RUI: Searching for Gamma-Ray Burst and Fast Radio Burst Counterparts in LIGO Gravitational Wave Data

RUI：在 LIGO 引力波数据中搜索伽马射线爆发和快速无线电爆发对应物

• 批准号: 1912599
• 负责人: Ryan Fisher
• 金额: $ 15万
• 依托单位: Christopher Newport University
• 依托单位国家: 美国
• 项目类别: Continuing Grant
• 财政年份: 2019
• 资助国家: 美国
• 起止时间: 2019-06-15 至 2023-05-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1912599&HistoricalAwards=false
• 关键词: RUI; Searching; Gamma; Ray; Burst

Starting with the initial detection of gravitational waves (GW) from a binary black hole merger, and now continuing with the first detection of GWs from a binary neutron star merger associated with a gamma-ray burst (GRB), the era of true GW astronomy has begun. The detection of GWs from the binary neutron star merger, GW170817, when combined with the coincident GRB detection, GRB 170817A, and the electromagnetic follow-up campaign that discovered associated afterglows across the electromagnetic spectrum, has had a significant impact on the understanding of the progenitors of short GRBs, kilonovae, and the equation of state of neutron stars. This collection of observations and discoveries has demonstrated the capabilities of multi-messenger astronomy with the addition GWs. These successes of the first and second Observing Runs of The Advanced Laser Interferometer Gravitational-wave Observatory (LIGO) and the French-Italian Virgo detector are now being expanded upon, as these detectors began observing the universe at sensitivities never before achieved in their third Observing Run, starting in April of 2019. This award will support the search for GWs associated with new GRB events, for which only one coincident detection has so far been made. The award will also support the search for GWs associated with fast radio bursts (FRB), which are extremely short-lived and extremely energetic bursts radio waves first detected by radio telescopes in 2007. The progenitors of FRBs are completely unknown, and many astronomers are actively trying to detect more of these events to learn what might cause them. Any detection of a GW associated with a FRB would result in a significant increase in the understanding of the astrophysical origin of these mysterious events. The award will support the development of a diverse, globally competitive STEM workforce through the training of undergraduate and masters students to become competent scientific researchers able to conduct research at the internationally recognized level as the next generation of gravitational-wave astronomers.As was demonstrated with the multi-messenger observations of GW170817, combined detections of GWs with electromagnetic detections have significantly advanced the understanding of astrophysics of high-energy events. This award will support the search for GWs associated with GRBs using a coherent, matched-filter search for compact binary coalescence sources. These searches will be conducted in response to announced GRB detections, and any GWs detected will be announced to the astronomical community for prompt follow-up. This search extends the effective sensitivity of the GW detection network beyond that of an all-sky search by using the information provided by the external trigger's sky location. Additional detections of GWs associated with GRBs in the third and fourth observing runs of LIGO and complimentary Virgo data will enable the astrophysical properties of neutron stars to be better constrained. Additionally, the full electromagnetic emission model for these binary neutron star merger sources will be refined with future multi-messenger observations. This award will also support the coherent, template-based search for GWs associated with fast radio bursts (FRB). Currently, the models of FRB progenitors are poorly constrained, and very few candidate progenitor sources have been eliminated due to a combination of the paucity of bursts detected thus far and a lack of multispectral observations. If a GW were detected with a template-based search in LIGO and Virgo data and found to be associated with a FRB, this would immediately indicate that the source of FRBs are binary neutron star mergers or neutron star-black hole mergers. At the same time, if no coincident detections are made in this search, this will better constrain models of the FRB progenitors.This award reflects NSF's statutory mission and has been deemed worthy of support through evaluation using the Foundation's intellectual merit and broader impacts review criteria.

