardi(National Astronomical Observatory of Japan), E. Leonova(University of Amsterdam), N. Leroy(Centre National de la Recherche Scientifique), N. Letendre(Centre National de la Recherche Scientifique), M. Lethuillier(Université Claude Bernard Lyon 1), C. Lévesque(Polytechnique Montréal), Y. Levin(ARC Centre of Excellence for Gravitational Wave Discovery), K. Leyde(Centre National de la Recherche Scientifique), A. K. Y. Li(California Institute of Technology), Kwan-Lok Li(National Cheng Kung University), Tjonnie G. F. Li(Chinese University of Hong Kong), X. Li(California Institute of Technology), Chun-Yu Lin(National Central University), E. T. Lin(National Tsing Hua University), F-K. Lin(Institute of Physics, Academia Sinica), F-L. Lin(National Taiwan Normal University), Feng-Li Lin(National Central University), H. L. Lin(National Central University), H. L. Lin(National Cheng Kung University), L. C.-C. Lin(National Institute for Subatomic Physics), F. Linde(University of Sannio), S. D. Linker(Marshall Space Flight Center), T. B. Littenberg(Chinese University of Hong Kong), A. Liu(Tamkang University), Guo-Chin Liu(The University of Texas Rio Grande Valley), F. Llamas(California Institute of Technology), R. K. L. Lo(National Tsing Hua University), T. Lo(Massachusetts Institute of Technology), L. T. London(Istituto Nazionale di Fisica Nucleare, Sezione di Roma Tre), A. Longo(University of Zurich), D. Lopez(Utrecht University), M. Lopez Portilla(University of Rome Tor Vergata), M. Lorenzini(Centre National de la Recherche Scientifique), V. Loriette(LIGO Scientific Collaboration), M. Lormand(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), G. Losurdo(Georgia Institute of Technology), T. P. Lott(Leibniz University Hannover), J. D. Lough(Massachusetts Institute of Technology), Hudson A. Loughlin(Rochester Institute of Technology), C. O. Loustó(California State University, Fullerton), Geoffrey Lovelace(Christopher Newport University), M.J Lowry(Leibniz University Hannover), H. Lück(University of Rome Tor Vergata), D. Lumaca(University of Portsmouth), A. P. Lundgren(Chinese University of Hong Kong), Y. Lung(Polytechnique Montréal), A. W. Lussier(Christopher Newport University), J. E. Lynam(National Tsing Hua University), Longfei Ma(California Institute of Technology), Sizheng Ma(National Central University), M. Ma’arif(University of Portsmouth), R. Macas(Massachusetts Institute of Technology), M. MacInnis(Cardiff University), D. M. Macleod(California Institute of Technology), I. A. O. MacMillan(Institució Catalana de Recerca i Estudis Avançats), A. Macquet(University of Wisconsin–Milwaukee), I. Magaña Hernandez(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), C. Magazzù(California Institute of Technology), R. M. Magee(National Institute for Subatomic Physics), R. Maggiore(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), M. Magnozzi(Universität Hamburg), M. Mahesh(West Virginia University), S. Mahesh(University of Rhode Island), M. Maini(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), E. Majorana(California Institute of Technology), C. N. Makarem(California Institute of Technology), S. Maliakal(Raja Ramanna Centre for Advanced Technology), A. Malik(Centre National de la Recherche Scientifique), N. Man(University of Minnesota), Vuk Mandic(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), V. Mangano(University of Oregon), B. Mannix(Massachusetts Institute of Technology), G. L. Mansell(American University), G. Mansingh(University of Wisconsin–Milwaukee), M. Manske(European Gravitational Observatory), M. Mantovani(University of Padua), Michela Mapelli(Università di Camerino), F. Marchesoni(Institut d'Estudis Espacials de Catalunya), D. Marín Pina(Centre National de la Recherche Scientifique), F. Marion(Columbia University), Szabolcs Márka(Columbia University), Z. Márka(Queen Mary University of London), C. Markakis(Stanford University), A. S. Markosyan(California Institute of Technology), A. Markowitz(California Institute of Technology), E. Maros(Universitat de València), Antonio Marquina(Centre National de la Recherche Scientifique), S. Marsat(University of Urbino), F. Martelli(University of Glasgow), I. W. Martin(Montclair State University), R. M. Martin(Texas A&M University), B. B. Martinez(Institució Catalana de Recerca i Estudis Avançats), M. Martı́nez(University of Florida), V. A. Martinez(Université Claude Bernard Lyon 1), V. Martínez(University of London), K. Martinovic(University of Birmingham), Д. В. Мартынов(Massachusetts Institute of Technology), E. J. Marx(Universität Hamburg), H. Masalehdan(Massachusetts Institute of Technology), K. Mason(Centre National de la Recherche Scientifique), A. Masserot(University of Glasgow), M. Masso‐Reid(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), M. Mastrodicasa(Centre National de la Recherche Scientifique), S. Mastrogiovanni(Universitat de les Illes Balears), M. Mateu-Lucena(Leibniz University Hannover), M. Matiushechkina(University