Proposal for UK Involvement in the Operation of Advanced LIGO

英国参与先进 LIGO 运营的提案

• 批准号: ST/N00003X/1
• 负责人: Kenneth Strain
• 金额: $ 49.4万
• 依托单位: University of Glasgow
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2016
• 资助国家: 英国
• 起止时间: 2016 至 无数据
• 项目状态: 已结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FN00003X%2F1
• 关键词: Proposal; UK; Involvement; Operation; Advanced

Within the next five years, and before the end of the period covered by this proposal, Advanced LIGO (aLIGO) is expected to detect gravitational waves and hence open a new era in astronomy. In this proposal we request support for essential infrastructure and travel costs required to ensure that the UK maintains its place among the leaders in the field and its partnership within the project.Through the design and construction project "Advanced LIGO UK", and building on existing strengths, the UK has succeeded in making unique and fundamental contributions to major aspects of the aLIGO gravitational wave detectors in the US, primarily by transfer of silica suspension technology originally developed at Glasgow for GEO600. The resulting suspensions are absolutely central in enabling aLIGO to meet its sensitivity target. During the first phase of operations, the UK supplied equipment has been installed and integrated into two aLIGO detectors. As a direct result, UK groups are in a position to exploit the rich science data that will be produced by these detectors and their observing partners during the current decade. We propose to strengthen the UK position by providing the support and infrastructure necessary for full involvement in the operation of the aLIGO detectors and therefore to remain active partners in the user-community group, the LIGO Scientific Collaboration (LSC), through which data rights are earned and distributed. Of similar importance is the need to ensure that UK-delivered equipment and facilities for the aLIGO detectors are fully exploited to maximise the science potential of aLIGO. This is true both in terms of their implementation within aLIGO, and later when it is planned that aLIGO will be further upgraded. The applicant groups are recognised leaders in the field of analysis of data from gravitational wave detectors. Novel methods were developed for searches with GEO600 and other detectors operational over the past decade. Leadership in this area has ensured that the UK groups have strong roles in all of the LSC data analysis groups that coordinate search campaigns, set priorities and validate results. This complements the similarly strong role that the UK has on the hardware side, in the LSC's technical working groups.The UK membership of the LSC is considerable - currently 12% by authorship. The ALUK project and exchange of data from GEO600 have allowed us to leverage top-level project management positions for a relatively small investment in the aLIGO hardware. This is set out in our Memorandum of Understanding (MOU) with LIGO, and includes a seat on the project Oversight Committee for an STFC representative and membership of the LSC Executive Committee. Of course we have full access to data and an equal share in the science return. It is essential that we maintain involvement at the highest level as set out in detail in this proposal. We therefore request travel support for essential observing duties and resources to allow us to provide technical support during detector commissioning and operations. Analysis of the data requires access to high performance computer infrastructure. With the first detections, demand for computing resources is certain to be high. Therefore, to provide a solid basis for exploitation of aLIGO science data within the UK we request computing infrastructure resources commensurate with our membership of the LSC.At the US LIGO sites - the LIGO Livingston and LIGO Hanford Observatories (LLO/LHO) - first tests of the completed detectors are underway, and in November 2014, just a few months after first operation, the LLO detector achieved sensitivity to coalescing binary neutron stars at over 50 megaparsec (Mpc) distance - well on target for initial science runs to start in 2015.

