Warwick Astronomy & Astrophysics Consolidated Grant 2023-2026

沃里克天文学

• 批准号: ST/X001121/1
• 负责人: Danny Steeghs
• 金额: $ 309.49万
• 依托单位: University of Warwick
• 依托单位国家: 英国
• 项目类别: Research Grant
• 财政年份: 2023
• 资助国家: 英国
• 起止时间: 2023 至 无数据
• 项目状态: 未结题
• 来源: https://gtr.ukri.org/projects?ref=ST%2FX001121%2F1
• 关键词: Warwick; Astronomy; Astrophysics; Consolidated; Grant

How do stars, planets and galaxies form? How do they evolve, how do they die? The Astronomy and Astrophysics group at the University of Warwick studies questions such as these through observations on telescopes, both large and small, and through physics-driven computational modelling. The use of optical telescopes in astronomy dates back over 400 years to Galileo, but we are now in a new Galilean era of discovery with the first detection of gravitational waves (GWs) only made in 2015. GWs provide a completely different view of the universe, delving to the heart of the most extreme events known as unimaginably dense stars spiral together, and, in their last moments before merging, rival the power output of the rest of the entire observable universe. GW telescopes can "see" almost everywhere at once, but have the equivalent of very blurred vision. To pinpoint sources, we need to see them electromagnetically (EM), i.e. with optical, radio and x-ray telescopes, but even that is difficult because you have to know where to look first. At Warwick we are working on a telescope called GOTO to do just this. From sites in Europe and Australia, GOTO is designed for breadth of vision and speed, to chase the universe's fastest and most violent events within minutes of their detection. Many less powerful, but longer lasting objects emit GWs much closer to Earth within our own galaxy, the Milky Way. We are starting to find systems from EM observations that will also be detectable as GW sources from space. These are exotic sources: one consists of two stars, each the size of the Earth but 100,000 times more massive, that circle each other in a little over five minutes. We will apply specialist high-speed cameras to their study, mounted on large optical telescopes, to probe how they evolve and important step in understanding how many of them there are, and how they came to be. Gravitational waves have given us new eyes on the universe, but new instruments and techniques do almost the same thing. In 1995 the first exoplanet was found through a particularly sensitive application of an old tool of astronomy called spectroscopy. Since then thousands of planets have been found in a bewildering variety of systems, many very different from our Solar System. At Warwick we have long pursued the discovery of exoplanets using both telescopes on Earth and in space, and will do so in this grant in order to understand processes that can destroy or erode planets when they are close to their host stars. Many known exoplanets are close to their host stars, but that is in part due to how we find them, so another strand of our research aims to push planetary detection to wider orbits, closer to those of our Solar system. Warwick has a strong interest in a new ESA-led space mission called PLATO which will provide a dramatic boost to this work. PLATO has a large field of view to allow it to pick up planets orbiting the brightest stars. These are key targets as they are close by, but above all they allow even more challenging application of spectroscopy, enough to allow us to probe the very composition of the planetary atmospheres. Earth and the other planets of the Solar system formed from a disk of material around the young Sun that lives on as the planets themselves but also "debris" in the form of comets, asteroids and dust. We aim to find evidence for similar structures around other stars, in particular from their dust as it scatters starlight. Such material can survive the several billion year lifetime of the star until just a hot dense remnant called a white dwarf remains. The formation of a white dwarf should "deep clean" the environment close to the star, and yet remarkably we have found many example of the planetary debris, and within our research we aim to find out how this can be. There are many other white dwarfs left from stellar evolution which we will map using a new generation of fibre-fed spectrographs that capture objects, 1000 at a time.