of Toyama), K. Matsunaga(Massachusetts Institute of Technology), N. Mavalvala, R. McCarthy(Australian National University), D. E. McClelland(Pennsylvania State University), P. K. McClincy(LIGO Scientific Collaboration), S. McCormick(California Institute of Technology), L. McCuller(University of Glasgow), G. I. McGhee(University of Glasgow), J Mcginn(University of Portsmouth), C. McIsaac(University of British Columbia), J. McIver(The University of Western Australia), A. McLeod(Australian National University), T. McRae(West Virginia University), S. T. McWilliams(University of Wisconsin–Milwaukee), D. Meacher(Leibniz University Hannover), M. Mehmet(Max Planck Institute for Gravitational Physics), A. K. Mehta(Utrecht University), Q. Meijer(The University of Melbourne), A. Melatos, G. Mendell(Institució Catalana de Recerca i Estudis Avançats), A. Menéndez-Vázquez(Colorado State University), Carmen S. Menoni(University of Wisconsin–Milwaukee), R. A. Mercer(Université Claude Bernard Lyon 1), L. Mereni(University of Oregon), K. Merfeld(LIGO Scientific Collaboration), E. L. Merilh(University of Oregon), J. D. Merritt(Centre National de la Recherche Scientifique), M. Merzougui(University of Glasgow), C. Messenger(Massachusetts Institute of Technology), C. Messick(California Institute of Technology), P. M. Meyers(Leibniz University Hannover), F. Meylahn(Inter-University Centre for Astronomy and Astrophysics), A. Mhaske(University of Trento), A. Miani(Tsinghua University), H. Miao(University of Florida), I. Michaloliakos(Université Claude Bernard Lyon 1), C. Michel(California Institute of Technology), Yuta Michimura(University of Birmingham), H. Middleton(Max Planck Institute for Gravitational Physics), Deyan P. Mihaylov(California State University Los Angeles), A. L. Miller(UCLouvain), A. L. Miller(National Institute for Subatomic Physics), B. Miller(California Institute of Technology), Simona J. Miller(Georgia Institute of Technology), M. Millhouse(Cardiff University), J. C. Mills(University of Trieste), E. Milotti(Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata), Y. Minenkov(The University of Tokyo), N. Mio(Institució Catalana de Recerca i Estudis Avançats), Ll. M. Mir(Universitat de València), M. Miravet-Tenés(Inter-University Centre for Astronomy and Astrophysics), Arvind Kumar Mishra(Indian Institute of Technology Madras), C. Mishra(University of Florida), T. Mishra(University of Sheffield), T. Mistry(National Institute for Subatomic Physics), A. L. Mitchell(Inter-University Centre for Astronomy and Astrophysics), S. Mitra(Lomonosov Moscow State University), V. P. Mitrofanov(University of Florida), G. Mitselmakher(Massachusetts Institute of Technology), R. Mittleman(The University of Tokyo), O. Miyakawa(The University of Tokyo), S. Miyoki(Massachusetts Institute of Technology), Geoffrey Mo(Universitat de les Illes Balears), L. M. Modafferi(Kenyon College), E. Moguel(Massachusetts Institute of Technology), M. Mondin(University of Wisconsin–Milwaukee), S. R. Mohite(University of California, Berkeley), M. Molina-Ruiz(Centre National de la Recherche Scientifique), C. Mondal(California State University Los Angeles), M. Mondin(University of Urbino), M. Montani(University of Birmingham), C. J. Moore(Universitat de les Illes Balears), J. Moragues, D. Moraru(Nicolaus Copernicus Astronomical Center), F. Morawski(Inter-University Centre for Astronomy and Astrophysics), Anupreeta More(Inter-University Centre for Astronomy and Astrophysics), Surhud More(Embry–Riddle Aeronautical University), Claudia Moreno, G. Moreno(University of Wisconsin–Milwaukee), S. Morisaki(University of Toyama), Yoshiki Moriwaki(Universidad Autónoma de Madrid), Gonzalo Morrás(University of Padua), A. Moscatello(Centre National de la Recherche Scientifique), B. Mours(National Institute for Subatomic Physics), C. M. Mow–Lowry(University of Portsmouth), S. Mozzon(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), F. Muciaccia(Marshall Space Flight Center), Debnandini Mukherjee(The University of Texas Rio Grande Valley), Soma Mukherjee(Institute for Plasma Research), S. Mukherjee(Tata Institute of Fundamental Research), Suvodip Mukherjee(Leibniz University Hannover), N. Mukund(LIGO Scientific Collaboration), A. Mullavey(ARC Centre of Excellence for Gravitational Wave Discovery), J. Münch(Syracuse University), E. A. Muñiz(University of Glasgow), P. G. Murray(Cardiff University), J. Murray-Dean(ARC Centre of Excellence for Gravitational Wave Discovery), S. Muusse(Leibniz University Hannover), S. L. Nadji(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), A. Nagar(ARC Centre of Excellence for Gravitational Wave Discovery), Tushar Nagar(University of Glasgow), N. Nagarajan(National Astronomical Observatory of Japan), K. Nakamura(Ryukoku University), Hiroyuki Nakano(LIGO Scientific Collaboration), M. Nakano(University of Toyama), Y. Nakayama(European Gravitational Observatory), V. Napolano(University of Rome Tor Vergata), I. Nardecchia(The