Gravitational Wave Astrophysics with LIGO: The Oregon Experimental Relativity Group

LIGO 引力波天体物理学：俄勒冈实验相对论小组

• 批准号: 1912604
• 负责人: Raymond Frey
• 金额: $ 90万
• 依托单位: University of Oregon Eugene
• 依托单位国家: 美国
• 项目类别: Standard Grant
• 财政年份: 2019
• 资助国家: 美国
• 起止时间: 2019-08-01 至 2022-07-31
• 项目状态: 已结题
• 来源: https://www.nsf.gov/awardsearch/showAward?AWD_ID=1912604&HistoricalAwards=false
• 关键词: Gravitational; Wave; Astrophysics; LIGO; Oregon

This award supports research in gravitational wave detector commissioning and characterization, as well as data analysis and it addresses the priority areas of NSF's "Windows on the Universe" Big Idea. A Search for Gravitational Radiation at LIGO Oregon Experimental Relativity Group. With the discovery of gravitational waves in September 2015 via the observation a merger of black holes, and the birth of multi-messenger astrophysics with gravitational waves in 2017 via the observation of a merger of neutron stars, the LIGO collaboration has become a key player in 21st century science in the areas of fundamental physics, astronomy, astrophysics, and cosmology. Because the LIGO detectors measure such tiny perturbations in spacetime -- distances 10,000 smaller than the diameter of a proton -- it is extremely sensitive to environmental disturbances, such as ground motion or background magnetic fields. During the period of this award, the LIGO instruments will be even more sensitive, meaning that the rate of detections of known astrophysical sources will be increased, and new, previously unobserved sources may appear. With this award, the group will develop the expertise and toolkits needed to meet the data quality and analysis challenges provided by the enhanced LIGO instruments. The team's graduate students will continue to play a critical role in these developments. The team will give public presentations on these exciting developments. This includes the organization of a yearly workshop for Oregon high school science teachers, so that they can convey the latest findings to their students.The team will further develop the ability to characterize the coupling of relevant environmental disturbances to gravitational-wave data. The greater sensitivity of the detectors, along with the associated higher detection rates make these developments imperative. The team has developed software to determine potential environmental contamination levels to gravitational wave candidates in low latency. This is provided in the data quality reports made available for immediate evaluation for the O3 open public alerts. These tools are fairly rudimentary and further development will be needed to achieve the goal of a fully automatized process which is reliable and accurate. Continued improvement of the instrumentation and delivery of environmental injections will be needed to keep pace with the improved sensitivity of the LIGO interferometers. Graduate students will undertake environmental injection studies and associated data analyses, as well as gravitational wave astrophysics projects, covering the topics of GRBs, magnetar flares, and supernovae. While refinements will be needed for these studies to keep pace with the improved LIGO sensitivities and better astrophysical understanding of the sources, in some cases new techniques will be needed. One example for this is for the so-called sub-threshold GRBs. The need for this was spectacularly illustrated with GRB/GW170817.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.

