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Bicocca Open Archive
We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC-2020 March 27 17:00 UTC). We conduct two independent searches: A generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate.
Abbott, R., Abbott, T., Acernese, F., Ackley, K., Adams, C., Adhikari, N., et al. (2022). Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b. THE ASTROPHYSICAL JOURNAL, 928(2) [10.3847/1538-4357/ac532b].
Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b
R. Abbott;T. D. Abbott;F. Acernese;K. Ackley;C. Adams;N. Adhikari;R. X. Adhikari;V. B. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. D. Aguiar;L. Aiello;A. Ain;P. Ajith;T. Akutsu;S. Albanesi;A. Allocca;P. A. Altin;A. Amato;C. Anand;S. Anand;A. Ananyeva;S. B. Anderson;W. G. Anderson;M. Ando;T. Andrade;N. Andres;T. Andri??;S. V. Angelova;S. Ansoldi;J. M. Antelis;S. Antier;S. Appert;Koji Arai;Koya Arai;Y. Arai;S. Araki;A. Araya;M. C. Araya;J. S. Areeda;M. Ar??ne;N. Aritomi;N. Arnaud;S. M. Aronson;K. G. Arun;H. Asada;Y. Asali;G. Ashton;Y. Aso;M. Assiduo;S. M. Aston;P. Astone;F. Aubin;C. Austin;S. Babak;F. Badaracco;M. K. M. Bader;C. Badger;S. Bae;Y. Bae;A. M. Baer;S. Bagnasco;Y. Bai;L. Baiotti;J. Baird;R. Bajpai;M. Ball;G. Ballardin;S. W. Ballmer;A. Balsamo;G. Baltus;S. Banagiri;D. Bankar;J. C. Barayoga;C. Barbieri;B. C. Barish;D. Barker;P. Barneo;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;M. A. Barton;I. Bartos;R. Bassiri;A. Basti;M. Bawaj;J. C. Bayley;A. C. Baylor;M. Bazzan;B. B??csy;V. M. Bedakihale;M. Bejger;I. Belahcene;V. Benedetto;D. Beniwal;T. F. Bennett;J. D. Bentley;M. BenYaala;F. Bergamin;B. K. Berger;S. Bernuzzi;C. P. L. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;D. Beveridge;R. Bhandare;U. Bhardwaj;D. Bhattacharjee;S. Bhaumik;I. A. Bilenko;G. Billingsley;S. Bini;R. Birney;O. Birnholtz;S. Biscans;M. Bischi;S. Biscoveanu;A. Bisht;B. Biswas;M. Bitossi;M. -A. Bizouard;J. K. Blackburn;C. D. Blair;D. G. Blair;R. M. Blair;F. Bobba;N. Bode;M. Boer;G. Bogaert;M. Boldrini;L. D. Bonavena;F. Bondu;E. Bonilla;R. Bonnand;P. Booker;B. A. Boom;R. Bork;V. Boschi;N. Bose;S. Bose;V. Bossilkov;V. Boudart;Y. Bouffanais;A. Bozzi;C. Bradaschia;P. R. Brady;A. Bramley;A. Branch;M. Branchesi;J. E. Brau;M. Breschi;T. Briant;J. H. Briggs;A. Brillet;M. Brinkmann;P. Brockill;A. F. Brooks;J. Brooks;D. D. Brown;S. Brunett;G. Bruno;R. Bruntz;J. Bryant;T. Bulik;H. J. Bulten;A. Buonanno;R. Buscicchio;D. Buskulic;C. Buy;R. L. Byer;L. Cadonati;G. Cagnoli;C. Cahillane;J. Calder??n Bustillo;J. D. Callaghan;T. A. Callister;E. Calloni;J. Cameron;J. B. Camp;M. Canepa;S. Canevarolo;M. Cannavacciuolo;K. C. Cannon;H. Cao;Z. Cao;E. Capocasa;E. Capote;G. Carapella;F. Carbognani;J. B. Carlin;M. F. Carney;M. Carpinelli;G. Carrillo;G. Carullo;T. L. Carver;J. Casanueva Diaz;C. Casentini;G. Castaldi;S. Caudill;M. Cavagli??;F. Cavalier;R. Cavalieri;M. Ceasar;G. Cella;P. Cerd??