University of Tokyo), T. Narikawa(Utrecht University), Harsh Narola(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), L. Naticchioni(Indian Institute of Science Education and Research Kolkata), R. K. Nayak(The University of Western Australia), B. F. Neil(University of Sannio), J. Neilson(Texas A&M University), A. Nelson(LIGO Scientific Collaboration), T. J. N. Nelson(Leibniz University Hannover), M. Nery(Universidad Autónoma de Madrid), Savvas Nesseris(University of Washington Bothell), A. Neunzert(Massachusetts Institute of Technology), K.Y. Ng(ARC Centre of Excellence for Gravitational Wave Discovery), S. Ng(Centre National de la Recherche Scientifique), C. Nguyen(University of Oregon), P. Nguyen(Cardiff University), R. Nguyen(Massachusetts Institute of Technology), T. Nguyen(University of Notre Dame), L. Nguyen Quynh(Louisiana State University), S. A. Nichols(Nicolaus Copernicus Astronomical Center), G. Nieradka(National Astronomical Observatory of Japan), Y. Nishino(The University of Tokyo), A. Nishizawa(National Institute for Subatomic Physics), S. Nissanke(Université Claude Bernard Lyon 1), E. Nitoglia(Pennsylvania State University), W. Niu(European Gravitational Observatory), F. Nocera(Cardiff University), M. Norman(Cardiff University), C. North(Centre National de la Recherche Scientifique), J. Novák(Universidad Autónoma de Madrid), J. F. Nuño Siles(The University of Texas Rio Grande Valley), G. Nurbek(University of Portsmouth), L. K. Nuttall, J. Oberling(Rutherford Appleton Laboratory), J. O’Dell(University of Glasgow), E. Oelker(Centre National de la Recherche Scientifique), Micaela Oertel(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), G. Oganesyan(National Institute for Mathematical Sciences), J. J. Oh(Chungnam National University), Kyuseok Oh(National Institute for Mathematical Sciences), S. H. Oh(LIGO Scientific Collaboration), T. O’Hanlon(The University of Tokyo), M. Ohashi(Osaka City University), T. Ohashi(Niigata University), Masashi Ohkawa(Leibniz University Hannover), F. Ohme(The University of Tokyo), H. Ohta(Columbia University), A. S. Oliveira(Centre National de la Recherche Scientifique), Roberto Oliveri(The Open University of Japan), K. Oohara(LIGO Scientific Collaboration), B. O’Reilly(University of Minnesota), R. G. Ormiston(Christopher Newport University), N. D. Ormsby(University of Perugia), Marta Orselli(Rochester Institute of Technology), R. O’Shaughnessy(Cornell University), E. O’Shea(The University of Tokyo), Y. Oshima(The University of Tokyo), S. Oshino(Max Planck Institute for Gravitational Physics), Serguei Ossokine(California Institute of Technology), C. Osthelder(ARC Centre of Excellence for Gravitational Wave Discovery), D. J. Ottaway(LIGO Scientific Collaboration), H. Overmier(Pennsylvania State University), A. E. Pace(Louisiana State University), R. Pagano(National Astronomical Observatory of Japan), M. A. Page(Indian Institute of Technology Bombay), Archana Pai(Raja Ramanna Centre for Advanced Technology), S. A. Pai(Indian Institute of Science Education and Research Kolkata), S. Pal(Institute of Applied Physics), O. Palashov(Eötvös Loránd University), M Pálfi(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), C. Palomba(National Tsing Hua University), K. Pan(Research & Development Establishment (Engrs.)), K. Pan(Utrecht University), P. T. H. Pang(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), F. Pannarale(Raja Ramanna Centre for Advanced Technology), B. C. Pant(The University of Western Australia), F. H. Panther(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), F. Paoletti(European Gravitational Observatory), A. Paoli(Institute for Complex Systems), A. Paolone(University of California, Riverside), Evangelos E. Papalexakis(Aristotle University of Thessaloniki), G. Pappas(Scuola Normale Superiore), A. Parisi(Korea Astronomy and Space Science Institute), J. Park(LIGO Scientific Collaboration), W. Parker(Ghent University), D. Pascucci(European Gravitational Observatory), A. Pasqualetti(University of Pisa), R. Passaquieti(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), D. Passuello(Christopher Newport University), M. Patel(ARC Centre of Excellence for Gravitational Wave Discovery), M. Pathak(Cardiff University), A. Patra(University of Pisa), B. Patricelli(Louisiana State University), A.S Patron(University of Oregon), S. Paul(California Institute of Technology), Ethan Payne(Cardiff University), T. Pearce(California Institute of Technology), M. Pedraza(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), R. Pedurand(University of Pisa), R. Pegna(Istituto Nazionale di Fisica Nucleare, Sezione di Padova), M. Pegoraro(California Institute of Technology), A. Pele(The University of Tokyo), F. E. Peña Arellano(Hobart and William Smith Colleges), S. Penn(University of Trento), Albino Perego(Université Claude Bernard Lyon 1), A. Pereira, C. J. Perez(Osservatorio Astronomico di Padova), C. Périgois(University of Florida), C. C. Perkins(University