该奖项支持引力波探测器调试和表征以及数据分析方面的研究，并解决了NSF“宇宙窗口”大创意的优先领域。在LIGO俄勒冈州实验相对论组寻找引力辐射。随着2015年9月通过观察黑洞合并发现引力波，以及2017年通过观察中子星合并产生的引力波多信使天体物理学的诞生，LIGO合作已成为基础物理学，天文学，天体物理学和宇宙学领域21世纪科学的关键参与者。由于LIGO探测器测量的是时空中如此微小的扰动--距离比质子直径小10,000倍--它对环境扰动（如地面运动或背景磁场）极其敏感。在此期间，LIGO仪器将更加灵敏，这意味着对已知天体物理源的探测率将提高，并且可能会出现新的，以前未观测到的源。凭借该奖项，该团队将开发所需的专业知识和工具包，以满足增强型LIGO仪器提供的数据质量和分析挑战。该团队的研究生将继续在这些发展中发挥关键作用。该团队将对这些令人兴奋的发展进行公开演示。这包括每年为俄勒冈州的高中科学教师组织一次研讨会，使他们能够向学生传达最新的发现，该小组将进一步发展描述相关环境干扰与引力波数据耦合的能力。探测器更高的灵敏度，沿着伴随着更高的探测率，使得这些发展势在必行。该团队已经开发了软件来确定低延迟引力波候选者的潜在环境污染水平。这是在数据质量报告中提供的，可用于O3开放公共警报的即时评估。这些工具相当初级，需要进一步开发，以实现可靠和准确的完全自动化过程的目标。为了跟上LIGO干涉仪灵敏度的提高，需要继续改进仪器和环境注入的提供。研究生将进行环境注入研究和相关的数据分析，以及引力波天体物理学项目，涵盖GRB，磁星耀斑和超新星的主题。虽然这些研究需要改进，以跟上LIGO灵敏度的提高和对源的更好天体物理理解，但在某些情况下，将需要新的技术。一个例子是所谓的亚阈值伽玛暴。GRB/GW 170817清楚地说明了这一点的必要性。该奖项反映了NSF的法定使命，并通过使用基金会的知识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

Diving below the Spin-down Limit: Constraints on Gravitational Waves from the Energetic Young Pulsar PSR J0537-6910