在未来五年内，在该计划所涵盖的时期结束之前，高级LIGO（aLIGO）有望探测到引力波，从而开启天文学的新时代。在这份提案中，我们请求支持必要的基础设施和差旅费用，以确保英国保持其在该领域的领导者地位以及在该项目中的合作伙伴关系。通过设计和建设项目“Advanced LIGO UK”，并在现有优势的基础上，英国成功地为美国的alIGO引力波探测器的主要方面做出了独特和根本性的贡献，主要通过转移最初在格拉斯哥为GEO 600开发的二氧化硅悬浮技术。由此产生的悬浮液是使aLIGO能够达到其灵敏度目标的绝对核心。在运行的第一阶段，联合王国提供的设备已经安装并集成到两个aLIGO探测器中。其直接结果是，英国的研究小组能够利用这些探测器及其观测伙伴在本十年期间产生的丰富科学数据。我们建议通过提供充分参与aLIGO探测器运行所需的支持和基础设施来加强英国的地位，因此继续积极参与用户社区组织LIGO科学合作（LSC），通过该组织获得和分配数据权利。同样重要的是，需要确保英国提供的用于aLIGO探测器的设备和设施得到充分利用，以最大限度地发挥aLIGO的科学潜力。无论是在alIGO中的实现，还是以后计划进一步升级alIGO时，都是如此。申请团队是引力波探测器数据分析领域公认的领导者。在过去十年中，为使用GEO 600和其他探测器进行搜索开发了新的方法。在这一领域的领导确保了英国小组在所有LSC数据分析小组中发挥重要作用，这些小组协调搜索活动，确定优先事项并验证结果。这补充了英国在LSC技术工作组中在硬件方面的类似强大作用。LSC的英国成员相当多-目前有12%的作者。ALUK项目和来自GEO 600的数据交换使我们能够利用顶级项目管理职位对aLIGO硬件进行相对较小的投资。这在我们与LIGO的谅解备忘录（MOU）中有所规定，其中包括STFC代表在项目监督委员会中的席位以及LSC执行委员会的成员资格。当然，我们有充分的机会获得数据，并在科学回报中享有平等的份额。至关重要的是，我们必须按照本提案的详细规定，保持最高级别的参与。因此，我们请求提供必要的观测职责和资源方面的差旅支持，以便我们能够在探测器调试和运行期间提供技术支持。数据分析需要访问高性能计算机基础设施。随着第一次检测，对计算资源的需求肯定会很高。因此，为了在英国境内利用aLIGO科学数据提供坚实的基础，我们要求与我们LSC成员资格相称的计算基础设施资源。在美国LIGO站点-LIGO利文斯顿和LIGO汉福德天文台（LLO/LHO）-完成的探测器的第一次测试正在进行中，并在2014年11月，在首次运行后的几个月，LLO探测器实现了对超过50兆秒差距（Mpc）距离的合并中子星的灵敏度--完全达到了2015年开始的初始科学运行的目标。

项目成果

Prospects for Observing and Localizing Gravitational-Wave Transients with Advanced LIGO and Advanced Virgo.