of Trento), A. Perreca(Université Claude Bernard Lyon 1), S. Perriès(National Institute for Subatomic Physics), J. W. Perry(Aristotle University of Thessaloniki), D Pesios(Universität Hamburg), J. Petermann(University of Perugia), C. Petrillo(Max Planck Institute for Gravitational Physics), Harald Pfeiffer(LIGO Scientific Collaboration), H. Pham(University of Minnesota), K. A. Pham(National Institute for Subatomic Physics), K. S. Phukon(Chinese University of Hong Kong), Hemanta Phurailatpam(Institució Catalana de Recerca i Estudis Avançats), O. J. Piccinni(Centre National de la Recherche Scientifique), M. Pichot(University of Pisa), M. Piendibene(University of Urbino), F. Piergiovanni(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), L. Pierini(Université Claude Bernard Lyon 1), G. Pierra(University of Sannio), V. Pierro(European Gravitational Observatory), G. Pillant(Centre National de la Recherche Scientifique), G. Pierra(Istituto Nazionale di Fisica Nucleare, Sezione di Pisa), F. Pilo(Université Claude Bernard Lyon 1), L. Pinard(California State University Los Angeles), C. Pineda-Bosque(University of Sannio), I. M. Pinto(University of Wisconsin–Milwaukee), B. J. Piotrzkowski(UCLouvain), K. Piotrzkowski, M. Pirello(University of Cambridge), M. Pitkin(University of Perugia), A. Placidi(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), E. Placidi(Universitat de les Illes Balears), M. L. Planas(Roma Tre University), W. Plastino(University of Pisa), R. Poggiani(Centre National de la Recherche Scientifique), E. Polini(Max Planck Institute for Gravitational Physics), Lorenzo Pompili(Chinese University of Hong Kong), D. Y. T. Pong(Inter-University Centre for Astronomy and Astrophysics), S. Ponrathnam(National Institute for Subatomic Physics), E. Porcelli(Institut d'Estudis Espacials de Catalunya), J. Portell(Centre National de la Recherche Scientifique), E. K. Porter(Pennsylvania State University), C. Posnansky(European Gravitational Observatory), R. Poulton(ARC Centre of Excellence for Gravitational Wave Discovery), J. Powell(Cardiff University), Jonathan Powell(Centre National de la Recherche Scientifique), M. Pracchia(Centre National de la Recherche Scientifique), T. Pradier(Institute for Plasma Research), A. K. Prajapati(Stanford University), K. Prasai(Research & Development Establishment (Engrs.)), R. Prasanna(University of Birmingham), G. Pratten(University of Sannio), M. Principe(University of Trento), G. A. Prodi(University of Birmingham), L. Prokhorov(University of Rome Tor Vergata), P. Prosposito(Max Planck Institute for Gravitational Physics), L. Prudenzi(Utrecht University), A. Puecher(Louisiana State University), Jorge Pullin(Istituto Nazionale di Fisica Nucleare, Sezione di Perugia), M. Punturo(University of Pisa), F. Puosi(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), P. Puppo(Max Planck Institute for Gravitational Physics), M. Pürrer(Louisiana State University), H. Qi(The University of Texas Rio Grande Valley), V. Quetschke(Embry–Riddle Aeronautical University), P. J. Quinonez(Missouri University of Science and Technology), R. Quitzow-James, F. J. Raab(National Institute for Subatomic Physics), G. Raaijmakers(Centre National de la Recherche Scientifique), N. Radulesco(Eötvös Loránd University), P. Raffai(Polytechnique Montréal), S. X. Rail(Raja Ramanna Centre for Advanced Technology), S. Raja(Raja Ramanna Centre for Advanced Technology), C. Rajan(LIGO Scientific Collaboration), K. E. Ramirez(California State University, Fullerton), T. D. Ramirez(Max Planck Institute for Gravitational Physics), A. Ramos-Buades(Inter-University Centre for Astronomy and Astrophysics), Divya Rana(Pennsylvania State University), J. Rana(Colorado State University), E. Randel(Stanford University), P. R. Rangnekar(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), P. Rapagnani(University of Wisconsin–Milwaukee), Anarya Ray(Cardiff University), V. Raymond(University of British Columbia), N. Raza(University of Pisa), M. Razzano(California State University, Fullerton), J. Read(Centre National de la Recherche Scientifique), T. Regimbau(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), L. Rei(University of Strathclyde), S. Reid(Christopher Newport University), S. W. Reid(California Institute of Technology), D. H. Reitze(Cardiff University), P. Relton(California Institute of Technology), A. Renzini(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), P. Rettegno(Centre National de la Recherche Scientifique), B. Revenu(National Institute for Subatomic Physics), A. Reza(California State University, Fullerton), M. Rezac(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), A. S. Rezaei(Istituto Nazionale di Fisica Nucleare, Sezione di Roma I), F. Ricci(Rutherford Appleton Laboratory), Daniel A. Richards(University of California, Riverside), J. W. Richardson(Embry–Riddle Aeronautical University), A. Rijal(University of Michigan), K. Riles(Cardiff University), H. K. Riley(University of