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/N000072/1
• 负责人: Alberto Vecchio
• 金额: $ 31.07万
• 依托单位: University of Birmingham
• 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%2FN000072%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.

在接下来的五年内，也就是在这一提议所涵盖的时期结束之前，高级LIGO(ALIGO)有望探测到引力波，从而开启天文学的一个新纪元。在这份提案中，我们要求为必要的基础设施和旅行成本提供支持，以确保英国保持其在该领域的领先地位及其在该项目中的合作伙伴关系。通过设计和建设项目“Advanced LIGO UK”，并建立在现有优势的基础上，英国成功地对美国aLIGO引力波探测器的主要方面做出了独特和基本的贡献，主要是通过转让最初在格拉斯哥为GEO600开发的二氧化硅悬浮技术。由此产生的暂停绝对是使ALIGO达到其敏感性目标的关键。在第一阶段的运行中，英国提供的设备已经安装并集成到两个aLIGO探测器中。直接的结果是，英国的团体能够利用这些探测器及其观测伙伴在当前十年将产生的丰富科学数据。我们建议加强联合王国的地位，为全面参与aLIGO探测器的运作提供必要的支持和基础设施，并因此继续成为用户社区小组--LIGO科学协作(LSC)的积极合作伙伴，通过该小组获得和分发数据权。同样重要的是需要确保英国提供的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。无论是它们在aLIGO中的实现，还是后来计划进一步升级aLIGO时，都是如此。申请团体是引力波探测器数据分析领域公认的领导者。在过去的十年里，开发了使用GEO600和其他探测器进行搜索的新方法。在这一领域的领导地位确保了英国小组在所有LSC数据分析小组中发挥强大的作用，这些小组负责协调搜索活动、设定优先事项和验证结果。这是对英国在硬件方面的类似强大作用的补充，在LSC的技术工作组中。英国是LSC的相当大的成员-目前按作者身份计算为12%。Aluk项目和来自GEO600的数据交换使我们能够利用顶级项目管理职位在aLIGO硬件上进行相对较小的投资。这在我们与LIGO的谅解备忘录(MOU)中列出，并包括STFC代表在项目监督委员会的一个席位和LSC执行委员会的成员。当然，我们完全可以访问数据，并在科学回报中享有平等份额。至关重要的是，我们必须保持这项提议中详细规定的最高级别的参与。因此，我们要求为必要的观测任务和资源提供差旅支持，以便我们能够在探测器调试和运行期间提供技术支持。数据分析需要使用高性能的计算机基础设施。对于第一次检测，对计算资源的需求肯定很高。因此，为了为在英国境内利用LIGO科学数据提供坚实的基础，我们需要与我们的LSC成员资格相称的计算基础设施资源。在美国的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，2014年11月，在首次运行几个月后，LLO探测器实现了对超过50兆秒(MPC)距离的双星中子星聚合的灵敏度-很好地实现了2015年开始的初步科学运行的目标。

项目成果

Effects of data quality vetoes on a search for compact binary coalescences in Advanced LIGO's first observing run

• DOI: 10.1088/1361-6382/aaaafa
• 发表时间: 2018-03-22
• 期刊: CLASSICAL AND QUANTUM GRAVITY
• 影响因子: 3.5
• 作者: Abbott, B. P.;Abbott, R.;Zweizig, J.
• 通讯作者: Zweizig, J.

Narrow-band search for gravitational waves from known pulsars using the second LIGO observing run