观察和定位带有晚期Ligo和晚期处女座的重力波瞬变的前景。

• DOI: 10.1007/lrr-2016-1
• 发表时间: 2016
• 期刊: Living reviews in relativity
• 影响因子: 40.6
• 作者: Abbott BP;LIGO Scientific Collaboration;Virgo Collaboration;Abbott R;Abbott TD;Abernathy MR;Acernese F;Ackley K;Adams C;Adams T;Addesso P;Adhikari RX;Adya VB;Affeldt C;Agathos M;Agatsuma K;Aggarwal N;Aguiar OD;Ain A;Ajith P;Allen B;Allocca A;Altin PA;Amariutei DV;Anderson SB;Anderson WG;Arai K;Araya MC;Arceneaux CC;Areeda JS;Arnaud N;Arun KG;Ashton G;Ast M;Aston SM;Astone P;Aufmuth P;Aulbert C;Babak S;Baker PT;Baldaccini F;Ballardin G;Ballmer SW;Barayoga JC;Barclay SE;Barish BC;Barker D;Barone F;Barr B;Barsotti L;Barsuglia M;Barta D;Bartlett J;Bartos I;Bassiri R;Basti A;Batch JC;Baune C;Bavigadda V;Bazzan M;Behnke B;Bejger M;Belczynski C;Bell AS;Bell CJ;Berger BK;Bergman J;Bergmann G;Berry CP;Bersanetti D;Bertolini A;Betzwieser J;Bhagwat S;Bhandare R;Bilenko IA;Billingsley G;Birch J;Birney R;Biscans S;Bisht A;Bitossi M;Biwer C;Bizouard MA;Blackburn JK;Blair CD;Blair D;Blair RM;Bloemen S;Bock O;Bodiya TP;Boer M;Bogaert G;Bogan C;Bohe A;Bojtos P;Bond C;Bondu F;Bonnand R;Bork R;Boschi V;Bose S;Bozzi A;Bradaschia C;Brady PR;Braginsky VB;Branchesi M;Brau JE;Briant T;Brillet A;Brinkmann M;Brisson V;Brockill P;Brooks AF;Brown DA;Brown DD;Brown NM;Buchanan CC;Buikema A;Bulik T;Bulten HJ;Buonanno A;Buskulic D;Buy C;Byer RL;Cadonati L;Cagnoli G;Cahillane C;Calderón Bustillo J;Callister T;Calloni E;Camp JB;Cannon KC;Cao J;Capano CD;Capocasa E;Carbognani F;Caride S;Casanueva Diaz J;Casentini C;Caudill S;Cavaglià M;Cavalier F;Cavalieri R;Cella G;Cepeda C;Cerboni Baiardi L;Cerretani G;Cesarini E;Chakraborty R;Chalermsongsak T;Chamberlin SJ;Chan M;Chao S;Charlton P;Chassande-Mottin E;Chen HY;Chen Y;Cheng C;Chincarini A;Chiummo A;Cho HS;Cho M;Chow JH;Christensen N;Chu Q;Chua S;Chung S;Ciani G;Clara F;Clark JA;Cleva F;Coccia E;Cohadon PF;Colla A;Collette CG;Constancio M Jr;Conte A;Conti L;Cook D;Corbitt TR;Cornish N;Corsi A;Cortese S;Costa CA;Coughlin MW;Coughlin SB;Coulon JP;Countryman ST;Couvares P;Coward DM;Cowart MJ;Coyne DC;Coyne R;Craig K;Creighton JD;Cripe J;Crowder SG;Cumming A;Cunningham L;Cuoco E;Dal Canton T;Danilishin SL;D'Antonio S;Danzmann K;Darman NS;Dattilo V;Dave I;Daveloza HP;Davier M;Davies GS;Daw EJ;Day R;DeBra D;Debreczeni G;Degallaix J;De Laurentis M;Deléglise S;Del Pozzo W;Denker T;Dent T;Dereli H;Dergachev V;DeRosa R;De Rosa R;DeSalvo R;Dhurandhar S;Díaz MC;Di Fiore L;Di Giovanni M;Di Lieto A;Di Palma I;Di Virgilio A;Dojcinoski G;Dolique V;Donovan F;Dooley KL;Doravari S;Douglas R;Downes TP;Drago M;Drever RW;Driggers JC;Du Z;Ducrot M;Dwyer SE;Edo TB;Edwards MC;Effler A;Eggenstein HB;Ehrens P;Eichholz JM;Eikenberry SS;Engels W;Essick RC;Etzel T;Evans M;Evans TM;Everett R;Factourovich M;Fafone V;Fair H;Fairhurst S;Fan X;Fang Q;Farinon S;Farr B;Farr WM;Favata