Pisa), S. Rinaldi(Rutherford Appleton Laboratory), C. W. Robertson(California Institute of Technology), N. A. Robertson(Centre National de la Recherche Scientifique), F. Robinet(Istituto Nazionale di Fisica Nucleare, Roma Tor Vergata), A. Rocchi(California State University, Fullerton), Saul Rodriguez(Centre National de la Recherche Scientifique), L. Rolland(California Institute of Technology), J. G. Rollins(Centre National de la Recherche Scientifique), M. Romanelli(University of Salerno), R. Romano, C. L. Romel(Institució Catalana de Recerca i Estudis Avançats), A. Romero(ARC Centre of Excellence for Gravitational Wave Discovery), I. M. Romero-Shaw(LIGO Scientific Collaboration), J. H. Romie(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran Sasso), S. Ronchini(ARC Centre of Excellence for Gravitational Wave Discovery), T. J. Roocke(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), Luigi Rosa(University of California, Riverside), T. J. Rosauer(University of Wisconsin–Milwaukee), C. A. Rose(University of Warsaw), D. Rosińska(University of Washington), M. P. Ross(Universitat de les Illes Balears), M. Rossello(Cardiff University), A. Roussel(University of Glasgow), S. Rowan(University of Birmingham), S. J. Rowlinson(Utrecht University), Soumen Roy(University of Utah), A. Royzman(University of Sassari), D. Rozza(European Gravitational Observatory), P. Ruggi(Universidad Autónoma de Madrid), E. Ruiz Morales(Vanderbilt University), K. Ruiz-Rocha, K. Ryan(Georgia Institute of Technology), S. Sachdev, T. Sadecki(Universidade de Santiago de Compostela), J. Sadiq(National Institute for Subatomic Physics), P. Saffarieh(National Tsing Hua University), S. S. Saha(High Energy Accelerator Research Organization), Surojit Saha(High Energy Accelerator Research Organization), Y. Saito(Nagaoka National College of Technology), K. Sakai(University of London), Mairi Sakellariadou(University of Toyama), T. Sako(Pennsylvania State University), S. Sakon(Brera Astronomical Observatory), O. S. Salafia(California Institute of Technology), F. Salces-Cárcoba(European Gravitational Observatory), L. Salconi(University of Minnesota), M. Saleem(University of Trento), F. Salemi(National Institute for Subatomic Physics), M. Sallé(Istituto Nazionale di Fisica Nucleare, Sezione di Milano Bicocca), A. Samajdar(California Institute of Technology), E. J. Sanchez(Northwestern University), J. H. Sanchez(California Institute of Technology), L. E. Sanchez(Universitat de València), N. Sanchis-Gual(Marquette University), J. R. Sanders(Universitat de Barcelona), A. Sanuy(Inter-University Centre for Astronomy and Astrophysics), T. R. Saravanan(ARC Centre of Excellence for Gravitational Wave Discovery), Nikhil Sarin(Aristotle University of Thessaloniki), A. Sasli(University of Perugia), Paola Sassi(Université Claude Bernard Lyon 1), B. Sassolas(The University of Western Australia), H. Satari(University of Florida), O. Sauter, R. L. Savage(Inter-University Centre for Astronomy and Astrophysics), V. Savant(Osaka City University), T. Sawada(Inter-University Centre for Astronomy and Astrophysics), H. L. Sawant(Université Claude Bernard Lyon 1), S. Sayah(California Institute of Technology), D. Schaetzl(California Institute of Technology), M. Scheel(Stanford University), S. J. Scherf(Northwestern University), Jacob Scheuer(ARC Centre of Excellence for Gravitational Wave Discovery), M. G. Schiworski(University of Birmingham), P. Schmidt(Utrecht University), S. Schmidt(Kenyon College), S. J. Schmitz(Universität Hamburg), Roman Schnabel(Leibniz University Hannover), M. Schneewind(University of Oregon), R. M. S. Schofield(Universität Hamburg), A. Schönbeck(Pennsylvania State University), H. Schuler(Leibniz University Hannover), B. W. Schulte(Leibniz University Hannover), B. F. Schutz(Cardiff University), E. Schwartz(University of Glasgow), J. Scott(Australian National University), S. M. Scott(University of Glasgow), T. C. Seetharamu(Centre National de la Recherche Scientifique), M. Seglar-Arroyo(Toho University), Yuichiro Sekiguchi(LIGO Scientific Collaboration), D. Sellers(Indian Institute of Technology Gandhinagar), A. S. Sengupta(European Gravitational Observatory), D. Sentenac(Chinese University of Hong Kong), E. G. Seo(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), V. Sequino(Institute of Applied Physics), A. Sergeev(Laboratoire Univers et Théories), G. Servignat(Utrecht University), Y. Setyawati, T. Shaffer(Northwestern University), M. S. Shahriar(Seoul National University), Md Arif Shaikh(University of Utah), B. Shams(Peking University), Lijing Shao(Raja Ramanna Centre for Advanced Technology), P. Sharma(Missouri University of Science and Technology), Sushant Sharma Chaudhary(University of Maryland, College Park), P. Shawhan(Centre National de la Recherche Scientifique), N. S. Shcheblanov(Indian Institute of Technology Madras), A. Sheela(University of Maryland, College Park), Bowen Shen(Andrews University), K. G. Shepard(Vanderbilt