从最初检测到双黑洞合并中的引力波（GW）开始，到现在首次检测到与伽马射线暴（GRB）相关的双中子星合并中的引力波，真正的引力波天文学时代已经开始。双中子星合并 GW170817 中引力波的探测，与同时发生的伽玛射线暴探测（GRB 170817A）以及在整个电磁频谱中发现相关余辉的电磁后续活动相结合，对理解短伽玛暴的前身、千新星和中子星的状态方程产生了重大影响。这些观测和发现的集合证明了多信使天文学与额外引力波的能力。 先进激光干涉仪引力波天文台 (LIGO) 和法国-意大利室女座探测器的第一和第二次观测运行所取得的成功现在正在得到扩展，因为这些探测器开始以在 2019 年 4 月开始的第三次观测运行中从未达到的灵敏度观测宇宙。该奖项将支持寻找与新伽玛暴事件相关的引力波，迄今为止，只有一次同时探测到了这些引力波事件。 制成。 该奖项还将支持寻找与快速射电爆发 (FRB) 相关的引力波，这是一种寿命极短、能量极高的爆发无线电波，于 2007 年首次被射电望远镜探测到。FRB 的起源完全未知，许多天文学家正在积极尝试探测更多此类事件，以了解可能导致它们的原因。 任何与快速射电暴相关的引力波的探测都会显着增加人们对这些神秘事件的天体物理起源的理解。 该奖项将通过培训本科生和硕士生成为能够在国际公认水平上开展研究的下一代引力波天文学家，支持培养多元化、具有全球竞争力的 STEM 人才队伍。正如 GW170817 的多信使观测所证明的那样，引力波探测与电磁探测相结合极大地增进了对天体物理学的理解 的高能事件。 该奖项将支持使用相干、匹配滤波器搜索紧凑二元聚并源来搜索与伽玛暴相关的引力波。 这些搜索将根据已公布的伽玛射线暴检测进行，任何检测到的引力波都将向天文学界公布，以便及时跟进。通过使用外部触发器的天空位置提供的信息，该搜索将引力波检测网络的有效灵敏度扩展到全天空搜索之外。 在 LIGO 的第三次和第四次观测运行中额外检测到与伽玛暴相关的引力波以及补充的 Virgo 数据将使中子星的天体物理特性得到更好的限制。此外，这些双中子星合并源的完整电磁发射模型将通过未来的多信使观测进行完善。 该奖项还将支持对与快速无线电爆发（FRB）相关的引力波进行连贯的、基于模板的搜索。 目前，FRB 祖源的模型约束很差，并且由于迄今为止检测到的爆发的缺乏以及缺乏多光谱观测，很少有候选祖源被消除。如果在 LIGO 和 Virgo 数据中通过基于模板的搜索检测到引力波，并发现它与 FRB 相关，那么这将立即表明 FRB 的来源是双中子星合并或中子星-黑洞合并。同时，如果在这次搜索中没有进行一致的检测，这将更好地限制 FRB 祖先的模型。该奖项反映了 NSF 的法定使命，并通过使用基金会的智力价值和更广泛的影响审查标准进行评估，被认为值得支持。

项目成果

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift during the LIGO–Virgo Run O3a

搜索与费米和斯威夫特在 LIGO–Virgo Run O3a 期间检测到的伽马射线爆发相关的引力波

• DOI: 10.3847/1538-4357/abee15
• 发表时间: 2021
• 期刊: The Astrophysical Journal
• 作者: Abbott, R.;Abbott, T. D.;Abraham, S.;Acernese, F.;Ackley, K.;Adams, C.;Adhikari, R. X.;Adya, V. B.;Affeldt, C.;Agathos, M.
• 通讯作者: Agathos, M.

GWTC-2: Compact Binary Coalescences Observed by LIGO and Virgo during the First Half of the Third Observing Run

• DOI: 10.1103/physrevx.11.021053
• 发表时间: 2021-06-09
• 期刊: PHYSICAL REVIEW X
• 影响因子: 12.5
• 作者: Abbott, R.;Abbott, T. D.;Zweizig, J.
• 通讯作者: Zweizig, J.

