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/N000080/1
• 负责人: Edward Daw
• 金额: $ 5.38万
• 依托单位: University of Sheffield
• 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%2FN000080%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 confidently expected to detect gravitational waves and hence to 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 partnership within the project.Through the design and construction project "Advanced LIGO UK", 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 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 maximise 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 potential scientific output. This is true both in terms of their implementation within aLIGO, and later when it is planned that aLIGO will be further upgraded. 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 data access and science return for a relatively small investment in the aLIGO hardware. As set out in our Memorandum of Understanding (MOU) with LIGO, we have been given top-level project management roles, up to and including a seat on the project Oversight Committee for an STFC representative. It is essential that we maintain involvement at the highest level as set out in detail in this proposal. We therefore request continuation of travel support for observing duties, resources to allow us to provide technical support during detector commissioning and operations, and computer infrastructure support to provide a solid basis for exploitation of aLIGO science data within the UK. At the LIGO sites, 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. We request funding for the period 01/01/2016 to 31/12/2019.

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，以确保英国在该领域保持领先地位，并在项目中保持合作伙伴关系。通过设计和建设项目“Advanced LIGO UK”，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，主要是通过转移最初为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，最大限度地发挥英国的作用，因此，我们将继续积极参与用户社区组织LIGO科学合作组织（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aLIGO探测器设备和设施得到充分利用，以最大限度地提高潜在的科学产出。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。 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数据访问和科学回报，对aLIGO硬件进行相对较小的投资。正如我们与LIGO的谅解备忘录（MOU）所述，我们被赋予了顶级项目管理角色，包括STFC代表在项目监督委员会中的席位。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，我们要求继续提供观测任务的旅行支持，资源，使我们能够在探测器调试和运行期间提供技术支持，以及计算机基础设施支持，为在英国利用aLIGO科学数据提供坚实的基础。在LIGO站点，完成的探测器的第一次测试正在进行中，2014年11月，在第一次运行后仅仅几个月，LLO探测器就实现了对超过50兆秒差距（Mpc）距离的合并中子星的灵敏度-完全符合2015年开始的初始科学运行的目标。我们申请2016年1月1日至2019年12月31日期间的资金。

项目成果

Erratum: "First Search for Gravitational Waves from Known Pulsars with Advanced LIGO" (2017, ApJ, 839, 12)

勘误表：“首次利用先进的 LIGO 搜索已知脉冲星的引力波”(2017, ApJ, 839, 12)

• DOI: 10.3847/1538-4357/aa9aee
• 发表时间: 2017
• 期刊: The Astrophysical Journal
• 作者: Abbott B

First narrow-band search for continuous gravitational waves from known pulsars in advanced detector data