University), E. Sheridan(Gunma University), Yutaka Shikano(The University of Tokyo), M. Shikauchi(High Energy Accelerator Research Organization), H. Shimizu(The University of Tokyo), K. Shimode(Osaka Institute of Technology), H. Shinkai(Massachusetts Institute of Technology), D. H. Shoemaker(The University of Texas at Austin), Deirdre Shoemaker(Raja Ramanna Centre for Advanced Technology), S. ShyamSundar(Université Libre de Bruxelles), A. Sider(Flatiron Health (United States)), H. Siegel(UCLouvain), M. Sieniawska, D. Sigg(Università di Camerino), L. Silenzi(Goddard Space Flight Center), L. P. Singer(Pennsylvania State University), D. Singh(Tata Institute of Fundamental Research), M. K. Singh(University of Warsaw), N. Singh(Maastricht University), A. Singha(Universitat de les Illes Balears), A. M. Sintes(University of Sassari), N. Singh(Cardiff University), V. Skliris(Australian National University), B. J. J. Slagmolen(The University of Western Australia), T. J. Slaven-Blair(University of Birmingham), J. Smetana(California State University, Fullerton), J. R. Smith(University of Glasgow), L. Smith(ARC Centre of Excellence for Gravitational Wave Discovery), R. J. E. Smith(Arcetri Astrophysical Observatory), J. Soldateschi(Indian Institute of Technology Hyderabad), S. Somala(Tokyo Institute of Technology), K. Somiya(Inter-University Centre for Astronomy and Astrophysics), K. Soni(Massachusetts Institute of Technology), S. Soni(Université Claude Bernard Lyon 1), V. Sordini(Istituto Nazionale di Fisica Nucleare, Sezione di Genova), F. Sorrentino(University of Pisa), N. Sorrentino(RIKEN), Hajime Sotani(Centre National de la Recherche Scientifique), R. Soulard(Indian Institute of Science Education and Research Pune), T. Souradeep(Texas Tech University), E. Sowell(Maastricht University), V. Spagnuolo(University of Glasgow), A. P. Spencer(University of Padua), Mario Spera(European Gravitational Observatory), P Spinicelli(Institute for Plasma Research), A. K. Srivastava(Syracuse University), V. Srivastava(Centre National de la Recherche Scientifique), C. Stachie(University of Glasgow), F. Stachurski(Centre National de la Recherche Scientifique), D. A. Steer(Maastricht University), J. Steinlechner(Maastricht University), S. Steinlechner(Aristotle University of Thessaloniki), Nikolaos Stergioulas(University of Rhode Island), M. StPierre(The University of Melbourne), L. C. Strang(Goethe University Frankfurt), G. Stratta(Louisiana State University), M. D. Strong, A. Strunk(Universidade Estadual Paulista (Unesp)), R. Sturani(Villanova University), A. L. Stuver(Nicolaus Copernicus Astronomical Center), M. Suchenek(Inter-University Centre for Astronomy and Astrophysics), S. Sudhagar(Universität Hamburg), N. Sueltmann(The University of Tokyo), T. Sugiyama(University of Wisconsin–Milwaukee), H. G. Suh(Columbia University), Andrew G. Sullivan(Andrews University), T. Z. Summerscales(Australian National University), L. Sun(Institute for Plasma Research), L. Sun(Nicolaus Copernicus Astronomical Center), A. Sur(The University of Tokyo), J. Suresh(Cardiff University), P. J. Sutton(Niigata University), Takamasa Suzuki(Tokyo Institute of Technology), Takanori Suzuki(National Institute for Subatomic Physics), B. L. Swinkels(Centre National de la Recherche Scientifique), A. Syx(University of Florida), M. J. Szczepańczyk(University of Warsaw), P. Szewczyk(National Institute for Subatomic Physics), M. Tacca(The University of Tokyo), Hideyuki Tagoshi(University of Glasgow), S. C. Tait(Tokyo City University), Hirotaka Takahashi(National Astronomical Observatory of Japan), Ryutaro Takahashi(The University of Tokyo), A. Takamori(The University of Tokyo), S. Takano(Kyoto University), H. Takeda(Osaka Metropolitan University), M. Takeda(University of Strathclyde), C. J. Talbot(Massachusetts Institute of Technology), C. Talbot(The University of Tokyo), M. Tamaki(Centre National de la Recherche Scientifique), Nicola Tamanini(National Central University), D. Tanabe(The University of Tokyo), K. Tanaka(Kyoto University), Takahiro Tanaka(UCLouvain), A. J. Tanasijczuk(Syracuse University), S. Tanioka(University of Florida), D. B. Tanner(California Institute of Technology), D. Tao(University of Florida), Tao Liu(Pennsylvania State University), Ron Tapia(National Institute for Subatomic Physics), E. N. Tapia San Martín(California Institute of Technology), R. Tarafder(University of Rome Tor Vergata), C. Taranto(Kyoto University), Atsushi Taruya(Carleton College), Jay D. Tasson(Université Libre de Bruxelles), M. Teloi(Universitat de les Illes Balears), R. Tenorio(Villanova University), J. E. S. Terhune(Universität Hamburg), L. Terkowski(California State University Los Angeles), H. Themann(Inter-University Centre for Astronomy and Astrophysics), M. P. Thirugnanasambandam(University of Birmingham), L. M. Thomas(LIGO Scientific Collaboration), M. Thomas, P. Thomas(Syracuse University), S. Thomas(Cardiff University), Jonathan E. Thompson(Raja Ramanna Centre for