Search for Gravitational Waves Associated with Gamma-Ray Bursts Detected by Fermi and Swift During the LIGO-Virgo Run O3b

• DOI: 10.3847/1538-4357/ac532b
• 发表时间: 2021-11
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;T. Abbott;F. Acernese;K. Ackley;C. Adams;N. Adhikari;R. Adhikari;V. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;T. Akutsu;S. Albanesi;A. Allocca;P. Altin;A. Amato;C. Anand;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;M. Ando;T. Andrade;N. Andrés;T. Andri'c;S. Angelova;S. Ansoldi;J. Antelis;S. Antier;S. Appert;K. Arai;K. Arai;Y. Arai;S. Araki;A. Araya;M. Araya;J. Areeda;M. Arène;N. Aritomi;N. Arnaud;S. Aronson;K. Arun;H. Asada;Y. Asali;G. Ashton;Y. Aso;M. Assiduo;S. Aston;P. Astone;F. Aubin;C. Austin;S. Babak;F. Badaracco;M. Bader;C. Badger;S. Bae;Y. Bae;A. Baer;S. Bagnasco;Y. Bai;L. Baiotti;J. Baird;R. Bajpai;M. Ball;G. Ballardin;S. Ballmer;A. Balsamo;G. Baltus;S. Banagiri;D. Bankar;J. Barayoga;C. Barbieri;B. Barish;D. Barker;P. Barneo;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;M. Barton;I. Bartos;R. Bassiri;A. Basti;M. Bawaj;J. Bayley;A. Baylor;M. Bazzan;B. B'ecsy;V. Bedakihale;M. Bejger;I. Belahcene;V. Benedetto;D. Beniwal;T. Bennett;J. Bentley;M. BenYaala;F. Bergamin;B. Berger;S. Bernuzzi;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;D. Beveridge;R. Bhandare;U. Bhardwaj;D. Bhattacharjee;S. Bhaumik;I. Bilenko;G. Billingsley;S. Bini;R. Birney;O. Birnholtz;S. Biscans;M. Bischi;S. Biscoveanu;A. Bisht;B. Biswas;M. Bitossi;M. Bizouard;J. Blackburn;C. Blair;D. Blair;R. 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. Brady;A. Bramley;A. Branch;M. Branchesi;J. Brau;M. Breschi;T. Briant;J. Briggs;A. Brillet;M. Brinkmann;P. Brockill;A. Brooks;J. Brooks;D. Brown;S. Brunett;G. Bruno;R. Bruntz;J. Bryant;T. Bulik;H. Bulten;A. Buonanno;R. Buscicchio;D. Buskulic;C. Buy;R. Byer;L. Cadonati;G. Cagnoli;C. Cahillane;J. C. Bustillo;J. Callaghan;T. Callister;E. Calloni;J. Cameron;J. Camp;M. Canepa;S. Canevarolo;M. Cannavacciuolo;K. Cannon;H. Cao;Z. Cao;E. Capocasa;E. Capote;G. Carapella;F. Carbognani;J. Carlin;M. Carney;M. Carpinelli;G. Carrillo;G. Carullo;T. Carver;J. C. Diaz;C. Casentini;G. Castaldi;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;M. Ceasar;G. Cella;P. Cerd'a-Dur'an;E. Cesarini;W. Chaibi;K. Chakravarti;S. Subrahmanya;E. Champion;C. Chan;C. Chan;C. Chan;K. Chan;M. Chan;K. Chandra;P. Chanial;S. Chao;P. Charlton;E. Chase;É. Chassande-Mottin;C. Chatterjee;D. Chatterjee;D. Chatterjee;M. Chaturvedi;S. Chaty;K. Chatziioannou;C. Chen;H. Chen;J. Chen;K. Chen;X. Chen;Y. Chen;Y.