LIGO detector characterization in the second and third observing runs

LIGO detector characterization in the second and third observing runs
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DOI:
10.1088/1361-6382/abfd85
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发表时间:
2021-01
影响因子:
3.5
通讯作者:
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
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
中科院分区:
物理与天体物理3区
文献类型:
--
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

文献摘要

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在第二次和第三次观测运行中,先进LIGO探测器的特性提高了仪器的灵敏度,允许更多的可探测引力波信号,并确认了所有观测到的引力波事件。在这项工作中,我们提出了用于表征LIGO探测器和管理公开数据集的方法,包括LIGO应变数据和数据质量产品。我们描述了这些数据集在LIGO-Virgo协作分析瞬态和持续源引力波中的重要作用,并详细介绍了这些数据集的来源,以支持更广泛的社区对LIGO数据的分析。最后,我们解释了预期的变化的作用,探测器的特性和目前的努力,以准备在未来的观测运行的高速率的引力波警报和事件。
The characterization of the Advanced LIGO detectors in the second and third observing runs has increased the sensitivity of the instruments, allowing for a higher number of detectable gravitational-wave signals, and provided confirmation of all observed gravitational-wave events. In this work, we present the methods used to characterize the LIGO detectors and curate the publicly available datasets, including the LIGO strain data and data quality products. We describe the essential role of these datasets in LIGO–Virgo Collaboration analyses of gravitational-waves from both transient and persistent sources and include details on the provenance of these datasets in order to support analyses of LIGO data by the broader community. Finally, we explain anticipated changes in the role of detector characterization and current efforts to prepare for the high rate of gravitational-wave alerts and events in future observing runs.