Advanced Technology), S. R. Thondapu(LIGO Scientific Collaboration), K. A. Thorne(ARC Centre of Excellence for Gravitational Wave Discovery), E. Thrane(University of Zurich), Shubhanshu Tiwari(Inter-University Centre for Astronomy and Astrophysics), Srishti Tiwari(Cardiff University), V. Tiwari(University of Minnesota), A. M. Toivonen(University of Portsmouth), A. E. Tolley(National Astronomical Observatory of Japan), T. Tomaru(Osaka Metropolitan University), K. Tomita(The University of Tokyo), T. Tomura(University of Pisa), M. Tonelli(Universitat de València), A. Torres-Forné(California Institute of Technology), C. I. Torrie(Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud), I. Tosta e Melo(Centre National de la Recherche Scientifique), E. Tournefier(Università di Camerino), A. Trapananti(Università di Camerino), F. Travasso(LIGO Scientific Collaboration), G. Traylor(Universitat de Barcelona), J. Trenado(University of Maryland, College Park), M. Trevor(European Gravitational Observatory), M. C. Tringali(University of Michigan), A. Tripathee(University of Salerno), Luigi Troiano(University of Trieste), A. Trovato(Istituto Nazionale di Fisica Nucleare, Sezione di Napoli), L. Trozzo(California Institute of Technology), R. J. Trudeau(University of Groningen), K. W. Tsang(Chinese University of Hong Kong), T. Tsang(Massachusetts Institute of Technology), M. Tse(California Institute of Technology), R. Tso(Fukui National College of Technology), S. Tsuchida(Pennsylvania State University), L. Tsukada(The University of Tokyo), T. Tsutsui(Vrije Universiteit Brussel), K. Turbang(Centre National de la Recherche Scientifique), M. Turconi(Ghent University), C. Turski(The University of Tokyo), D. Tuyenbayev(Universitat de Barcelona), H. Ubach(University of Birmingham), A. S. Ubhi(The University of Tokyo), N. Uchikata(The University of Tokyo), Takashi Uchiyama(California Institute of Technology), R. P. Udall(University of Florida), T. Uehara(The University of Tokyo), K. Ueno(Tata Institute of Fundamental Research), B. Krishnan(The University of Tokyo), T. Ushiba(Maastricht University), A. Utina(Leibniz University Hannover), H. Vahlbruch(California Institute of Technology), Nina Vaidya(California Institute of Technology), G. Vajente(ARC Centre of Excellence for Gravitational Wave Discovery), A. Vajpeyi(Texas A&M University), G. Valdés(University of Trento), M. Valentini(Istituto Nazionale di Fisica Nucleare, Sezione di Torino), S. Vallero(University of Wisconsin–Milwaukee), V. Valsan(National Institute for Subatomic Physics), N. van Bakel(Maastricht University), M. van Beuzekom(Utrecht University), M. van Dael(Syracuse University), J. F. J. van den Brand(Utrecht University), C. Van Den Broeck(Centre National de la Recherche Scientifique), D. C. Vander‐Hyde(National Institute for Subatomic Physics), Marc van der Sluys(University of Antwerp), Axel van de Walle(UCLouvain), J. van Dongen(California Institute of Technology), Hans Van Haevermaet(Sejong University), J. V. van Heijningen(Maastricht University), J. Vanosky(University of Antwerp), Maurice H. P. M. van Putten(National Institute for Subatomic Physics), Z. van Ranst(The University of Melbourne), N. Van Remortel(Max Planck Institute for Gravitational Physics), M. Vardaro(HUN-REN Wigner Research Centre for Physics), A. F. Vargas(University of Birmingham), Vijay Varma(Istituto Nazionale di Fisica Nucleare, Sezione di Padova), M. Vasúth(University of Glasgow), A. Vecchio(ARC Centre of Excellence for Gravitational Wave Discovery), G. Vedovato(Leibniz University Hannover), J. Veitch(California Institute of Technology), P. J. Veitch(Université Claude Bernard Lyon 1), J. Venneberg(Centre National de la Recherche Scientifique), G. Venugopalan(National Centre for Nuclear Research), P. Verdier(Raja Ramanna Centre for Advanced Technology), D. Verkindt(Cardiff University), P. Verma(Columbia University), Y. Verma(University of Urbino), S. M. Vermeulen(University of Urbino), Doğa Veske(Syracuse University), F. Vetrano(Concordia University Wisconsin), A. Viceré(Tata Institute of Fundamental Research), S. Vidyant(Universidade de Santiago de Compostela), A. D. Viets(Cardiff University), A. Vijaykumar(Georgia Institute of Technology), V. Villa-Ortega(Centre National de la Recherche Scientifique), M. Viña(Université Claude Bernard Lyon 1), E. T. Vincent(University of Trieste), J.