-R. Chen;Z. Chen;H. Cheng;C. Cheong;H. Cheung;H. Chia;F. Chiadini;C. Chiang;G. Chiarini;R. Chierici;A. Chincarini;M. Chiofalo;A. Chiummo;G. Cho;H. Cho;Rupesh Kumar Choudhary;S. Choudhary;N. Christensen;H. Chu;Q. Chu;Y. Chu;S. Chua;K. Chung;G. Ciani;P. Ciecieląg;M. Cie'slar;M. Cifaldi;A. Ciobanu;R. Ciolfi;F. Cipriano;A. Cirone;F. Clara;E. Clark;J. Clark;L. Clarke;P. Clearwater;S. Clesse;F. Cleva;E. Coccia;E. Codazzo;P. Cohadon;D. Cohen;L. Cohen;M. Colleoni;C. Collette;A. Colombo;M. Colpi;C. Compton;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;I. Cordero-Carri'on;S. Corezzi;K. Corley;N. Cornish;D. Corre;A. Corsi;S. Cortese;C. Costa;R. Cotesta;M. Coughlin;J. Coulon;S. Countryman;B. Cousins;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;J. Creighton;T. Creighton;A. Criswell;M. Croquette;S. Crowder;J. Cudell;T. Cullen;A. Cumming;R. Cummings;L. Cunningham;E. Cuoco;M. Curyło;P. Dabadie;T. D. Canton;S. Dall’Osso;G. D'alya;A. Dana;L. M. DaneshgaranBajastani;Beatrice D'Angelo;S. Danilishin;S. D’Antonio;K. Danzmann;C. Darsow-Fromm;A. Dasgupta;L. Datrier;S. Datta;V. Dattilo;I. Dave;M. Davier;G. Davies;D. Davis;M. Davis;E. Daw;R. Dean;D. DeBra;M. Deenadayalan;J. Degallaix;M. D. Laurentis;S. Del'eglise;V. D. Favero;F. D. Lillo;N. D. Lillo;W. D. Pozzo;L. DeMarchi;F. Matteis;V. D'Emilio;N. Demos;T. Dent;A. Depasse;R. Pietri;R. Rosa;C. D. 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Floden;H. Fong;J. Font;B. Fornal;P. Forsyth;A. Franke;S. Frasca;F. Frasconi;C. Frederick;J. Freed;Z. Frei;A. Freise;R. Frey;P. Fritschel;V. Frolov;G. G. Fronz'e-G.;Y. Fujii;Y. Fujikawa;M. Fukunaga;M. Fukushima;P. Fulda;M. Fyffe;H. Gabbard;B. Gadre;J. Gair;J. Gais;S. Galaudage;R. Gamba;D. Ganapathy;A. Ganguly;D. Gao;S. Gaonkar;B. Garaventa;C. Garc'ia-N'unez;C. Garc'ia-Quir'os;F. Garufi;B. Gateley;S. Gaudio;V. Gayathri;G. Ge;G. Gemme;A. Gennai;J. George;O. Gerberding;L. Gergely;P. Gewecke;S. Ghonge;A. Ghosh;A. Ghosh;Shaon Ghosh;Shrobana Ghosh;B. Giacomazzo;L. Giacoppo;J. Giaime;K. Giardina;D. Gibson;C. Gier;M. Giesler;P. Giri;F. Gissi;J. Glanzer;A. Gleckl;P. Godwin;E. Goetz;R. Goetz;N. Gohlke;B. Goncharov;G. Gonz'alez;A. Gopakumar;M. Gosselin;R. Gouaty;D. Gould;B. Grace;A. Grado;M. Granata;V. Granata;A. Grant;S. Gras;P. Grassia;C. Gray;R. Gray;G. Greco;A. Green;R. Green;A. Gretarsson;E. Gretarsson;D. Griffith;W. Griffiths;H. L. Griggs;G. Grignani;A. Grimaldi;S. Grimm;H. Grote;S. Grunewald;P. Gruning;D. Guerra;G. Guidi;A. R. Guimaraes;G. Guix'e;H. Gulati;H.-K. Guo;Y. Guo;Anchal Gupta;Anchal Gupta;P. Gupta;E. Gustafson;R. Gustafson;F. Guzmán;S. Ha;L. Haegel;A. Hagiwara;S. Haino;O. Halim;E. Hall;E. Hamilton;G. Hammond;W. Han;M. Haney;J. Hanks;C. Hanna;M. Hannam;O. Hannuksela;H. Hansen;T. Hansen;J. Hanson;T. Harder;T. Hardwick;K. Haris;J. Harms;G. Harry;I. Harry;D. Hartwig;K. Hasegawa;B. Haskell;R. Hasskew;C. Haster;K. Hattori;K. Haughian;H. Hayakawa;K. Hayama;F. Hayes;J. Healy;A. Heidmann;A. Heidt;M. Heintze;J. Heinze;J. Heinzel;H. Heitmann;F. Hellman;P. Hello;A. Helmling-Cornell;G. Hemming;M. Hendry;I. Heng;E. Hennes;J. Hennig;M. Hennig;A. Hernandez;F. Vivanco;M. Heurs;S. Hild;P. Hill;Y. Himemoto;A. Hines;Y. Hiranuma;N. Hirata;E. Hirose;S. Hochheim;D. Hofman;J. Hohmann;D. Holcomb;N. Holland;I. J. Hollows;Z. J. Holmes;K. Holt;D. Holz;Z. Hong;P. Hopkins;J. Hough;S. Hourihane;E. Howell;