-Dur??n;E. Cesarini;W. Chaibi;K. Chakravarti;S. Chalathadka Subrahmanya;E. Champion;C. -H. Chan;C. Chan;C. L. Chan;K. Chan;M. Chan;K. Chandra;P. Chanial;S. Chao;P. Charlton;E. A. Chase;E. Chassande-Mottin;C. Chatterjee;Debarati Chatterjee;Deep Chatterjee;M. Chaturvedi;S. Chaty;K. Chatziioannou;C. Chen;H. Y. Chen;J. Chen;K. Chen;X. Chen;Y. -B. Chen;Y. -R. Chen;Z. Chen;H. Cheng;C. K. Cheong;H. Y. Cheung;H. Y. Chia;F. Chiadini;C-Y. Chiang;G. Chiarini;R. Chierici;A. Chincarini;M. L. Chiofalo;A. Chiummo;G. Cho;H. S. Cho;R. K. Choudhary;S. Choudhary;N. Christensen;H. Chu;Q. 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Davis;M. C. Davis;E. J. Daw;R. Dean;D. DeBra;M. Deenadayalan;J. Degallaix;M. De Laurentis;S. Del??glise;V. Del Favero;F. De Lillo;N. De Lillo;W. Del Pozzo;L. M. DeMarchi;F. De Matteis;V. D???Emilio;N. Demos;T. Dent;A. Depasse;R. De Pietri;R. De Rosa;C. De Rossi;R. DeSalvo;R. De Simone;S. Dhurandhar;M. C. D??az;M. Diaz-Ortiz;N. A. Didio;T. Dietrich;L. Di Fiore;C. Di Fronzo;C. Di Giorgio;F. Di Giovanni;M. Di Giovanni;T. Di Girolamo;A. Di Lieto;B. Ding;S. Di Pace;I. Di Palma;F. Di Renzo;A. K. Divakarla;A. Dmitriev;Z. Doctor;L. D???Onofrio;F. Donovan;K. L. Dooley;S. Doravari;I. Dorrington;M. Drago;J. C. Driggers;Y. Drori;J. -G. Ducoin;P. Dupej;O. Durante;D. D???Urso;P. -A. Duverne;S. E. Dwyer;C. Eassa;P. J. Easter;M. Ebersold;T. Eckhardt;G. Eddolls;B. Edelman;T. B. Edo;O. Edy;A. Effler;S. Eguchi;J. Eichholz;S. S. Eikenberry;M. Eisenmann;R. A. Eisenstein;A. Ejlli;E. Engelby;Y. Enomoto;L. Errico;R. C. Essick;H. Estell??s;D. Estevez;Z. Etienne;T. Etzel;M. Evans;T. M. Evans;B. E. Ewing;V. Fafone;H. Fair;S. Fairhurst;A. M. Farah;S. Farinon;B. Farr;W. M. Farr;N. W. Farrow;E. J. Fauchon-Jones;G. Favaro;M. Favata;M. Fays;M. Fazio;J. Feicht;M. M. Fejer;E. Fenyvesi;D. L. Ferguson;A. Fernandez-Galiana;I. Ferrante;T. A. Ferreira;F. Fidecaro;P. Figura;I. Fiori;M. Fishbach;R. P. Fisher;R. Fittipaldi;V. Fiumara;R. Flaminio;E. Floden;H. Fong;J. A. Font;B. Fornal;P. W. F. Forsyth;A. Franke;S. Frasca;F. Frasconi;C. Frederick;J. P. Freed;Z. Frei;A. Freise;R. Frey;P. Fritschel;V. V. Frolov;G. G. Fronz??;Y. Fujii;Y. Fujikawa;M. Fukunaga;M. Fukushima;P. Fulda;M. Fyffe;H. A. Gabbard;B. U. Gadre;J. R. Gair;J. Gais;S. Galaudage;R. Gamba;D. Ganapathy;A. Ganguly;D. Gao;S. G. Gaonkar;B. Garaventa;C. Garc??a-N????ez;C. Garc??a-Quir??s;F. Garufi;B. Gateley;S. Gaudio;V. Gayathri;G. -G. Ge;G. Gemme;A. Gennai;J. George;O. Gerberding;L. Gergely;P. Gewecke;S. Ghonge;Abhirup