• DOI: 10.1103/physrevd.99.122002
• 发表时间: 2019-02
• 作者: The Ligo Scientific Collaboration;T. Abbott;R. Abbott;T. Abbott;S. Abraham;F. Acernese;K. Ackley;C. Adams;R. Adhikari;V. Adya;C. Affeldt;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;G. Allen;A. Allocca;M. Aloy;P. Altin;A. Amato;A. Ananyeva;S. Anderson;W. Anderson;S. Angelova;S. Antier;S. Appert;K. Arai;M. Araya;J. Areeda;M. Arène;N. Arnaud;S. Ascenzi;G. Ashton;S. Aston;P. Astone;F. Aubin;P. Aufmuth;K. AultONeal;C. Austin;V. Avendano;A. Ávila-Álvarez;S. Babak;P. Bacon;F. Badaracco;M. Bader;S. Bae;P. Baker;F. Baldaccini;G. Ballardin;S. Ballmer;S. Banagiri;J. Barayoga;S. Barclay;B. Barish;D. Barker;K. Barkett;S. Barnum;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;I. Bartos;R. Bassiri;A. Basti;M. Bawaj;J. Bayley;M. Bazzan;B. B'ecsy;M. Bejger;I. Belahcene;A. Bell;D. Beniwal;B. Berger;G. Bergmann;S. Bernuzzi;J. Bero;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;R. Bhandare;J. Bidler;I. Bilenko;S. Bilgili;G. Billingsley;J. Birch;R. Birney;O. Birnholtz;S. Biscans;S. Biscoveanu;A. Bisht;M. Bitossi;M. Bizouard;J. Blackburn;C. Blair;D. Blair;R. Blair;S. Bloemen;N. Bode;M. Boer;Y. Boetzel;G. Bogaert;F. Bondu;E. Bonilla;R. Bonnand;P. Booker;B. A. Boom;C. Booth;R. Bork;V. Boschi;S. Bose;K. Bossie;V. Bossilkov;J. Bosveld;Y. Bouffanais;A. Bozzi;C. Bradaschia;P. Brady;A. Bramley;M. Branchesi;J. Brau;T. Briant;J. Briggs;F. Brighenti;A. Brillet;M. Brinkmann;V. Brisson;P. Brockill;A. Brooks;D. Brown;S. Brunett;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;W. Campbell;M. Canepa;K. Cannon;H. Cao;J. Cao;E. Capocasa;F. Carbognani;S. Caride;M. Carney;Gregorio Carullo;J. C. Diaz;C. Casentini;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;G. Cella;P. Cerd'a-Dur'an;G. Cerretani;E. Cesarini;O. Chaibi;K. Chakravarti;S. Chamberlin;M. Chan;S. Chao;P. Charlton;E. Chase;É. Chassande-Mottin;D. Chatterjee;M. Chaturvedi;B. Cheeseboro;H. Chen;X. Chen;Y. Chen;H.-P. Cheng;C. Cheong;H. Chia;A. Chincarini;A. Chiummo;G. Cho;H. Cho;M. Cho;N. Christensen;Q. Chu;S. Chua;K. Chung;S. Chung;G. Ciani;A. Ciobanu;R. Ciolfi;F. Cipriano;A. Cirone;F. Clara;J. Clark;P. Clearwater;F. Cleva;C. Cocchieri;E. Coccia;P. Cohadon;D. Cohen;R. Colgan;M. Colleoni;C. Collette;C. Collins;L. Cominsky;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;I. Cordero-Carri'on;K. Corley;N. Cornish;A. Corsi;S. Cortese;C. Costa;R. Cotesta;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;M. Croquette;S. Crowder;T. Cullen;A. Cumming;L. Cunningham;E. Cuoco;T. D. Canton;G. D'alya;S. Danilishin;S. D’Antonio;K. Danzmann;A. Dasgupta;C. F. S. Costa;L. Datrier;V. Dattilo;I. Dave;M. Davier;D. Davis;E. Daw;D. DeBra;M. Deenadayalan;J. Degallaix;M. D. Laurentis;S. Del'eglise;W. D. Pozzo;L. DeMarchi;N. Demos;T. Dent;R. Pietri;J. Derby;R. Rosa;C. D. Rossi;R. DeSalvo;O. D. Varona;S. Dhurandhar;M. D'iaz;T. Dietrich;L. Fiore;M. Giovanni;T. D. Girolamo;A. Lieto;B. Ding;S. D. Pace;I. Palma;F. Renzo;A. Dmitriev;Zoheyr