恒星、行星和星系是如何形成的？它们是如何进化的，又是如何死亡的？沃里克大学的天文学和天体物理学小组通过对大型和小型望远镜的观测以及通过物理驱动的计算建模来研究这些问题。光学望远镜在天文学中的使用可以追溯到400多年前的伽利略，但我们现在正处于一个新的伽利略发现时代，2015年才首次探测到引力波。GWs提供了一个完全不同的宇宙观，深入研究了最极端事件的核心，这些事件被称为不可阻挡的密集恒星螺旋在一起，并且在合并前的最后时刻，与整个可观测宇宙的其余部分的功率输出相媲美。GW望远镜几乎可以同时“看到”任何地方，但相当于非常模糊的视觉。为了确定来源，我们需要用电磁（EM），即光学，无线电和X射线望远镜来观察它们，但即使这样也很困难，因为你必须知道首先从哪里看。在沃里克，我们正在研制一种名为后藤的望远镜来做这件事。从欧洲和澳大利亚的网站，后藤是专为广度的视野和速度，追逐宇宙中最快和最激烈的事件在几分钟内检测。在我们自己的星系银河系中，许多不那么强大但持续时间更长的物体在离地球更近的地方发出GW。我们开始从EM观测中发现系统，这些系统也将被检测为来自太空的GW源。这些是外来的来源：其中一个由两颗恒星组成，每颗恒星的大小都是地球的10万倍，它们在5分钟多一点的时间内相互环绕。我们将应用专业的高速相机进行研究，安装在大型光学望远镜上，以探索它们如何进化，以及了解它们有多少以及它们是如何形成的重要一步。引力波让我们对宇宙有了新的认识，但新的仪器和技术也能做同样的事情。1995年，第一颗系外行星通过一种被称为光谱学的古老天文学工具的特别敏感的应用被发现。从那时起，在令人眼花缭乱的各种系统中发现了数千颗行星，其中许多与我们的太阳系非常不同。在沃里克，我们长期以来一直在使用地球和太空望远镜发现系外行星，并将在本补助金中这样做，以了解当行星接近其宿主恒星时可能破坏或侵蚀行星的过程。许多已知的系外行星靠近它们的宿主恒星，但这在一定程度上是由于我们发现它们的方式，因此我们的另一项研究旨在将行星探测推向更广泛的轨道，更接近我们太阳系的轨道。沃里克对欧空局领导的名为PLATO的新太空使命有浓厚的兴趣，该使命将为这项工作提供巨大的推动力。PLATO有一个大的视野，使其能够拾取围绕最亮恒星运行的行星。这些都是关键的目标，因为它们离得很近，但最重要的是，它们允许光谱学更具挑战性的应用，足以让我们探测行星大气的组成。地球和太阳系的其他行星是由年轻的太阳周围的物质盘形成的，这些物质盘以行星本身的形式存在，但也以彗星、小行星和尘埃的形式存在。我们的目标是找到其他恒星周围类似结构的证据，特别是从它们的尘埃中散射星光。这种物质可以在星星的数十亿年寿命中存活下来，直到只剩下一个被称为白色矮星的热的致密残余物。白色矮星的形成应该“深度清洁”靠近星星的环境，然而值得注意的是，我们已经发现了许多行星碎片的例子，在我们的研究中，我们的目标是找出这是如何实现的。还有许多其他的白色矮星从恒星演化中遗留下来，我们将使用新一代的光纤光谱仪来绘制它们的地图，这种光谱仪可以一次捕获1000个物体。

项目成果

Constraints on the Cosmic Expansion History from GWTC–3

• DOI: 10.3847/1538-4357/ac74bb
• 发表时间: 2021-11
• 期刊: The Astrophysical Journal
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;H. Abe;F. Acernese;K. Ackley

GWTC-2.1: Deep extended catalog of compact binary coalescences observed by LIGO and Virgo during the first half of the third observing run

• DOI: 10.1103/physrevd.109.022001
• 发表时间: 2021-08
• 期刊: Physical Review D
• 影响因子: 5
• 作者: The Ligo Scientific Collaboration;T. Abbott;T. Abbott;F. Acernese;K. Ackley;C. Adams;N. Adhikari

Early Release Science of the exoplanet WASP-39b with JWST NIRCam.