-Y. Vinet(Massachusetts Institute of Technology), S. Viret(University of Perugia), A. Virtuoso(Universität Hamburg), S. Vitale, H. Vocca(Leibniz University Hannover), D Voigt, E. R. G. von Reis(Lomonosov Moscow State University), J. S. A. von Wrangel(Kenyon College), C. Vorvick(Kenyon College), S. P. Vyatchanin(Rochester Institute of Technology), L. E. Wade(National Institute for Subatomic Physics), M. Wade(Christopher Newport University), K. J. Wagner(University of Strathclyde), R. Walet(California Institute of Technology), M. Walker(The University of Tokyo), G. S. Wallace(University of Michigan), L. Wallace(The University of Texas Rio Grande Valley), H. Wang(Australian National University), J. Z. Wang, W. H. Wang(Centre National de la Recherche Scientifique), R. L. Ward(National Astronomical Observatory of Japan), J. Warner(California Institute of Technology), M. Wąs(Christopher Newport University), T. Washimi(The University of Tokyo), N. Y. Washington(Université Libre de Bruxelles), K. Watada(Kenyon College), D. Watarai, J. Watchi(University of Portsmouth), K. E. Wayt(University of Glasgow), B. Weaver(Leibniz University Hannover), C. R. Weaving(California Institute of Technology), S. A. Webster(Massachusetts Institute of Technology), M. Weinert(University of Washington), A. J. Weinstein(Vanderbilt University), R. Weiss(Leibniz University Hannover), C. M. Weller(The University of Western Australia), Robert A. Weller(Leibniz University Hannover), F. Wellmann(Australian National University), L. Wen(Rochester Institute of Technology), P. Weßels(California State University, Fullerton), K. Wette(University of Florida), J. T. Whelan(Massachusetts Institute of Technology), Dave D. White(Kenyon College), B. F. Whiting(Leibniz University Hannover), C. Whittle(Cardiff University), O. S. Wilk(University of Glasgow), Dennis Wilken(University of Glasgow), K. Willetts(University of Portsmouth), D. R. Williams(California Institute of Technology), M. J. Williams(Leibniz University Hannover), A. R. Williamson(California Institute of Technology), J. L. Willis(University of Glasgow), B. Willke(Leibniz University Hannover), C. C. Wipf(Rochester Institute of Technology), G. Woan(University of British Columbia), J. Woehler(National Central University), J. K. Wofford(Chinese University of Hong Kong), D. Wong(University of Glasgow), H. T. Wong(Max Planck Institute for Gravitational Physics), I. C. F. Wong(Leibniz University Hannover), M. Wright(Max Planck Institute for Gravitational Physics), Chien-Ming Wu(University of Wisconsin–Milwaukee), D. S. Wu(California Institute of Technology), H. Wu(Massachusetts Institute of Technology), D. M. Wysocki(Nicolaus Copernicus Astronomical Center), S. Xiao(High Energy Accelerator Research Organization), Victoria Xu(California Institute of Technology), N. Yadav(University of Toyama), T. Yamada(University of Toyama), H. Yamamoto(The University of Tokyo), K. Yamamoto(Nagoya University), M. Yamamoto(University of Toyama), T. Yamamoto(Aoyama Gakuin University), Takahiro Yamamoto(University of Utah), K. Yamashita(University of Minnesota), Ryo Yamazaki(National Tsing Hua University), F. W. Yang(Australian National University), K. Z. Yang(Cardiff University), Yi Yang(Rochester Institute of Technology), M. J. Yap(Andrews University), D. W. Yeeles(The University of Tokyo), A. B. Yelikar(The University of Tokyo), T. Y. Yeung(Cornell University), Jun’ichi Yokoyama(California Institute of Technology), T. Yokozawa(Massachusetts Institute of Technology), J. Yoo(The University of Tokyo), Hang Yu(National Centre for Nuclear Research), Haocun Yu(Christopher Newport University), H. Yuzurihara(Embry–Riddle Aeronautical University), A. Zadrożny(Rochester Institute of Technology), A. J. Zannelli(Rikkyo University), M. Zanolin(European Gravitational Observatory), M. Zeeshan(Istituto Nazionale di Fisica Nucleare, Sezione di Padova), S. Zeidler(University of Chicago), T. Zelenova(Australian National University), J.‐P. Zendri(California Institute of Technology), M. Zevin(University of Florida), J. Zhang(University of Birmingham), L. Zhang(Texas A&M University), R. Zhang(The University of Western Australia), T. Zhang(University of Utah), Y. Zhang(National Astronomical Observatory of Japan), C. Zhao(Missouri University of Science and Technology), Yue Zhao(University of Minnesota), Yang Zhao(University of California, Berkeley), Y. Zheng(ARC Centre of Excellence for Gravitational Wave Discovery), H. Zhong(Beijing Normal University), Rongpu Zhou(The University of Texas at Austin), X. J. Zhu(California Institute of Technology), Zong‐Hong Zhu(California Institute of Technology), Aaron Zimmerman, M. E. Zucker, J. Zweizig
Cited by 305Open Access
Abstract
Abstract The global network of gravitational-wave observatories now includes five detectors, namely LIGO Hanford, LIGO Livingston, Virgo, KAGRA, and GEO 600. These detectors collected data during their third observing run, O3, composed of three phases: O3a starting in 2019 April and lasting six months, O3b starting in 2019 November and lasting five months, and O3GK starting in 2020 April and lasting two weeks. In this paper we describe these data and various other science products that can be freely accessed through the Gravitational Wave Open Science Center at https://gwosc.org . The main data set, consisting of the gravitational-wave strain time series that contains the astrophysical signals, is released together with supporting data useful for their analysis and documentation, tutorials, as well as analysis software packages.
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