• DOI: 10.3847/2041-8213/abffcd
• 发表时间: 2020-12
• 期刊: The Astrophysical Journal Letters
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;T. Abbott;S. Abraham;F. Acernese;K. Ackley;A. Adams;C. Adams;R. Adhikari;V. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;T. Akutsu;K. M. Aleman;G. Allen;A. Allocca;P. Altin;A. Amato;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;M. Ando;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;S. Aston;P. Astone;F. Aubin;P. Aufmuth;K. AultONeal;C. Austin;S. Babak;F. Badaracco;M. Bader;S. Bae;Y. Bae;A. Baer;S. Bagnasco;Y. Bai;L. Baiotti;J. Baird;R. Bajpai;M. Ball;G. Ballardin;S. Ballmer;M. Bals;A. Balsamo;G. Baltus;S. Banagiri;D. Bankar;R. Bankar;J. Barayoga;C. Barbieri;B. Barish;D. Barker;P. Barneo;S. Barnum;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;M. Benjamin;T. Bennett;J. Bentley;M. BenYaala;F. Bergamin;B. Berger;S. Bernuzzi;D. Bersanetti;A. Bertolini;J. Betzwieser;R. Bhandare;A. Bhandari;D. Bhattacharjee;S. Bhaumik;J. Bidler;I. Bilenko;G. Billingsley;R. Birney;O. Birnholtz;S. Biscans;M. Bischi;S. Biscoveanu;A. Bisht;B. Biswas;M. Bitossi;M. Bizouard;J. Blackburn;J. Blackman;C. Blair;D. Blair;R. Blair;F. Bobba;N. Bode;M. Boer;G. Bogaert;M. Boldrini;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;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;A. Buikema;T. Bulik;H. Bulten;A. Buonanno;R. Buscicchio;D. Buskulic;L. Cadonati;M. Caesar;G. Cagnoli;C. Cahillane;H. Cain;J. C. Bustillo;J. Callaghan;T. Callister;E. 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Merzougui;S. Meshkov;C. Messenger;C. Messick;P. Meyers;F. Meylahn;A. Mhaske;A. Miani;H. Miao;I. Michaloliakos;C. Michel;Y. Michimura;H. Middleton;L. Milano;A. Miller;M. Millhouse;J. Mills;E. Milotti;M. Milovich-Goff;O. Minazzoli;Y. Minenkov;N. Mio;L. Mir;A. Mishkin;C. Mishra;T. Mishra;T. Mistry;S. Mitra;V. Mitrofanov;G. Mitselmakher;R. Mittleman;O. Miyakawa;A. Miyamoto;Y. Miyazaki;K. Miyo;S. Miyoki;G. Mo;K. Mogushi;S. Mohapatra;S. Mohite;I. Molina;M. Molina-Ruiz;M. Mondin;M. Montani;C. Moore;D. Moraru;F. Morawski;A. More;C. Moreno;G. Moreno;Y. Mori;S. Morisaki;Y. Moriwaki;B. Mours;C. Mow-Lowry;S. Mozzon;F. Muciaccia;A. Mukherjee;D. Mukherjee;S. Mukherjee;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Nadji;K. Nagano;S. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;R. Nakashima;Y. Nakayama;I. Nardecchia;T. Narikawa;L. Naticchioni;B. Nayak;R. Nayak;R. Negishi;B. Neil;J. Neilson;G. Nelemans;T. Nelson;M. Nery;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;W. Ni;S. Nichols;A. Nishizawa;S. Nissanke;F. Nocera;M. Noh;M. Norman;C. North;S. Nozaki;L. Nuttall;J. Oberling;B. O'Brien;Y. Obuchi;J. O'Dell;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;K. Pan;P. K. Panda;H. Pang;P. T. Pang;C. Pankow;F. Pannarale;B. Pant;F. Paoletti;A. Paoli;A. Paolone;A. Parisi;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;B. Patricelli;E. Payne;T. Pechsiri;M. Pedraza;M. Pegoraro;A. Pele;F. Arellano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. P'erigois;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;F. Pilo;L. Pinard;I. Pinto;B. Piotrzkowski;K. Piotrzkowski;M. Pirello;M. Pitkin;E. Placidi;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;D. T. Pong;S. Ponrathnam;P. Popolizio;E. Porter;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;T. Prestegard;M. Principe;G. Prodi;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;P. Puppo;M. Purrer;H. Qi;V. Quetschke;P. J. Quinonez;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;B. Ratto;V. Raymond;N. Raza;M. Razzano;J. Read;L. A. Rees;T. Regimbau;L. Rei;S. Reid;D. Reitze;P. Relton;P. Rettegno;F. Ricci;C. J. Richardson;J. Richardson;L. Richardson;P. Ricker;G. Riemenschneider;K. Riles;M. Rizzo;N. Robertson;R. Robie;F. Robinet;A. Rocchi;J. Rocha;S. Rodriguez;R. D. Rodriguez-Soto;L. Rolland;J. Rollins;V. Roma;M. Romanelli;R. Romano;C. Romel;A. Romero;I. Romero-Shaw;J. Romie;C. Rose;D. Rosi'nska;S. Rosofsky;M. Ross;S. Rowan;S. Rowlinson;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;J. H. Sánchez;L. Sanchez;N. Sanchis-Gual;J. Sanders;A. Sanuy;T. R. Saravanan;N. Sarin;B. Sassolas;H. Satari;S. Sato;T. Sato;O. Sauter;R. Savage;V. Savant;T. Sawada;D. Sawant;H. Sawant;S. Sayah;D. Schaetzl;M. Scheel;J. Scheuer;A. Schindler-Tyka;P. Schmidt;R. Schnabel;M. Schneewind;R. Schofield;A. Schonbeck;B. Schulte;B. Schutz;E. Schwartz;J. Scott;S. Scott;M. Seglar-Arroyo;E. Seidel;T. Sekiguchi;Y. Sekiguchi;D. Sellers;A. Sengupta;N. Sennett;D. Sentenac;E. Seo;V. Sequino;Y. Setyawati;T. Shaffer;M. Shahriar;B. Shams;L. Shao;S. Sharifi;A. Sharma;P. Sharma;P. Shawhan;N. Shcheblanov;H. Shen;S. Shibagaki;M. Shikauchi;R. Shimizu;T. Shimoda;K. Shimode;R. Shink;H. Shinkai;T. Shishido;A. Shoda;D. Shoemaker;D. Shoemaker;K. Shukla;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;S. Somala;K. Somiya;E. Son;K. Soni;S. Soni;B. Sorazu;V. Sordini;F. Sorrentino;N. Sorrentino;H. Sotani;R. Soulard;T. Souradeep;E. Sowell;V. Spagnuolo;A. Spencer;M. Spera;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;J. Sudbeck;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;H. Tanaka;Kazuyuki Tanaka;Kenta Tanaka;Taiki Tanaka;Takahiro Tanaka;A. Tanasijczuk;S. Tanioka;D. Tanner;D. Tao;A. Tapia;E. Martín;J. Tasson;S. Telada;R. Tenorio;L. Terkowski;M. Test;M. Thirugnanasambandam;M. Thomas;P. Thomas;J. Thompson;S. R. Thondapu;K. Thorne;E. Thrane;S. Tiwari;S. Tiwari;V. Tiwari;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. 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;M. Turconi;D. Tuyenbayev;A. Ubhi;N. Uchikata;T. Uchiyama;R. Udall;A. Ueda;T. Uehara;K. Ueno;G. Ueshima;D. Ugolini;C. Unnikrishnan;F. Uraguchi;A. Urban;T. Ushiba;S. A. Usman;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;M. Putten;M. Vardaro;A. Vargas;V. Varma;M. Vas'uth;A. Vecchio;G. Vedovato;J. Veitch;P. Veitch;K. Venkateswara;J. Venneberg;Gautam Venugopalan;D. Verkindt;Y. Verma;D. Veske;F. Vetrano;A. Vicer'e;A. Viets;V. Villa-Ortega;J. Vinet;S. Vitale;T. Vo;H. Vocca;E. V. Reis;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;L. Wei;M. Weinert;A. Weinstein;R. Weiss;C. Weller;F. Wellmann;L. Wen;P. Wessels;J. Westhouse;K. Wette;J. Whelan;D. White;B. Whiting;C. Whittle;D. Wilken;D. Williams;M. J. Williams;A. Williamson;J. Willis;B. Willke;D. Wilson;W. Winkler;C. Wipf;T. Włodarczyk;G. Woan;J. Woehler;J. Wofford;I. C. Wong;J. Wrangel;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;Yang Yang-Yang;Yi Yang;Z. Yang;M. Yap;D. Yeeles;Anjali B. Yelikar;M. Ying;K. Yokogawa;J. Yokoyama;T. Yokozawa;A. Yoon;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;R. Zhang;T. Zhang;C. Zhao;G. Zhao;Yue Zhao;Yuhang Zhao;Z. Zhou;X. Zhu;Z. Zhu;M. Zucker;J. Zweizig;D. Antonopoulou;Z. Arzoumanian;T. Enoto;C. Espinoza;S. Guillot

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

Search for anisotropic gravitational-wave backgrounds using data from Advanced LIGO and Advanced Virgo窶冱 first three observing runs

使用 Advanced LIGO 和 Advanced Virgo 前三次观测运行的数据搜索各向异性引力波背景

• DOI: 10.1103/physrevd.104.022005
• 发表时间: 2021
• 期刊: Physical Review D
• 影响因子: 5
• 作者: R. Abbott et al.

Environmental noise in advanced LIGO detectors

• DOI: 10.1088/1361-6382/ac011a
• 发表时间: 2021-07-22
• 期刊: CLASSICAL AND QUANTUM GRAVITY
• 影响因子: 3.5
• 作者: Nguyen, P.;Schofield, R. M. S.;Zweizig, J.
• 通讯作者: Zweizig, J.

Tests of General Relativity with Binary Black Holes from the second LIGO-Virgo Gravitational-Wave Transient Catalog

• DOI: 10.1103/physrevd.103.122002
• 发表时间: 2020-10
• 作者: The Ligo Scientific Collaboration;T. Abbott;T. Abbott;S. Abraham;F. Acernese;K. Ackley;A. Adams