• DOI: 10.1103/physrevd.96.122006
• 发表时间: 2017-10
• 期刊: Physical Review D
• 影响因子: 5
• 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;B. Allen;G. Allen;A. Allocca;P. Altin;A. Amato;A. Ananyeva;S. Anderson;W. Anderson;S. Angelova;S. Antier;S. Appert;K. Arai;M. Araya;J. Areeda;N. Arnaud;K. Arun;S. Ascenzi;G. Ashton;M. Ast;S. Aston;P. Astone;D. V. Atallah;P. Aufmuth;C. Aulbert;K. AultONeal;C. Austin;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;K. Barkett;F. Barone;B. Barr;L. Barsotti;M. Barsuglia;D. Barta;J. Bartlett;I. Bartos;R. Bassiri;A. Basti;J. Batch;M. Bawaj;J. Bayley;M. Bazzan;B. B'ecsy;C. Beer;M. Bejger;I. Belahcene;A. Bell;B. Berger;G. Bergmann;J. Bero;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;S. Biscoveanu;A. Bisht;M. Bitossi;C. Biwer;M. Bizouard;J. Blackburn;J. Blackman;C. Blair;D. Blair;R. Blair;S. Bloemen;O. Bock;N. Bode;M. Boer;G. Bogaert;A. Bohé;F. Bondu;E. Bonilla;R. Bonnand;B. A. Boom;R. Bork;V. Boschi;S. Bose;K. Bossie;Y. Bouffanais;A. Bozzi;C. Bradaschia;P. Brady;M. Branchesi;J. Brau;T. Briant;A. Brillet;M. Brinkmann;V. Brisson;P. Brockill;J. Broida;A. Brooks;D. Brown;D. 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;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;P. Cerd'a-Dur'an;G. Cerretani;E. Cesarini;S. Chamberlin;M. Chan;S. Chao;P. Charlton;E. Chase;É. Chassande-Mottin;D. Chatterjee;B. Cheeseboro;H. Chen;X. Chen;Y. Chen;H.-P. Cheng;H. Chia;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;P. Clearwater;F. Cleva;C. Cocchieri;E. Coccia;P. Cohadon;D. Cohen;A. Colla;C. Collette;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;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;G. D'alya;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;J. Degallaix;M. D. Laurentis;S. Del'eglise;W. D. Pozzo;N. Demos;T. Denker;T. Dent;R. Pietri;V. Dergachev;R. Rosa;R. Derosa;C. D. Rossi;R. DeSalvo;O. D. Varona;J. Devenson;S. Dhurandhar;M. D'iaz;L. Fiore;M. Giovanni;T. D. Girolamo;A. 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;C. Dreissigacker;J. Driggers;Z. Du;M. Ducrot;P. Dupej;S. Dwyer;T. Edo;M. Edwards;A. Effler;H. Eggenstein;P. Ehrens;J. Eichholz;S. Eikenberry;R. Eisenstein;R. Essick;D. Estevez;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;C. Fee;H. Fehrmann;J. Feicht;M. Fejer;Á. Fernández-Galiana;I. Ferrante;E. Ferreira;F. Ferrini;F. Fidecaro;D. Finstad;I. Fiori;D. Fiorucci;M. Fishbach;R. Fisher;M. Fitz-Axen;R. Flaminio;M. Fletcher;H. Fong;J. Font;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;B. Gadre;S. Gaebel;J. Gair;L. Gammaitoni;M. Ganija;S. Gaonkar;C. García-Quirós;F. Garufi;B. Gateley;S. Gaudio;G. Gaur;V. Gayathri;N. Gehrels;G. Gemme;E. Génin;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;B. Goncharov;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;E. Gretarsson;P. Groot;H. Grote;S. Grunewald;P. Gruning;G. Guidi;X. Guo;A. Gupta;M. Gupta;K. Gushwa;E. Gustafson;R. Gustafson;O. Halim;B. Hall;E. Hall;E. Hamilton;G. Hammond;M. Haney;M. Hanke;J. Hanks;C. Hanna;M. Hannam;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;A. Heptonstall;M. Heurs;S. Hild;T. Hinderer;W. Ho;D. Hoak;D. Hofman;K. Holt;D. Holz;P. Hopkins;C. Horst;J. Hough;E. Houston;E. Howell;A. Hreibi;Y. Hu;E. Huerta;D. Huet;B. Hughey;S. Husa;S. Huttner;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;N. Indik;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;B. Kamai;S. Kandhasamy;G. Kang;J. Kanner;S. Kapadia;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