M;Fays M;Fehrmann H;Fejer MM;Ferrante I;Ferreira EC;Ferrini F;Fidecaro F;Fiori I;Fisher RP;Flaminio R;Fletcher M;Fournier JD;Franco S;Frasca S;Frasconi F;Frei Z;Freise A;Frey R;Fricke TT;Fritschel P;Frolov VV;Fulda P;Fyffe M;Gabbard HA;Gair JR;Gammaitoni L;Gaonkar 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PG;Mytidis A;Nardecchia I;Naticchioni L;Nayak RK;Necula V;Nedkova K;Nelemans G;Neri M;Neunzert A;Newton G;Nguyen TT;Nielsen AB;Nissanke S;Nitz A;Nocera F;Nolting D;Normandin ME;Nuttall LK;Oberling J;Ochsner E;O'Dell J;Oelker E;Ogin GH;Oh JJ;Oh SH;Ohme F;Oliver M;Oppermann P;Oram RJ;O'Reilly B;O'Shaughnessy R;Ott CD;Ottaway DJ;Ottens RS;Overmier H;Owen BJ;Pai A;Pai SA;Palamos JR;Palashov O;Palomba C;Pal-Singh A;Pan H;Pankow C;Pannarale F;Pant BC;Paoletti F;Paoli A;Papa MA;Paris HR;Parker W;Pascucci D;Pasqualetti A;Passaquieti R;Passuello D;Patrick Z;Pearlstone BL;Pedraza M;Pedurand R;Pekowsky L;Pele A;Penn S;Pereira R;Perreca A;Phelps M;Piccinni O;Pichot M;Piergiovanni F;Pierro V;Pillant G;Pinard L;Pinto IM;Pitkin M;Poggiani R;Post A;Powell J;Prasad J;Predoi V;Premachandra SS;Prestegard T;Price LR;Prijatelj M;Principe M;Privitera S;Prodi GA;Prokhorov L;Punturo M;Puppo P;Pürrer M;Qi H;Qin J;Quetschke V;Quintero EA;Quitzow-James R;Raab FJ;Rabeling DS;Radkins H;Raffai P;Raja S;Rakhmanov 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D;Stephens BC;Stone R;Strain KA;Straniero N;Stratta G;Strauss NA;Strigin S;Sturani R;Stuver AL;Summerscales TZ;Sun L;Sutton PJ;Swinkels BL;Szczepanczyk MJ;Tacca M;Talukder D;Tanner DB;Tápai M;Tarabrin SP;Taracchini A;Taylor R;Theeg T;Thirugnanasambandam MP;Thomas EG;Thomas M;Thomas P;Thorne KA;Thorne KS;Thrane E;Tiwari S;Tiwari V;Tokmakov KV;Tomlinson C;Tonelli M;Torres CV;Torrie CI;Töyrä D;Travasso F;Traylor G;Trifirò D;Tringali MC;Trozzo L;Tse M;Turconi M;Tuyenbayev D;Ugolini D;Unnikrishnan CS;Urban AL;Usman SA;Vahlbruch H;Vajente G;Valdes G;van Bakel N;van Beuzekom M;van den Brand JF;van den Broeck C;Vander-Hyde DC;van der Schaaf L;van der Sluys MV;van Heijningen JV;van Veggel AA;Vardaro M;Vass S;Vasúth M;Vaulin R;Vecchio A;Vedovato G;Veitch J;Veitch PJ;Venkateswara K;Verkindt D;Vetrano F;Viceré A;Vinciguerra S;Vine DJ;Vinet JY;Vitale S;Vo T;Vocca H;Vorvick C;Vousden WD;Vyatchanin SP;Wade AR;Wade LE;Wade M;Walker M;Wallace L;Walsh S;Wang G;Wang H;Wang M;Wang X;Wang Y;Ward RL;Warner J;Was M;Weaver B;Wei LW;Weinert M;Weinstein AJ;Weiss R;Welborn T;Wen L;Weßels P;Westphal T;Wette K;Whelan JT;White DJ;Whiting BF;Williams RD;Williamson AR;Willis JL;Willke B;Wimmer MH;Winkler W;Wipf CC;Wittel H;Woan G;Worden J;Wright JL;Wu G;Yablon J;Yam W;Yamamoto H;Yancey CC;Yap MJ;Yu H;Yvert M;Zadrożny A;Zangrando L;Zanolin M;Zendri JP;Zevin M;Zhang F;Zhang L;Zhang M;Zhang Y;Zhao C;Zhou M;Zhou Z;Zhu XJ;Zucker ME;Zuraw SE;Zweizig J
• 通讯作者: Zweizig J

