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，在该提案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。在本提案中，我们要求对必要的基础设施和差旅费用提供支持，以确保英国在该领域保持领先地位以及在项目内的合作伙伴关系。通过“Advanced LIGO UK”的设计和建设项目，英国成功地主要通过转让最初为 GEO600 开发的二氧化硅悬浮技术，为美国 aLIGO 引力波探测器的主要方面做出了独特和根本性的贡献。由此产生的悬浮液对于 aLIGO 达到其灵敏度目标绝对至关重要。在第一阶段的运营中，英国提供的设备已安装并集成到两个 aLIGO 探测器中。其直接结果是，英国研究小组能够利用这些探测器及其观测伙伴在当前十年中产生的丰富科学数据。我们建议通过提供充分参与 aLIGO 探测器操作所需的支持和基础设施来最大化英国的地位，从而保持用户社区团体 LIGO 科学合作组织 (LSC) 的积极合作伙伴，通过该组织数据权赚取并分配。 同样重要的是，需要确保英国交付的 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 内的实施，还是以后计划进一步升级 aLIGO 时，都是如此。 LSC 的英国会员数量相当可观——目前按作者划分占 12%。 ALUK 项目和 GEO600 的数据交换使我们能够以相对较小的 aLIGO 硬件投资来利用数据访问和科学回报。根据我们与 LIGO 的谅解备忘录 (MOU) 中的规定，我们被授予顶级项目管理职位，最高级别包括 STFC 代表的项目监督委员会席位。正如本提案中详细规定的那样，我们必须保持最高层的参与。因此，我们要求继续提供观测任务的差旅支持、使我们能够在探测器调试和操作期间提供技术支持的资源以及计算机基础设施支持，以便为在英国境内利用 aLIGO 科学数据提供坚实的基础。在 LIGO 站点，对已完成探测器的首次测试正在进行中，2014 年 11 月，首次运行后仅几个月，LLO 探测器就实现了对距离超过 50 兆秒差距 (Mpc) 的聚结双中子星的灵敏度 - 完全达到了目标初始科学运行将于 2015 年开始。我们请求在 2016 年 1 月 1 日至 2019 年 12 月 31 日期间提供资金。

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. R. Palamos;O. Palashov;C. Palomba;A. Pal-Singh;H. Pan;H. Pan;B. Pang;P. T. Pang;C. Pankow;F. Pannarale;B. Pant;F. Paoletti;A. Paoli;M. Papa;A. Parida;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patil;B. Patricelli;B. Pearlstone;M. Pedraza;R. Pedurand;L. Pekowsky;A. Pele;S. Penn;C. Perez;A. Perreca;L. Perri;H. Pfeiffer;M. Phelps;O. Piccinni;M. Pichot;F. Piergiovanni;V. Pierro;G. Pillant;L. Pinard;I. Pinto;M. Pirello;M. Pitkin;M. Poe;R. Poggiani;P. Popolizio;E. Porter;A. Post;J. Powell;J. Prasad;J. Pratt;G. Pratten;V. Predoi;T. Prestegard;M. Prijatelj;M. Principe;S. Privitera;G. Prodi;L. Prokhorov;O. Puncken;M. Punturo;P. Puppo;M. Purrer;H. Qi;V. Quetschke;E. Quintero;R. Quitzow-James;F. Raab;D. Rabeling;H. Radkins;P. Raffai;S. Raja;C. Rajan;B. Rajbhandari;M. Rakhmanov;K. Ramirez;A. Ramos-Buades;P. Rapagnani;V. Raymond;M. Razzano;J. Read;T. Regimbau;L. Rei;S. Reid;D. Reitze;W. Ren;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;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. Steinke;J. Steinlechner;S. Steinlechner;D. Steinmeyer;S. Stevenson;R. Stone;D. Stops;K. Strain;G. Stratta;S. Strigin;A. Strunk;R. Sturani;A. Stuver;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;J. A. Taylor;R. Taylor;S. Tewari;T. Theeg;F. Thies;E. Thomas;M. Thomas;P. Thomas;K. Thorne;E. Thrane;S. Tiwari;V. Tiwari;K. Tokmakov;K. Toland;M. Tonelli;Z. Tornasi;A. Torres-Forn'e;C. Torrie;D. Toyra;F. Travasso;G. Traylor;J. Trinastic;M. Tringali;L. Trozzo;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;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;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;J. Warner;M. Was;J. Watchi;B. Weaver;L.-W. Wei;M. Weinert;A. Weinstein;R. Weiss;L. Wen;E. Wessel;P. Wessels;J. Westerweck;T. Westphal;K. Wette;J. Whelan;B. Whiting;C. Whittle;D. Wilken;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;D. Wysocki;S. Xiao;H. Yamamoto;C. Yancey;L. Yang;M. Yap;M. Yazback;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;S. Zhu;X. Zhu;M. Zucker;J. Zweizig

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.

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

All-sky search for long-duration gravitational wave transients in the first Advanced LIGO observing run

首次高级 LIGO 观测运行中对长持续时间引力波瞬变的全天空搜索

• DOI: 10.1088/1361-6382/aaab76
• 发表时间: 2018
• 期刊: Classical and Quantum Gravity
• 影响因子: 3.5
• 作者: Abbott B