Ghosh;Archisman Ghosh;Shaon Ghosh;Shrobana Ghosh;B. Giacomazzo;L. Giacoppo;J. A. Giaime;K. D. Giardina;D. R. Gibson;C. Gier;M. Giesler;P. Giri;F. Gissi;J. Glanzer;A. E. Gleckl;P. Godwin;E. Goetz;R. Goetz;N. Gohlke;B. Goncharov;G. Gonz??lez;A. Gopakumar;M. Gosselin;R. Gouaty;D. W. Gould;B. Grace;A. Grado;M. Granata;V. Granata;A. Grant;S. Gras;P. Grassia;C. Gray;R. Gray;G. Greco;A. C. Green;R. Green;A. M. Gretarsson;E. M. Gretarsson;D. Griffith;W. Griffiths;H. L. Griggs;G. Grignani;A. Grimaldi;S. J. Grimm;H. Grote;S. Grunewald;P. Gruning;D. Guerra;G. M. Guidi;A. R. Guimaraes;G. Guix??;H. K. Gulati;H. -K. Guo;Y. Guo;Anchal Gupta;Anuradha Gupta;P. Gupta;E. K. Gustafson;R. Gustafson;F. Guzman;S. Ha;L. Haegel;A. Hagiwara;S. Haino;O. Halim;E. D. Hall;E. Z. Hamilton;G. Hammond;W. -B. Han;M. Haney;J. Hanks;C. Hanna;M. D. Hannam;O. Hannuksela;H. Hansen;T. J. Hansen;J. Hanson;T. Harder;T. Hardwick;K. Haris;J. Harms;G. M. Harry;I. W. Harry;D. Hartwig;K. Hasegawa;B. Haskell;R. K. Hasskew;C. -J. Haster;K. Hattori;K. Haughian;H. Hayakawa;K. Hayama;F. J. Hayes;J. Healy;A. Heidmann;A. Heidt;M. C. Heintze;J. Heinze;J. Heinzel;H. Heitmann;F. Hellman;P. Hello;A. F. Helmling-Cornell;G. Hemming;M. Hendry;I. S. Heng;E. Hennes;J. Hennig;M. H. Hennig;A. G. Hernandez;F. Hernandez Vivanco;M. Heurs;S. Higginbotham;S. Hild;P. Hill;Y. Himemoto;A. S. Hines;Y. Hiranuma;N. Hirata;E. Hirose;S. Hochheim;D. Hofman;J. N. Hohmann;D. G. Holcomb;N. A. Holland;I. J. Hollows;Z. J. Holmes;K. Holt;D. E. Holz;Z. Hong;P. Hopkins;J. Hough;S. Hourihane;E. J. Howell;C. G. Hoy;D. Hoyland;A. Hreibi;B-H. Hsieh;Y. Hsu;G-Z. Huang;H-Y. Huang;P. Huang;Y-C. Huang;Y. -J. Huang;Y. Huang;M. T. H??bner;A. D. Huddart;B. Hughey;D. C. Y. Hui;V. Hui;S. Husa;S. H. Huttner;R. Huxford;T. Huynh-Dinh;S. Ide;B. Idzkowski;A. Iess;B. Ikenoue;S. Imam;K. Inayoshi;C. Ingram;Y. Inoue;K. Ioka;M. Isi;K. Isleif;K. Ito;Y. Itoh;B. R. Iyer;K. Izumi;V. JaberianHamedan;T. Jacqmin;S. J. Jadhav;S. P. Jadhav;A. L. James;A. Z. Jan;K. Jani;J. Janquart;K. Janssens;N. N. Janthalur;P. Jaranowski;D. Jariwala;R. Jaume;A. C. Jenkins;K. Jenner;C. Jeon;M. Jeunon;W. Jia;H. -B. 