Upper Limits on Gravitational Waves from Scorpius X-1 from a Model-Based Cross-Correlation Search in Advanced LIGO Data

• DOI: 10.3847/1538-4357/aa86f0
• 发表时间: 2017-06
• 作者: The Ligo Scientific Collaboration;T. Abbott;R. Abbott;T. Abbott;F. Acernese;K. Ackley;C. Adams;T. Adams;P. Addesso;R. Adhikari;V. Adya;C. Affeldt;M. Afrough;B. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;B. Allen;G. Allen;A. Allocca;P. Altin;A. Amato;A. Ananyeva;S. Anderson;W. Anderson;S. Antier;S. Appert;K. Arai;M. Araya;J. Areeda;N. Arnaud;K. Arun;S. Ascenzi;G. Ashton;M. Ast;S. Aston;P. Astone;P. Aufmuth;C. Aulbert;K. AultONeal;A. Ávila-Álvarez;S. Babak;P. Bacon;M. Bader;S. Bae;P. Baker;F. Baldaccini;G. Ballardin;S. Ballmer;S. Banagiri;J. Barayoga;S. Barclay;B. Barish;D. Barker;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;I. Bartos;R. Bassiri;A. Basti;J. Batch;C. Baune;M. Bawaj;M. Bazzan;B. B'ecsy;C. Beer;M. Bejger;I. Belahcene;A. Bell;B. Berger;G. Bergmann;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;S. Bhagwat;R. Bhandare;I. Bilenko;G. Billingsley;C. Billman;J. Birch;R. Birney;O. Birnholtz;S. Biscans;A. Bisht;M. Bitossi;C. Biwer;M. Bizouard;J. K. Blackburn;J. Blackman;C. Blair;D. Blair;R. Blair;S. Bloemen;O. Bock;N. Bode;M. Boer;G. Bogaert;A. Bohe;F. Bondu;R. Bonnand;B. A. Boom;R. Bork;V. Boschi;S. Bose;Y. Bouffanais;A. Bozzi;C. Bradaschia;P. Brady;V. Braginsky;M. Branchesi;J. Brau;T. Briant;A. Brillet;M. Brinkmann;V. Brisson;P. Brockill;J. Broida;A. Brooks;D. Brown;D. Brown;N. Brown;S. Brunett;C. Buchanan;A. Buikema;T. Bulik;H. Bulten;A. Buonanno;D. Buskulic;C. Buy;R. Byer;M. Cabero;L. Cadonati;G. Cagnoli;C. Cahillane;J. C. Bustillo;T. Callister;E. Calloni;J. Camp;M. Canepa;P. Canizares;K. Cannon;H. Cao;J. Cao;C. Capano;E. Capocasa;F. Carbognani;S. Caride;M. Carney;J. C. Diaz;C. Casentini;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;G. Cella;C. Cepeda;L. Baiardi;G. Cerretani;E. Cesarini;S. Chamberlin;M. Chan;S. Chao;P. Charlton;E. Chassande-Mottin;D. Chatterjee;K. Chatziioannou;B. Cheeseboro;H. Chen;Y. Chen;H.-P. Cheng;A. Chincarini;A. Chiummo;T. Chmiel;H. Cho;M. Cho;J. Chow;N. Christensen;Q. Chu;A. J. Chua;S. Chua;A. K. Chung;S. Chung;G. Ciani;R. Ciolfi;C. Cirelli;A. Cirone;F. Clara;J. Clark;F. Cleva;C. Cocchieri;E. Coccia;P. Cohadon;A. Colla;C. Collette;L. Cominsky;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;K. Corley;N. Cornish;A. Corsi;S. Cortese;C. Costa;M. Coughlin;S. Coughlin;J. Coulon;S. Countryman;P. Couvares;P. Covas;E. Cowan;D. Coward;M. Cowart;D. Coyne;R. Coyne;J. Creighton;T. Creighton;J. Cripe;S. Crowder;T. Cullen;A. Cumming;L. Cunningham;E. Cuoco;T. D. Canton;S. Danilishin;S. D’Antonio;K. Danzmann;A. Dasgupta;C. F. S. Costa;V. Dattilo;I. Dave;M. Davier;D. Davis;E. Daw;B. Day;S. De;D. DeBra;E. Deelman;J. Degallaix;M. D. Laurentis;S. Del'eglise;W. D. Pozzo;T. Denker;T. Dent;V. Dergachev;R. Rosa;R. Derosa;R. DeSalvo;J. Devenson;R. Devine;S. Dhurandhar;M. D'iaz;L. Fiore;M. Giovanni;T. D. Girolamo;A. D. Lieto;S. D. Pace;I. Palma;F. Renzo;Zoheyr Doctor;V. Dolique;F. Donovan;K. Dooley;S. Doravari;I. Dorrington;R. Douglas;M. D. Álvarez;T. Downes;M. Drago;R. Drever;J. Driggers;Z. Du;M. Ducrot;J. Duncan;S. Dwyer;T. Edo;M. Edwards;A. Effler;H. Eggenstein;P. Ehrens;J. Eichholz;S. Eikenberry;R. Eisenstein;R. Essick;Z. Etienne;T. Etzel;M. Evans;T. Evans;M. Factourovich;V. Fafone;H. Fair;S. Fairhurst;X. Fan;S. Farinon;B. Farr;W. Farr;E. Fauchon-Jones;Marc