C. Hoy;D. Hoyland;A. Hreibi;B. Hsieh;Y. Hsu;G-Z. Huang;H. Huang;P. Huang;Y. Huang;Y. Huang;Y. Huang;M. Hubner;A. Huddart;B. Hughey;D. Hui;V. Hui;S. Husa;S. Huttner;R. Huxford;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;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. Iyer;K. Izumi;V. JaberianHamedan;T. Jacqmin;S. Jadhav;S. Jadhav;A. James;A. Jan;K. Jani;J. Janquart;K. Janssens;N. Janthalur;P. Jaranowski;D. Jariwala;R. Jaume;A. Jenkins;K. Jenner;C. Jeon;M. Jeunon;W. Jia;H. Jin;G. Johns;A. Jones;D. Jones;J. Jones;P. Jones;R. Jones;R. Jonker;L. Ju;P. Jung;K. Jung;J. Junker;V. Juste;K. Kaihotsu;T. Kajita;M. Kakizaki;C. Kalaghatgi;V. Kalogera;B. Kamai;M. Kamiizumi;N. Kanda;S. Kandhasamy;G. Kang;J. Kanner;Y. Kao;S. Kapadia;D. Kapasi;S. Karat;C. Karathanasis;S. Karki;R. Kashyap;M. Kasprzack;W. Kastaun;S. Katsanevas;E. Katsavounidis;W. Katzman;T. Kaur;K. Kawabe;K. Kawaguchi;N. Kawai;T. Kawasaki;F. K'ef'elian;D. Keitel;J. Key;S. Khadka;F. Khalili;S. Khan;E. Khazanov;N. Khetan;M. Khursheed;N. 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Lin;F. Linde;S. Linker;J. Linley;T. Littenberg;G. Liu;J. Liu;K. Liu;X. Liu;F. Llamas;M. Llorens-Monteagudo;R. K. Lo;A. Lockwood;L. London;A. Longo;D. Lopez;M. Portilla;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;T. Lott;J. Lough;C. Lousto;G. Lovelace;J. F. Lucaccioni;H. Luck;D. Lumaca;A. Lundgren;L. Luo;J. Lynam;R. Macas;M. Macinnis;D. Macleod;I. MacMillan;A. Macquet;I. M. Hernandez;C. Magazzù;R. Magee;R. Maggiore;M. Magnozzi;S. Mahesh;E. Majorana;C. Makarem;I. Maksimovic;S. Maliakal;A. Malik;N. Man;V. Mandic;V. Mangano;J. Mango;G. Mansell;M. Manske;M. Mantovani;M. Mapelli;F. Marchesoni;M. Marchiò;F. Marion;Z. Mark;S. M'arka;Z. M'arka;C. Markakis;A. Markosyan;A. Markowitz;E. Maros;A. Marquina;S. Marsat;F. Martelli;I. Martin;R. Martin;M. Martínez;V. Martínez;V. Martínez;K. Martinovic;D. Martynov;E. J. Marx;H. Masalehdan;K. Mason;E. Massera;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;M. Mateu-Lucena;F. Matichard;M. Matiushechkina;N. Mavalvala;J. McCann;R. 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Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Muusse;S. Nadji;K. Nagano;S. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;R. Nakashima;Y. Nakayama;V. Napolano;I. Nardecchia;T. Narikawa;L. Naticchioni;B. Nayak;R. Nayak;R. Negishi;B. Neil;J. Neilson;G. Nelemans;T. Nelson;M. Nery;P. Neubauer;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;W. Ni;S. Nichols;A. Nishizawa;S. Nissanke;E. Nitoglia;F. Nocera;M. Norman;C. North;S. Nozaki;L. Nuttall;J. Oberling;B. O'Brien;Y. Obuchi;J. O'Dell;E. Oelker;W. Ogaki;G. Oganesyan;J. Oh;K. Oh;S. -. Oh;M. Ohashi;N. Ohishi;M. Ohkawa;F. Ohme;H. Ohta;M. A. Okada;Y. Okutani;K. Okutomi;C. Olivetto;K. Oohara;C. Ooi;R. Oram;B. O'reilly;R. Ormiston;N. Ormsby;L. F. Ortega;R. O’Shaughnessy;É. O’Shea;S. Oshino;S. Ossokine;C. Osthelder;S. Otabe;D. Ottaway;H. Overmier;A. Pace;G. Pagano;M. Page;G. Pagliaroli;A. Pai;S. Pai;J. R. Palamos;O. Palashov;C. Palomba;H. Pan;K. Pan;P. K. Panda;H. Pang;P. T. Pang;C. Pankow;F. Pannarale;B. Pant;F. Panther;F. Paoletti;A. Paoli;A. Paolone;A. Parisi;H. Park;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;M. Pathak;B. Patricelli;A. S. Patron;S. Paul;E. Payne;M. Pedraza;M. Pegoraro;A. Pele;F. Arellano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. P'erigois;C. Perkins;A. Perreca;S. Perriès;J. Petermann;D. Petterson;H. Pfeiffer;K. A. Pham;K. S. Phukon;O. Piccinni;M. Pichot;M. Piendibene;F. Piergiovanni;L. Pierini;V. Pierro;G. Pillant;M. Pillas;F. Pilo;L. Pinard;I. Pinto;M. Pinto;K. Piotrzkowski;M. Pirello;M. Pitkin;E. Placidi;L. Planas;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;D. T. Pong;S. Ponrathnam;P. Popolizio;E. Porter;R. Poulton;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;M. Principe;G. Prodi;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;P. Puppo;M. Purrer;H. Qi;V. Quetschke;R. Quitzow-James;F. Raab;G. Raaijmakers;H. Radkins;N. Radulesco;P. Raffai;S. X. Rail;S. Raja;C. Rajan;K. Ramirez;T. Ramirez;A. Ramos-Buades;J. Rana;P. Rapagnani;U. Rapol;A. Ray;V. Raymond;N. Raza;M. Razzano;J. Read;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. Reid;D. Reitze;P. Relton;A. Renzini;P. Rettegno;M. Rezac;F. Ricci;D. Richards;J. Richardson;L. Richardson;G. Riemenschneider;K. Riles;S. Rinaldi;K. Rink;M. Rizzo;N. Robertson;R. Robie;F. Robinet;A. Rocchi;S. Rodriguez;L. Rolland;J. Rollins;M. Romanelli;R. Romano;C. Romel;A. Romero-Rodr'iguez;I. Romero-Shaw;J. Romie;S. Ronchini;L. Rosa;C. Rose;D. Rosi'nska;M. Ross;S. Rowan;S. Rowlinson;S. Roy;S. Roy;S. 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. Salafia;L. Salconi;M. Saleem;F. Salemi;A. Samajdar;E. Sanchez;Joaquín Sánchez;L. Sanchez;N. Sanchis-Gual;J. Sanders;A. Sanuy;T. R. Saravanan;N. Sarin;B. Sassolas;H. Satari;B. Sathyaprakash;S. Sato;T. Sato;O. Sauter;R. Savage;T. Sawada;D. Sawant;H. Sawant;S. Sayah;D. Schaetzl;M. Scheel;J. Scheuer;M. Schiworski;P. Schmidt;S. Schmidt;R. Schnabel;M. Schneewind;R. Schofield;A. Schonbeck;B. Schulte;B. Schutz;E. Schwartz;J. Scott;S. Scott;M. Seglar-Arroyo;T. Sekiguchi;Y. Sekiguchi;D. Sellers;A. Sengupta;D. Sentenac;E. Seo;V. Sequino;A. Sergeev;Y. Setyawati;T. Shaffer;M. Shahriar;B. Shams;L. Shao;A. Sharma;P. Sharma;S. Sharma-Chaudhary;P. Shawhan;N. Shcheblanov;S. Shibagaki;M. Shikauchi;R. Shimizu;T. Shimoda;K. Shimode;H. Shinkai;T. Shishido;A. Shoda;D. Shoemaker;D. Shoemaker;S. Shyamsundar;M. Sieniawska;D. Sigg;L. Singer;D. Singh;N. Singh;A. Singha;A. Sintes;V. Sipala;V. Skliris;B. Slagmolen;T. Slaven-Blair;J. Smetana;J. R. Smith;R. Smith;J. Soldateschi;S. Somala;K. Somiya;E. Son;K. Soni;S. Soni;V. Sordini;F. Sorrentino;N. Sorrentino;H. Sotani;R. Soulard;T. Souradeep;E. Sowell;V. Spagnuolo;A. Spencer;M. Spera;R. Srinivasan;A. Srivastava;V. Srivastava;K. Staats;C. Stachie;D. Steer;J. Steinlechner;S. Steinlechner;D. Stops;M. Stover;K. Strain;L. Strang;G. Stratta;A. Strunk;R. Sturani;A. Stuver;S. Sudhagar;V. Sudhir;R. Sugimoto;H. Suh;T. Summerscales;H. Sun;L. Sun;S. Sunil;A. Sur;J. Suresh;P. Sutton;Takamasa Suzuki;Toshikazu Suzuki;B. Swinkels;M. J. Szczepa'nczyk;P. Szewczyk;M. Tacca;H. Tagoshi;S. Tait;H. Takahashi;R. Takahashi;A. Takamori;S. Takano;H. Takeda;M. Takeda;C. Talbot;C. Talbot;H. Tanaka;Kazuyuki D. Tanaka;Kenta Tanaka;Taiki Tanaka;Takahiro Tanaka;A. Tanasijczuk;S. Tanioka;D. Tanner;D. Tao;L. Tao;E. Mart'in;C. Taranto;J. Tasson;S. Telada;R. Tenorio;J. Terhune;L. Terkowski;M. Thirugnanasambandam;M. Thomas;P. Thomas;E. E. Thompson-E.;J. E. Thompson;S. R. Thondapu;K. Thorne;E. Thrane;S. Tiwari;S. Tiwari;V. Tiwari;A. Toivonen;K. Toland;A. Tolley;T. Tomaru;Y. Tomigami;T. Tomura;M. Tonelli;A. Torres-Forn'e;C. Torrie;I. T. E. Melo;D. Toyra;A. Trapananti;F. Travasso;G. Traylor;M. Trevor;M. Tringali;A. Tripathee;L. Troiano;A. Trovato;L. Trozzo;R. Trudeau;D. Tsai;D. Tsai;K. W. Tsang;T. Tsang;J. Tsao;M. Tse;R. Tso;K. Tsubono;S. Tsuchida;L. Tsukada;D. Tsuna;T. Tsutsui;T. Tsuzuki;K. Turbang;M. Turconi;D. Tuyenbayev;A. Ubhi;N. Uchikata;T. Uchiyama;R. Udall;A. Ueda;T. Uehara;K. Ueno;G. Ueshima;C. Unnikrishnan;F. Uraguchi;A. Urban;T. Ushiba;A. Utina;H. Vahlbruch;G. Vajente;A. Vajpeyi;G. Valdes;M. Valentini;V. Valsan;N. Bakel;M. Beuzekom;J. Brand;C. Broeck;D. Vander-Hyde;L. V. D. Schaaf;J. V. Heijningen;J. Vanosky;M. Putten;N. Remortel;M. Vardaro;A. Vargas;V. Varma;M. Vas'uth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;J. Venneberg;G. Venugopalan;D. Verkindt;P. Verma;Y. Verma;D. Veske;F. Vetrano;A. Vicer'e;S. Vidyant;A. Viets;A. Vijaykumar;V. Villa-Ortega;J. Vinet;A. Virtuoso;S. Vitale;T. Vo;H. Vocca;E. V. Reis;J. Wrangel;C. Vorvick;S. Vyatchanin;L. Wade;M. Wade;K. Wagner;R. Walet;M. Walker;G. Wallace;L. Wallace;S. Walsh;J. Wang;J. Wang;W. H. Wang;R. Ward;J. Warner;M. Was;T. Washimi;N. Y. Washington;J. Watchi;B. Weaver;S. Webster;M. Weinert;A. Weinstein;R. Weiss;C. Weller;F. Wellmann;L. Wen;P. Wessels;K. Wette;J. Whelan;D. White;B. Whiting;C. Whittle;D. Wilken;D. Williams;M. Williams;A. Williamson;J. Willis;B. Willke;D. Wilson;W. Winkler;C. Wipf;T. Włodarczyk;G. Woan;J. Woehler;J. Wofford;I. C. Wong;C. Wu;D. Wu;H. Wu;S. Wu;D. Wysocki;L. Xiao;W-R. Xu;T. Yamada;H. Yamamoto;Kazuhiro Yamamoto;Kohei Yamamoto;T. Yamamoto;K. Yamashita;R. Yamazaki;F. Yang;L. Yang;Y. Yang;Yang Yang-Yang;Z. Yang;M. Yap;D. Yeeles;A. Yelikar;M. Ying;K. Yokogawa;J. Yokoyama;T. Yokozawa;J. Yoo;T. Yoshioka;Hang Yu;Haocun Yu;H. Yuzurihara;A. Zadro.zny;M. Zanolin;S. Zeidler;T. Zelenova;J. 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. Zhu;Z. Zhu;A. Zimmerman;M. Zucker;J. Zweizig

LIGO detector characterization in the second and third observing runs

• DOI: 10.1088/1361-6382/abfd85
• 发表时间: 2021-01
• 期刊: Classical and Quantum Gravity
• 影响因子: 3.5