• DOI: 10.1038/s41586-022-05590-4
• 发表时间: 2023-03
• 期刊: NATURE
• 影响因子: 64.8
• 作者: Ahrer, Eva-Maria;Stevenson, Kevin B.;Mansfield, Megan;Moran, Sarah E.;Brande, Jonathan;Morello, Giuseppe;Murray, Catriona A.;Nikolov, Nikolay K.;de la Roche, Dominique J. M. Petit Dit;Schlawin, Everett;Wheatley, Peter J.;Zieba, Sebastian;Batalha, Natasha E.;Damiano, Mario;Goyal, Jayesh M.;Lendl, Monika;Lothringer, Joshua D.;Mukherjee, Sagnick;Ohno, Kazumasa;Batalha, Natalie M.;Battley, Matthew P.;Bean, Jacob L.;Beatty, Thomas G.;Benneke, Bjorn;Berta-Thompson, Zachory K.;Carter, Aarynn L.;Cubillos, Patricio E.;Daylan, Tansu;Espinoza, Nestor;Gao, Peter;Gibson, Neale P.;Gill, Samuel;Harrington, Joseph;Hu, Renyu;Kreidberg, Laura;Lewis, Nikole K.;Line, Michael R.;Lopez-Morales, Mercedes;Parmentier, Vivien;Powell, Diana K.;Sing, David K.;Tsai, Shang-Min;Wakeford, Hannah R.;Welbanks, Luis;Alam, Munazza K.;Alderson, Lili;Allen, Natalie H.;Anderson, David R.;Barstow, Joanna K.;Bayliss, Daniel;Bell, Taylor J.;Blecic, Jasmina;Bryant, Edward M.;Burleigh, Matthew R.;Carone, Ludmila;Casewell, S. L.;Changeat, Quentin;Chubb, Katy L.;Crossfield, Ian J. M.;Crouzet, Nicolas;Decin, Leen;Desert, Jean-Michel;Feinstein, Adina D.;Flagg, Laura;Fortney, Jonathan J.;Gizis, John E.;Heng, Kevin;Iro, Nicolas;Kempton, Eliza M. -R.;Kendrew, Sarah;Kirk, James;Knutson, Heather A.;Komacek, Thaddeus D.;Lagage, Pierre-Olivier;Leconte, Jeremy;Lustig-Yaeger, Jacob;MacDonald, Ryan J.;Mancini, Luigi;May, E. M.;Mayne, N. J.;Miguel, Yamila;Mikal-Evans, Thomas;Molaverdikhani, Karan;Palle, Enric;Piaulet, Caroline;Rackham, Benjamin V.;Redfield, Seth;Rogers, Laura K.;Roy, Pierre-Alexis;Rustamkulov, Zafar;Shkolnik, Evgenya L.;Sotzen, Kristin S.;Taylor, Jake;Tremblin, P.;Tucker, Gregory S.;Turner, Jake D.;de Val-Borro, Miguel;Venot, Olivia;Zhang, Xi
• 通讯作者: Zhang, Xi

GWTC-3: Compact Binary Coalescences Observed by LIGO and Virgo during the Second Part of the Third Observing Run