Favata;M. Fays;H. Fehrmann;J. Feicht;M. Fejer;Á. Fernández-Galiana;I. Ferrante;E. Ferreira;F. Ferrini;F. Fidecaro;I. Fiori;D. Fiorucci;R. Fisher;R. Flaminio;M. Fletcher;H. Fong;P. Forsyth;S. Forsyth;J. Fournier;S. Frasca;F. Frasconi;Z. Frei;A. Freise;R. Frey;V. Frey;E. Fries;P. Fritschel;V. Frolov;P. Fulda;M. Fyffe;H. Gabbard;M. Gabel;B. Gadre;S. Gaebel;J. Gair;D. Galloway;L. Gammaitoni;M. Ganija;S. Gaonkar;F. Garufi;S. Gaudio;G. Gaur;V. Gayathri;N. Gehrels;G. Gemme;Eric Genin;A. Gennai;D. George;J. George;L. Gergely;V. Germain;S. Ghonge;A. Ghosh;A. Ghosh;S. Ghosh;J. Giaime;K. Giardina;A. Giazotto;K. Gill;L. Glover;E. Goetz;R. Goetz;S. Gomes;G. Gonz'alez;J. M. Castro;A. Gopakumar;M. Gorodetsky;S. Gossan;M. Gosselin;R. Gouaty;A. Grado;C. Graef;M. Granata;A. Grant;S. Gras;C. Gray;G. Greco;A. Green;P. Groot;H. Grote;S. Grunewald;P. Gruning;G. Guidi;X. Guo;A. Gupta;M. Gupta;K. Gushwa;E. Gustafson;R. Gustafson;B. Hall;E. Hall;G. Hammond;M. Haney;M. Hanke;J. Hanks;C. Hanna;O. Hannuksela;J. Hanson;T. Hardwick;J. Harms;G. Harry;I. Harry;M. Hart;C. Haster;K. Haughian;J. Healy;A. Heidmann;M. Heintze;H. Heitmann;P. Hello;G. Hemming;M. Hendry;I. Heng;J. Hennig;J. Henry;A. Heptonstall;M. Heurs;S. Hild;D. Hoak;D. Hofman;K. Holt;D. Holz;P. Hopkins;C. Horst;J. Hough;E. Houston;E. Howell;Y. Hu;E. Huerta;D. Huet;B. Hughey;S. Husa;S. Huttner;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;N. Indik;D. Ingram;R. Inta;G. Intini;H. N. Isa;J. Isac;M. Isi;B. Iyer;K. Izumi;T. Jacqmin;K. Jani;P. Jaranowski;S. Jawahar;F. Jim'enez-Forteza;W. Johnson;D. Jones;R. Jones;R. Jonker;L. Ju;J. Junker;C. Kalaghatgi;V. Kalogera;S. Kandhasamy;G. Kang;J. Kanner;S. Karki;K. Karvinen;M. Kasprzack;M. Katolik;E. Katsavounidis;W. Katzman;S. Kaufer;K. Kawabe;F. K'ef'elian;D. Keitel;A. Kemball;R. Kennedy;C. Kent;J. Key;F. Khalili;I. Khan;S. Khan;Z. Khan;E. Khazanov;N. Kijbunchoo;Chunglee Kim;J. Kim;W. Kim;W. Kim;Y. Kim;S. Kimbrell;E. King;P. King;R. Kirchhoff;J. S. Kissel;L. Kleybolte;S. Klimenko;P. Koch;S. Koehlenbeck;S. Koley;V. Kondrashov;A. Kontos;M. Korobko;W. Korth;I. Kowalska;D. Kozak;C. Kramer;V. Kringel;B. Krishnan;A. Kr'olak;G. Kuehn;P. Kumar;R. Kumar;S. Kumar;L. Kuo;A. Kutynia;S. Kwang;B. Lackey;K. Lai;M. Landry;R. Lang;J. Lange;B. Lantz;R. Lanza;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;C. Lee;H. Lee;H. Lee;H. W. Lee;K. Lee;J. Lehmann;A. Lenon;M. Leonardi;N. Leroy;N. Letendre;Y. Levin;T. G. F. Li;A. Libson;T. Littenberg;J. Liu;R. K. Lo;N. Lockerbie;L. London;J. Lord;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;J. Lough;C. Lousto;G. Lovelace;H. Luck;D. Lumaca;A. Lundgren;R. Lynch;Y. Ma;S. Macfoy;B. Machenschalk;M. Macinnis;D. Macleod;I. M. Hernandez;F. Magaña-Sandoval;L. M. Zertuche;R. Magee;E. Majorana;I. Maksimovic;N. Man;V. Mandic;V. Mangano;G. Mansell;M. Manske;M. Mantovani;F. Marchesoni;F. Marion;S. M'arka;Z. M'arka;C. Markakis;A. Markosyan;E. Maros;F. Martelli;L. Martellini;I. Martin;D. Martynov;K. Mason;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;F. Matichard;L. Matone;N. Mavalvala;R. Mayani;N. Mazumder;R. Mccarthy;D. McClelland;S. Mccormick;L. McCuller;S. Mcguire;G. Mcintyre;J. McIver;D. McManus;T. McRae;S. McWilliams;D. Meacher;G. Meadors;J. Meidam;E. Mejuto-Villa;A. Melatos;G. Mendell;R. Mercer;E. Merilh;M. Merzougui;S. Meshkov;C. Messenger;C. Messick;R. Metzdorff;P. Meyers;F. Mezzani;H. Miao;C. Michel;H. Middleton;E. Mikhailov;L. Milano;A. Miller;A. Miller;B. Miller;J. Miller;M. Millhouse;O. Minazzoli;Y. Minenkov;J. Ming;C. Mishra;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;A. Moggi;M. Mohan;S. Mohapatra;M. Montani;B. Moore;C. Moore;D. Moraru;G. Moreno;S. Morriss;B. 