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Ramos-Buades;J. Rana;P. Rapagnani;U. D. Rapol;A. Ray;V. Raymond;N. Raza;M. Razzano;J. Read;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. W. Reid;D. H. Reitze;P. Relton;A. Renzini;P. Rettegno;M. Rezac;F. Ricci;D. Richards;J. W. Richardson;L. Richardson;G. Riemenschneider;K. Riles;S. Rinaldi;K. Rink;M. Rizzo;N. A. Robertson;R. Robie;F. Robinet;A. Rocchi;S. Rodriguez;L. Rolland;J. G. Rollins;M. Romanelli;R. Romano;C. L. Romel;A. Romero-Rodr??guez;I. M. Romero-Shaw;J. H. Romie;S. Ronchini;L. Rosa;C. A. Rose;D. Rosi??ska;M. P. Ross;S. Rowan;S. J. Rowlinson;S. Roy;Santosh Roy;Soumen Roy;D. Rozza;P. Ruggi;K. Ryan;S. Sachdev;T. Sadecki;J. Sadiq;N. Sago;S. Saito;Y. Saito;K. Sakai;Y. Sakai;M. Sakellariadou;Y. Sakuno;O. S. Salafia;L. Salconi;M. Saleem;F. Salemi;A. Samajdar;E. J. Sanchez;J. H. Sanchez;L. E. Sanchez;N. Sanchis-Gual;J. R. Sanders;A. Sanuy;T. R. Saravanan;N. Sarin;B. Sassolas;H. Satari;B. S. Sathyaprakash;S. Sato;T. Sato;O. Sauter;R. L. Savage;T. Sawada;D. Sawant;H. L. Sawant;S. Sayah;D. Schaetzl;M. Scheel;J. Scheuer;M. Schiworski;P. Schmidt;S. Schmidt;R. Schnabel;M. Schneewind;R. M. S. Schofield;A. Sch??nbeck;B. W. Schulte;B. F. Schutz;E. Schwartz;J. Scott;S. M. Scott;M. Seglar-Arroyo;T. Sekiguchi;Y. Sekiguchi;D. Sellers;A. S. Sengupta;D. Sentenac;E. G. Seo;V. Sequino;A. Sergeev;Y. Setyawati;T. Shaffer;M. S. Shahriar;B. Shams;L. Shao;A. Sharma;P. Sharma;S. Sharma-Chaudhary;P. Shawhan;N. S. Shcheblanov;S. Shibagaki;M. Shikauchi;R. Shimizu;T. Shimoda;K. Shimode;H. Shinkai;T. Shishido;A. Shoda;D. H. Shoemaker;D. M. Shoemaker;S. ShyamSundar;M. Sieniawska;D. Sigg;L. P. Singer;D. Singh;N. Singh;A. Singha;A. M. Sintes;V. Sipala;V. Skliris;B. J. J. Slagmolen;T. J. Slaven-Blair;J. Smetana;J. R. Smith;R. J. E. Smith;J. Soldateschi;S. N. Somala;K. Somiya;E. J. Son;K. Soni;S. Soni;V. Sordini;F. Sorrentino;N. Sorrentino;H. Sotani;R. Soulard;T. Souradeep;E. Sowell;V. Spagnuolo;A. P. Spencer;M. Spera;R. Srinivasan;A. K. Srivastava;V. Srivastava;K. Staats;C. Stachie;D. A. Steer;J. Steinlechner;S. Steinlechner;D. J. Stops;M. Stover;K. A. Strain;L. C. Strang;G. Stratta;A. Strunk;R. Sturani;A. L. Stuver;S. Sudhagar;V. Sudhir;R. Sugimoto;H. G. Suh;T. Z. Summerscales;H. Sun;L. Sun;S. Sunil;A. Sur;J. Suresh;P. J. Sutton;Takamasa Suzuki;Toshikazu Suzuki;B. L. Swinkels;M. J. Szczepa??czyk;P. Szewczyk;M. Tacca;H. Tagoshi;S. C. Tait;H. Takahashi;R. Takahashi;A. Takamori;S. Takano;H. Takeda;M. Takeda;C. J. Talbot;C. Talbot;H. Tanaka;Kazuyuki Tanaka;Kenta Tanaka;Taiki Tanaka;Takahiro Tanaka;A. J. Tanasijczuk;S. Tanioka;D. B. Tanner;D. Tao;L. Tao;E. N. Tapia San Martin;E. N. Tapia San Mart??n;C. Taranto;J. D. Tasson;S. Telada;R. Tenorio;J. E. Terhune;L. Terkowski;M. P. Thirugnanasambandam;M. Thomas;P. Thomas;E. E. Thompson;J. E. Thompson;S. R. Thondapu;K. A. Thorne;E. Thrane;Shubhanshu Tiwari;Srishti