• 作者: D. Davis;J. Areeda;B. Berger;R. Bruntz;A. Effler;R. Essick;R. Fisher;P. Godwin;E. Goetz;A. Helmling-Cornell;B. Hughey;E. Katsavounidis;A. Lundgren;D. Macleod;Z. Márka;T. Massinger;A. Matas;J. McIver;G. Mo;K. Mogushi;P. Nguyen;L. Nuttall;R. Schofield;D. Shoemaker;S. Soni;A. Stuver;A. Urban;G. Valdes;M. Walker;R. Abbott;C. Adams;R. Adhikari;A. Ananyeva;S. Appert;K. Arai;Y. Asali;S. Aston;C. Austin;A. Baer;M. Ball;S. Ballmer;S. Banagiri;D. Barker;C. Barschaw;L. Barsotti;J. Bartlett;J. Betzwieser;R. Beda;D. Bhattacharjee;J. Bidler;G. Billingsley;S. Biscans;C. Blair;R. Blair;N. Bode;P. Booker;R. Bork;A. Bramley;A. Brooks;D. Brown;A. Buikema;C. Cahillane;T. Callister;G. Caneva Santoro;K. Cannon;J. Carlin;K. Chandra;X. Chen;N. Christensen;A. Ciobanu;F. Clara;C. Compton;S. Cooper;K. Corley;M. Coughlin;S. Countryman;P. Covas;D. Coyne;S. Crowder;T. Dal Canton;B. Danila;L. Datrier;G. Davies;T. Dent;N. Didio;C. Di Fronzo;K. Dooley;J. Driggers;P. Dupej;S. Dwyer;T. Etzel;M. Evans;T. Evans;S. Fairhurst;J. Feicht;Á. Fernández-Galiana;R. Frey;P. Fritschel;V. Frolov;P. Fulda;M. Fyffe;B. Gadre;J. Giaime;K. Giardina;G. González;S. Gras;C. Gray;R. Gray;A. Green;A. Gupta;E. Gustafson;R. Gustafson;J. Hanks;J. Hanson;T. Hardwick;I. Harry;R. Hasskew;M. Heintze;J. Heinzel;N. Holland;I. J. Hollows;C. Hoy;S. Hughey;S. Jadhav;K. Janssens;G. Johns;J. Jones;S. Kandhasamy;S. Karki;M. Kasprzack;K. Kawabe;D. Keitel;N. Kijbunchoo;Y. M. Kim;P. King;J. Kissel;S. Kulkarni;Rahul Kumar;M. Landry;B. Lane;B. Lantz;M. Laxen;Y. Lecoeuche;J. Leviton;J. Liu;M. Lormand;R. Macas;A. Macedo;M. Macinnis;V. Mandic;G. Mansell;S. Márka;B. Martinez;K. Martinovic;D. Martynov;K. Mason;F. Matichard;N. Mavalvala;R McCarthy-;D. McClelland;S. Mccormick;L. McCuller;C. McIsaac;T. McRae;G. Mendell;K. Merfeld;E. Merilh;P. Meyers;F. Meylahn;I. Michaloliakos;H. Middleton;J. Mills;T. Mistry;R. Mittleman;G. Moreno;C. Mow-Lowry;S. Mozzon;L. Mueller;N. Mukund;A. Mullavey;J. Muth;T. Nelson;A. Neunzert;S. Nichols;E. Nitoglia;J. Oberling;J. Oh;S. Oh;R. Oram;R. Ormiston;N. Ormsby;C. Osthelder;D. Ottaway;H. Overmier;A. Pai;J. R. Palamos;F. Pannarale;W. Parker;O. Patane;M. Patel;E. Payne;A. Pele;R. Penhorwood;C. Perez;K. S. Phukon;M. Pillas;M. Pirello;H. Radkins;K. Ramirez;J. Richardson;K. Riles;K. Rink;N. Robertson;J. Rollins;C. Romel;J. Romie;M. Ross;K. Ryan;T. Sadecki;M. Sakellariadou;E. Sanchez;L. Sanchez;L. Sandles;T. R. Saravanan;R. Savage;D. Schaetzl;R. Schnabel;E. Schwartz;D. Sellers;T. Shaffer;D. Sigg;A. Sintes;B. Slagmolen;J. R. Smith;K. Soni;B. Sorazu;A. Spencer;K. Strain;D. Strom;L. Sun;M. Szczepańczyk;J. Tasson;R. Tenorio;M. Thomas;P. Thomas;K. Thorne;K. Toland;C. Torrie;A. Tran;G. Traylor;M. Trevor;M. Tse;G. Vajente;N. van Remortel;D. Vander-Hyde;A. Vargas;J. Veitch;P. Veitch;K. Venkateswara;Gautam Venugopalan;A. Viets;V. Villa-Ortega;T. Vo;C. Vorvick;M. Wade;G. Wallace;R. Ward;J. Warner;B. Weaver;A. Weinstein;R. Weiss;K. Wette;D. White;L. White;C. Whittle;A. Williamson;B. Willke;C. Wipf;L. Xiao;R. Xu;H. Yamamoto;Hang Yu;Haocun Yu;L. Zhang;Y. Zheng;M. Zucker;J. Zweizig