;K. Kim;W. Kim;W. Kim;Y. Kim;S. Kimbrell;E. King;P. King;M. Kinley-Hanlon;R. Kirchhoff;J. Kissel;L. Kleybolte;S. Klimenko;T. Knowles;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;S. Linker;T. Littenberg;J. Liu;R. K. Lo;N. Lockerbie;L. London;J. Lord;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;J. Lough;G. Lovelace;H. Luck;D. Lumaca;A. Lundgren;R. Lynch;Y. Ma;R. Macas;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;A. Markowitz;E. Maros;A. Marquina;F. Martelli;L. Martellini;I. Martin;R. Martin;D. Martynov;K. Mason;E. Massera;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;F. Matichard;L. Matone;N. Mavalvala;N. Mazumder;R. McCarthy-;D. McClelland;S. Mccormick;L. McCuller;S. Mcguire;G. Mcintyre;J. McIver;D. McManus;L. McNeill;T. McRae;S. McWilliams;D. Meacher;G. Meadors;M. Mehmet;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;H. Miao;C. Michel;H. Middleton;E. Mikhailov;L. Milano;A. Miller;B. Miller;J. Miller;M. Millhouse;M. Milovich-Goff;O. Minazzoli;Y. Minenkov;J. Ming;C. Mishra;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;D. Moffa;A. Moggi;K. Mogushi;M. Mohan;S. Mohapatra;M. Montani;C. Moore;D. Moraru;G. Moreno;S. Morriss;B. Mours;C. Mow-Lowry;G. Mueller;A. Muir;A. Mukherjee;D. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;M. Muratore;P. Murray;K. Napier;I. Nardecchia;L. Naticchioni;R. Nayak;J. Neilson;G. Nelemans;T. Nelson;M. Nery;A. Neunzert;L. Nevin;J. Newport;G. Newton;K. Ng;T. Nguyen;D. Nichols;A. Nielsen;S. Nissanke;A. Nitz;A. Noack;F. Nocera;D. Nolting;C. North;L. Nuttall;J. Oberling;G. O’Dea;G. Ogin;J. Oh;S. Oh;F. Ohme;M. A. Okada;M. Oliver;P. Oppermann;R. Oram;B. O'reilly;R. Ormiston;L. F. Ortega;R. O’Shaughnessy;S. Ossokine;D. Ottaway;H. Overmier;B. Owen;A. Pace;J. Page;M. Page;A. Pai;S. Pai;J. 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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;G. Rutins;K. Ryan;S. Sachdev;T. Sadecki;L. Sadeghian;M. Sakellariadou;L. Salconi;M. Saleem;F. Salemi;A. Samajdar;L. Sammut;L. Sampson;E. Sanchez;L. Sanchez;N. Sanchis-Gual;V. Sandberg;J. Sanders;B. Sassolas;B. Sathyaprakash;P. Saulson;O. Sauter;R. Savage;A. Sawadsky;P. Schale;M. Scheel;J. Scheuer;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. Shah;M. Shahriar;M. Shaner;L. Shao;B. Shapiro;P. Shawhan;A. Sheperd;D. Shoemaker;D. Shoemaker;K. Siellez;X. Siemens;M. Sieniawska;D. Sigg;A. Silva;L. Singer;A. Singh;A. Singhal;A. Sintes;B. Slagmolen;B. Smith;J. R. Smith;R. Smith;S. Somala;E. Son;J. Sonnenberg;B. Sorazu;F. Sorrentino;T. Souradeep;A. Spencer;A. Srivastava;K. Staats;A. Staley;M. 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THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914

• DOI: 10.3847/2041-8205/833/1/l1
• 发表时间: 2016-02
• 期刊: The Astrophysical Journal Letters
• 作者: The Ligo Scientific Collaboration;T. Abbott;R. Abbott;T. Abbott;M. Abernathy;F. Acernese;K. Ackley

SUPPLEMENT: "THE RATE OF BINARY BLACK HOLE MERGERS INFERRED FROM ADVANCED LIGO OBSERVATIONS SURROUNDING GW150914" (2016, ApJL, 833, L1)

• DOI: 10.3847/0067-0049/227/2/14
• 发表时间: 2016-12-01
• 期刊: ASTROPHYSICAL JOURNAL SUPPLEMENT SERIES
• 影响因子: 8.7
• 作者: Abbott, B. P.;Abbott, R.;Zuraw, S. E.
• 通讯作者: Zuraw, S. E.

Search of the Orion spur for continuous gravitational waves using a loosely coherent algorithm on data from LIGO interferometers

使用松散相干算法对来自 LIGO 干涉仪的数据搜索猎户座支线的连续引力波

• DOI: 10.1103/physrevd.93.042006
• 发表时间: 2016
• 期刊: Physical Review D
• 影响因子: 5
• 作者: Aasi J