Doctor;F. Donovan;K. Dooley;S. Doravari;I. Dorrington;T. Downes;M. Drago;J. Driggers;Z. Du;J. Ducoin;P. Dupej;S. Dwyer;P. Easter;T. Edo;M. Edwards;A. Effler;P. Ehrens;J. Eichholz;S. Eikenberry;M. Eisenmann;R. Eisenstein;R. Essick;H. Estellés;D. Estevez;Z. Etienne;T. Etzel;M. Evans;T. Evans;V. Fafone;H. Fair;S. Fairhurst;X. Fan;S. Farinon;B. Farr;W. Farr;E. Fauchon-Jones;Marc Favata;M. Fays;M. Fazio;C. Fee;J. Feicht;M. Fejer;F. Feng;Á. Fernández-Galiana;I. Ferrante;E. Ferreira;T. A. Ferreira;F. Ferrini;F. Fidecaro;I. Fiori;D. Fiorucci;M. Fishbach;R. Fisher;J. Fishner;M. Fitz-Axen;R. Flaminio;M. Fletcher;E. Flynn;H. Fong;J. Font;P. Forsyth;J. Fournier;S. Frasca;F. Frasconi;Z. Frei;A. Freise;R. Frey;V. Frey;P. Fritschel;V. Frolov;P. Fulda;M. Fyffe;H. Gabbard;B. Gadre;S. Gaebel;J. Gair;L. Gammaitoni;M. Ganija;S. Gaonkar;A. 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Holgado;N. Holland;K. Holt;D. Holz;P. Hopkins;C. Horst;J. Hough;E. Howell;C. Hoy;A. Hreibi;E. Huerta;D. Huet;B. Hughey;M. Hulko;S. Husa;S. Huttner;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;B. Idzkowski;A. Iess;C. Ingram;R. Inta;G. Intini;B. Irwin;H. N. Isa;J. Isac;M. Isi;B. Iyer;K. Izumi;T. Jacqmin;S. Jadhav;K. Jani;N. Janthalur;P. Jaranowski;A. Jenkins;J. Jiang;D. S. Johnson;A. Jones;D. Jones;R. Jones;R. Jonker;L. Ju;J. Junker;C. Kalaghatgi;V. Kalogera;B. Kamai;S. Kandhasamy;G. Kang;J. Kanner;S. Kapadia;S. Karki;K. Karvinen;R. Kashyap;M. Kasprzack;S. Katsanevas;E. Katsavounidis;W. Katzman;S. Kaufer;K. Kawabe;N. V. Keerthana;F. K'ef'elian;D. Keitel;R. Kennedy;J. Key;F. Khalili;H. Khan;I. Khan;S. Khan;Z. Khan;E. Khazanov;M. Khursheed;N. Kijbunchoo;Chunglee Kim;J. Kim;K. Kim;W. Kim;W. Kim;Y. Kim;C. Kimball;E. King;P. King;M. Kinley-Hanlon;R. Kirchhoff;J. Kissel;L. Kleybolte;J. H. Klika;S. Klimenko;T. Knowles;P. Koch;S. Koehlenbeck;G. Koekoek;S. Koley;V. Kondrashov;A. Kontos;N. Koper;M. Korobko;W. Korth;I. Kowalska;D. Kozak;V. Kringel;N. Krishnendu;A. Kr'olak;G. Kuehn;A. Kumar;P. Kumar;R. Kumar;S. Kumar;L. Kuo;A. Kutynia;S. Kwang;B. Lackey;K. Lai;T. Lam;M. Landry;B. Lane;R. Lang;J. Lange;B. Lantz;R. Lanza;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;Y. Lecoeuche;C. Lee;H. Lee;H. Lee;H. W. Lee;J. Lee;K. Lee;J. Lehmann;A. Lenon;N. Leroy;N. Letendre;Y. Levin;J. Li;K. Li;T. G. F. Li;X. Li;F. Lin;F. Linde;S. Linker;T. Littenberg;J. Liu;X. Liu;R. K. Lo;N. Lockerbie;L. London;A. Longo;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;J. Lough;G. Lovelace;M. Lower;H. Luck;D. Lumaca;A. Lundgren;R. Lynch;Y. Ma;R. Macas;S. Macfoy;M. Macinnis;D. Macleod;A. Macquet;F. Magaña-Sandoval;L. M. Zertuche;R. Magee;E. Majorana;I. Maksimovic;A. Malik;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;A. Markowitz;E. Maros;A. Marquina;S. Marsat;F. Martelli;I. Martin;R. Martin;D. 