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Pinto;M. Pitkin;R. Poggiani;P. Popolizio;E. Porter;A. Post;J. Powell;J. Prasad;J. Pratt;V. Predoi;T. Prestegard;M. Prijatelj;M. Principe;S. Privitera;R. Prix;G. Prodi;L. Prokhorov;O. Puncken;M. Punturo;P. Puppo;M. Purrer;H. Qi;J. Qin;S. Qiu;V. Quetschke;E. Quintero;R. Quitzow-James;F. Raab;D. Rabeling;H. Radkins;P. Raffai;S. Raja;C. Rajan;M. Rakhmanov;K. Ramirez;P. Rapagnani;V. Raymond;M. Razzano;J. Read;T. Regimbau;L. Rei;S. Reid;D. Reitze;H. Rew;S. Reyes;F. Ricci;P. Ricker;S. Rieger;K. Riles;M. Rizzo;N. Robertson;R. Robie;F. Robinet;A. Rocchi;L. Rolland;J. Rollins;V. Roma;R. Romano;C. Romel;J. Romie;D. Rosi'nska;M. Ross;S. Rowan;A. Rudiger;P. Ruggi;K. Ryan;M. Rynge;S. Sachdev;T. Sadecki;L. Sadeghian;M. Sakellariadou;L. Salconi;M. Saleem;F. Salemi;A. Samajdar;L. Sammut;L. Sampson;E. Sanchez;V. Sandberg;B. Sandeen;J. Sanders;B. Sassolas;B. Sathyaprakash;P. Saulson;O. Sauter;R. Savage;A. Sawadsky;P. Schale;J. Scheuer;E. Schmidt;J. Schmidt;P. Schmidt;R. Schnabel;R. Schofield;A. Schonbeck;E. Schreiber;D. Schuette;B. Schulte;B. Schutz;S. Schwalbe;J. Scott;S. Scott;E. Seidel;D. Sellers;A. Sengupta;D. Sentenac;V. Sequino;A. Sergeev;D. Shaddock;T. Shaffer;A. A. Shah-A.;M. Shahriar;L. Shao;B. Shapiro;P. Shawhan;A. Sheperd;D. Shoemaker;D. Shoemaker;K. Siellez;X. Siemens;M. Sieniawska;D. Sigg;A. D. Silva;A. Singer;L. Singer;A. Singh;R. Singh;A. Singhal;A. Sintes;B. Slagmolen;B. Smith;J. R. Smith;R. Smith;E. Son;J. Sonnenberg;B. Sorazu;F. Sorrentino;T. Souradeep;A. Spencer;A. Srivastava;A. Staley;M. Steinke;J. Steinlechner;S. Steinlechner;D. Steinmeyer;B. Stephens;R. Stone;K. Strain;G. Stratta;S. Strigin;R. Sturani;A. Stuver;T. Summerscales;L. Sun;S. Sunil;P. Sutton;B. Swinkels;M. J. Szczepa'nczyk;M. Tacca;D. Talukder;D. Tanner;M. T'apai;A. Taracchini;J. A. Taylor;R. Taylor;T. Theeg;E. Thomas;M. Thomas;P. Thomas;K. Thorne;K. Thorne;E. Thrane;S. Tiwari;V. Tiwari;K. Tokmakov;K. Toland;M. Tonelli;Z. Tornasi;C. Torrie;D. Toyra;F. Travasso;G. Traylor;D. Trifirò;J. Trinastic;M. Tringali;L. Trozzo;K. W. Tsang;M. Tse;R. Tso;D. Tuyenbayev;K. Ueno;D. Ugolini;C. Unnikrishnan;A. Urban;S. Usman;K. Vahi;H. Vahlbruch;G. Vajente;G. Valdes;M. Vallisneri;N. Bakel;M. Beuzekom;J. Brand;C. Broeck;D. Vander-Hyde;L. V. D. Schaaf;J. V. Heijningen;A. V. Veggel;M. Vardaro;V. Varma;S. Vass;M. Vas'uth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;K. Venkateswara;Gautam Venugopalan;D. Verkindt;F. Vetrano;A. Vicer'e;A. Viets;S. Vinciguerra;D. Vine;J. Vinet;S. Vitale;T. Vo;H. Vocca;C. Vorvick;D. Voss;W. Vousden;S. Vyatchanin;A. Wade;L. Wade;M. Wade;R. Walet;M. Walker;L. Wallace;S. Walsh;G. Wang;H. Wang;J. Wang;M. Wang;Y.-F. Wang;Y. Wang;R. Ward;J. Warner;M. Was;J. Watchi;B. Weaver;L.-W. Wei;M. Weinert;A. Weinstein;R. Weiss;L. Wen;E. Wessel;P. Wessels;T. Westphal;K. Wette;J. Whelan;B. Whiting;C. Whittle;D. Williams;R. Williams;A. Williamson;J. Willis;B. Willke;M. Wimmer;W. Winkler;C. Wipf;H. Wittel;G. Woan;J. Woehler;J. Wofford;K. Wong;J. Worden;J. Wright;D. Wu;G. Wu;W. Yam;H. Yamamoto;C. Yancey;M. Yap;Hang Yu;Haocun Yu;M. Yvert;A. Zadro.zny;M. Zanolin;T. Zelenova;J. Zendri;M. Zevin;L. Zhang;M. Zhang;T. Zhang;Y.H. Zhang;C. Zhao;M. Zhou;Z. Zhou;X. Zhu;M. Zucker;J. Zweizig;D. Steeghs;L. Wang