Tiwari;V. Tiwari;A. M. Toivonen;K. Toland;A. E. Tolley;T. Tomaru;Y. Tomigami;T. Tomura;M. Tonelli;A. Torres-Forn??;C. I. Torrie;I. Tosta e Melo;D. T??yr??;A. Trapananti;F. Travasso;G. Traylor;M. Trevor;M. C. Tringali;A. Tripathee;L. Troiano;A. Trovato;L. Trozzo;R. J. Trudeau;D. S. Tsai;D. Tsai;K. W. Tsang;T. Tsang;J-S. Tsao;M. Tse;R. Tso;K. Tsubono;S. Tsuchida;L. Tsukada;D. Tsuna;T. Tsutsui;T. Tsuzuki;K. Turbang;M. Turconi;D. Tuyenbayev;A. S. Ubhi;N. Uchikata;T. Uchiyama;R. P. Udall;A. Ueda;T. Uehara;K. Ueno;G. Ueshima;C. S. Unnikrishnan;F. Uraguchi;A. L. Urban;T. Ushiba;A. Utina;H. Vahlbruch;G. Vajente;A. Vajpeyi;G. Valdes;M. Valentini;V. Valsan;N. van Bakel;M. van Beuzekom;J. F. J. van den Brand;C. Van Den Broeck;D. C. Vander-Hyde;L. van der Schaaf;J. V. van Heijningen;J. Vanosky;M. H. P. M. van Putten;N. van Remortel;M. Vardaro;A. F. Vargas;V. Varma;M. Vas??th;A. Vecchio;G. Vedovato;J. Veitch;P. J. Veitch;J. Venneberg;G. Venugopalan;D. Verkindt;P. Verma;Y. Verma;D. Veske;F. Vetrano;A. Vicer??;S. Vidyant;A. D. Viets;A. Vijaykumar;V. Villa-Ortega;J. -Y. Vinet;A. Virtuoso;S. Vitale;T. Vo;H. Vocca;E. R. G. von Reis;J. S. A. von Wrangel;C. Vorvick;S. P. Vyatchanin;L. E. Wade;M. Wade;K. J. Wagner;R. C. Walet;M. Walker;G. S. Wallace;L. Wallace;S. Walsh;J. Wang;J. Z. Wang;W. H. Wang;R. L. Ward;J. Warner;M. Was;T. Washimi;N. Y. Washington;J. Watchi;B. Weaver;S. A. Webster;M. Weinert;A. J. Weinstein;R. Weiss;C. M. Weller;F. Wellmann;L. Wen;P. We??els;K. Wette;J. T. Whelan;D. D. White;B. F. Whiting;C. Whittle;D. Wilken;D. Williams;M. J. Williams;A. R. Williamson;J. L. Willis;B. Willke;D. J. Wilson;W. Winkler;C. C. Wipf;T. Wlodarczyk;G. Woan;J. Woehler;J. K. Wofford;I. C. F. Wong;C. Wu;D. S. Wu;H. Wu;S. Wu;D. M. Wysocki;L. Xiao;W-R. Xu;T. Yamada;H. Yamamoto;Kazuhiro Yamamoto;Kohei Yamamoto;T. Yamamoto;K. Yamashita;R. Yamazaki;F. W. Yang;L. Yang;Y. Yang;Yang Yang;Z. Yang;M. J. Yap;D. W. Yeeles;A. B. Yelikar;M. Ying;K. Yokogawa;J. Yokoyama;T. Yokozawa;J. Yoo;T. Yoshioka;Hang Yu;Haocun Yu;H. Yuzurihara;A. Zadro??ny;M. Zanolin;S. Zeidler;T. Zelenova;J. -P. Zendri;M. Zevin;M. Zhan;H. Zhang;J. Zhang;L. Zhang;T. Zhang;Y. Zhang;C. Zhao;G. Zhao;Y. Zhao;Yue Zhao;Y. Zheng;R. Zhou;Z. Zhou;X. J. Zhu;Z. -H. Zhu;A. B. Zimmerman;M. E. Zucker;J. Zweizig
2022
Abstract