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Sharma;P. Shawhan;H. Shen;R. Shink;D. Shoemaker;D. Shoemaker;S. Shyamsundar;K. Siellez;M. Sieniawska;D. Sigg;A. Silva;L. Singer;N. Singh;A. Singhal;A. Sintes;S. Sitmukhambetov;V. Skliris;B. Slagmolen;T. Slaven-Blair;J. R. Smith;R. Smith;S. Somala;E. Son;B. Sorazu;F. Sorrentino;T. Souradeep;E. Sowell;A. Spencer;A. Srivastava;V. Srivastava;K. Staats;C. Stachie;M. Standke;D. Steer;M. Steinke;J. Steinlechner;S. Steinlechner;D. Steinmeyer;S. Stevenson;D. Stocks;R. Stone;D. Stops;K. Strain;G. Stratta;S. Strigin;A. Strunk;R. Sturani;A. Stuver;V. Sudhir;T. Summerscales;L. Sun;S. Sunil;J. Suresh;P. Sutton;B. Swinkels;M. J. Szczepa'nczyk;M. Tacca;S. Tait;C. Talbot;D. Talukder;D. Tanner;M. T'apai;A. Taracchini;J. Tasson;R. Taylor;F. Thies;M. Thomas;P. Thomas;S. R. Thondapu;K. Thorne;E. Thrane;S. Tiwari;S. Tiwari;V. Tiwari;K. Toland;M. Tonelli;Z. Tornasi;A. Torres-Forn'e;C. Torrie;D. Toyra;F. Travasso;G. Traylor;M. Tringali;A. Trovato;L. Trozzo;R. Trudeau;K. W. Tsang;M. Tse;R. Tso;L. Tsukada;D. Tsuna;D. Tuyenbayev;K. Ueno;D. Ugolini;C. Unnikrishnan;A. Urban;S. A. Usman;H. Vahlbruch;G. Vajente;G. Valdes;N. Bakel;M. Beuzekom;J. Brand;C. Broeck;D. Vander-Hyde;J. V. Heijningen;L. V. D. Schaaf;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;D. Vine;J. Vinet;S. Vitale;T. Vo;H. Vocca;C. Vorvick;S. Vyatchanin;A. Wade;L. Wade;M. Wade;R. Walet;M. Walker;L. Wallace;S. Walsh;G. Wang;H. Wang;J. Wang;W. H. Wang;Y. Wang;R. Ward;Z. A. Warden;J. Warner;M. Was;J. Watchi;B. Weaver;L.-W. Wei;M. Weinert;A. Weinstein;R. Weiss;F. Wellmann;L. Wen;E. Wessel;P. Wessels;J. Westhouse;K. Wette;J. Whelan;B. Whiting;C. Whittle;D. Wilken;D. Williams;A. Williamson;J. Willis;B. Willke;M. Wimmer;W. Winkler;C. Wipf;H. Wittel;G. Woan;J. Woehler;J. Wofford;J. Worden;J. Wright;D. Wu;D. Wysocki;L. Xiao;H. Yamamoto;C. Yancey;L. Yang;M. Yap;M. Yazback;D. Yeeles;Hang Yu;Haocun Yu;S. Yuen;M. Yvert;A. Zadro.zny;M. Zanolin;T. Zelenova;J. Zendri;M. Zevin;J. Zhang;L. Zhang;T. Zhang;C. Zhao;M. Zhou;Z. Zhou;X. Zhu;M. Zucker;J. Zweizig;M. Keith;A. Lyne;B. Stappers;P. Weltevrede

Search for Gravitational-wave Signals Associated with Gamma-Ray Bursts during the Second Observing Run of Advanced LIGO and Advanced Virgo

在 Advanced LIGO 和 Advanced Virgo 的第二次观测运行期间搜索与伽马射线爆发相关的引力波信号

• DOI: 10.3847/1538-4357/ab4b48
• 发表时间: 2019
• 期刊: The Astrophysical Journal
• 作者: Abbott B

First targeted search for gravitational-wave bursts from core-collapse supernovae in data of first-generation laser interferometer detectors

首次在第一代激光干涉仪探测器的数据中定向搜索核心塌缩超新星的引力波爆发

• DOI: 10.1103/physrevd.94.102001
• 发表时间: 2016
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Abbott B

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.