Search for Eccentric Binary Black Hole Mergers with Advanced LIGO and Advanced Virgo during Their First and Second Observing Runs

• DOI: 10.3847/1538-4357/ab3c2d
• 发表时间: 2019-10-01
• 期刊: ASTROPHYSICAL JOURNAL
• 影响因子: 4.9
• 作者: Abbott, B. P.;Abbott, R.;Salemi, F.
• 通讯作者: Salemi, F.

Low-latency Gravitational-wave Alerts for Multimessenger Astronomy during the Second Advanced LIGO and Virgo Observing Run

• DOI: 10.3847/1538-4357/ab0e8f
• 发表时间: 2019-04-20
• 期刊: ASTROPHYSICAL JOURNAL
• 影响因子: 4.9
• 作者: Abbott, B. P.;Abbott, R.;Zweizig, J.
• 通讯作者: Zweizig, J.

Estimating the Contribution of Dynamical Ejecta in the Kilonova Associated with GW170817

• DOI: 10.3847/2041-8213/aa9478
• 发表时间: 2017-12-01
• 期刊: ASTROPHYSICAL JOURNAL LETTERS
• 影响因子: 7.9
• 作者: Abbott, B. P.;Abbott, R.;Zweizig, J.
• 通讯作者: Zweizig, J.