We search for gravitational-wave signals associated with gamma-ray bursts (GRBs) detected by the Fermi and Swift satellites during the second half of the third observing run of Advanced LIGO and Advanced Virgo (2019 November 1 15:00 UTC-2020 March 27 17:00 UTC). We conduct two independent searches: A generic gravitational-wave transients search to analyze 86 GRBs and an analysis to target binary mergers with at least one neutron star as short GRB progenitors for 17 events. We find no significant evidence for gravitational-wave signals associated with any of these GRBs. A weighted binomial test of the combined results finds no evidence for subthreshold gravitational-wave signals associated with this GRB ensemble either. We use several source types and signal morphologies during the searches, resulting in lower bounds on the estimated distance to each GRB. Finally, we constrain the population of low-luminosity short GRBs using results from the first to the third observing runs of Advanced LIGO and Advanced Virgo. The resulting population is in accordance with the local binary neutron star merger rate.
Abbott, R., Abbott, T., Acernese, F., Ackley, K., Adams, C., Adhikari, N., et al. (2022). Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO-Virgo Run O3b. THE ASTROPHYSICAL JOURNAL, 928(2) [10.3847/1538-4357/ac532b].
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/10281/392548
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simulazione ASN
Il report seguente simula gli indicatori relativi alla propria produzione scientifica in relazione alle soglie ASN 2023-2025 del proprio SC/SSD. Si ricorda che il superamento dei valori soglia (almeno 2 su 3) è requisito necessario ma non sufficiente al conseguimento dell'abilitazione. La simulazione si basa sui dati IRIS e sugli indicatori bibliometrici alla data indicata e non tiene conto di eventuali periodi di congedo obbligatorio, che in sede di domanda ASN danno diritto a incrementi percentuali dei valori. La simulazione può differire dall'esito di un’eventuale domanda ASN sia per errori di catalogazione e/o dati mancanti in IRIS, sia per la variabilità dei dati bibliometrici nel tempo. Si consideri che Anvur calcola i valori degli indicatori all'ultima data utile per la presentazione delle domande.
La presente simulazione è stata realizzata sulla base delle specifiche raccolte sul tavolo ER del Focus Group IRIS coordinato dall’Università di Modena e Reggio Emilia e delle regole riportate nel DM 598/2018 e allegata Tabella A. Cineca, l’Università di Modena e Reggio Emilia e il Focus Group IRIS non si assumono alcuna responsabilità in merito all’uso che il diretto interessato o terzi faranno della simulazione. Si specifica inoltre che la simulazione contiene calcoli effettuati con dati e algoritmi di pubblico dominio e deve quindi essere considerata come un mero ausilio al calcolo svolgibile manualmente o con strumenti equivalenti.