• DOI: 10.1103/physrevx.13.041039
• 发表时间: 2021-11
• 期刊: Physical Review X
• 影响因子: 12.5
• 作者: The Ligo Scientific Collaboration;The Virgo Collaboration;T. Abbott;T. Abbott;F. Acernese;K. Ackley;C. Adams;N. Adhikari;R. Adhikari;V. Adya;C. Affeldt;D. Agarwal;M. Agathos;K. Agatsuma;N. Aggarwal;O. Aguiar;L. Aiello;A. Ain;P. Ajith;S. Akçay;T. Akutsu;S. Albanesi;A. Allocca;P. Altin;A. Amato;C. Anand;S. Anand;A. Ananyeva;S. Anderson;W. Anderson;M. Ando;T. Andrade;N. Andrés;T. Andri'c;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;M. Arogeti;S. Aronson;K. Arun;H. Asada;Y. Asali;G. Ashton;Y. Aso;M. Assiduo;S. Aston;P. Astone;F. Aubin;C. Austin;S. Babak;F. Badaracco;M. Bader;C. Badger;S. Bae;Y. Bae;A. Baer;S. Bagnasco;Y. Bai;L. Baiotti;J. Baird;R. Bajpai;M. Ball;G. Ballardin;S. Ballmer;A. Balsamo;G. Baltus;S. Banagiri;D. Bankar;J. Barayoga;C. Barbieri;B. Barish;D. Barker;P. Barneo;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;T. Bennett;J. Bentley;M. BenYaala;F. Bergamin;B. Berger;S. Bernuzzi;C. Berry;D. Bersanetti;A. Bertolini;J. Betzwieser;D. Beveridge;R. Bhandare;U. Bhardwaj;D. Bhattacharjee;S. Bhaumik;I. Bilenko;G. Billingsley;S. Bini;R. Birney;O. Birnholtz;S. Biscans;M. Bischi;S. Biscoveanu;A. Bisht;B. Biswas;M. Bitossi;M. Bizouard;J. Blackburn;C. Blair;D. Blair;R. Blair;F. Bobba;N. Bode;M. Boer;G. Bogaert;M. Boldrini;L. D. Bonavena;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;J. Brandt;J. Brau;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;T. Bulik;H. Bulten;A. Buonanno;R. Buscicchio;D. Buskulic;C. Buy;R. Byer;G. Davies;L. Cadonati;G. Cagnoli;C. Cahillane;J. C. Bustillo;J. Callaghan;T. Callister;E. Calloni;J. Cameron;J. Camp;M. Canepa;S. Canevarolo;M. Cannavacciuolo;K. Cannon;H. Cao;Z. Cao;E. Capocasa;E. Capote;G. Carapella;F. Carbognani;J. Carlin;M. Carney;M. Carpinelli;G. Carrillo;G. Carullo;T. Carver;J. C. Diaz;C. Casentini;G. Castaldi;S. Caudill;M. Cavaglià;F. Cavalier;R. Cavalieri;M. Ceasar;G. Cella;P. Cerd'a-Dur'an;E. Cesarini;W. Chaibi;K. Chakravarti;S. Subrahmanya;E. Champion;C. Chan;C. Chan;C. Chan;K. Chan;M. Chan;K. Chandra;P. Chanial;S. Chao;C. Chapman-Bird;P. Charlton;E. Chase;É. Chassande-Mottin;C. Chatterjee;D. Chatterjee;D. Chatterjee;M. Chaturvedi;S. Chaty;K. Chatziioannou;C. Chen;H. Chen;J. Chen;K. Chen;X. Chen;Y. Chen;Y.-R. Chen;Z. Chen;H. Cheng;C. Cheong;H. Cheung;H. Chia;F. Chiadini;C. Chiang;G. Chiarini;R. Chierici;A. Chincarini;M. Chiofalo;A. Chiummo;G. Cho;H. Cho;Rupesh Kumar Choudhary;S. Choudhary;N. Christensen;H. Chu;Q. Chu;Y. Chu;S. Chua;K. Chung;G. Ciani;P. Ciecieląg;M. Cie'slar;M. Cifaldi;A. Ciobanu;R. Ciolfi;F. Cipriano;A. Cirone;F. Clara;E. Clark;J. Clark;L. Clarke;P. Clearwater;S. Clesse;F. Cleva;E. Coccia;E. Codazzo;P. Cohadon;D. Cohen;L. Cohen;M. Colleoni;C. Collette;A. Colombo;M. Colpi;C. Compton;M. Constancio;L. Conti;S. Cooper;P. Corban;T. Corbitt;I. Cordero-Carri'on;S. Corezzi;K. Corley;N. Cornish;D. Corre;A. Corsi;S. Cortese;C. Costa;R. Cotesta;M. Coughlin;J. Coulon;S. Countryman;B. Cousins;P. Couvares;D. Coward;M. Cowart;D. Coyne;R. Coyne;J. Creighton;T. Creighton;A. Criswell;M. Croquette;S. Crowder;J. Cudell;T. Cullen;A. Cumming;R. Cummings;L. Cunningham;E. Cuoco;M. Curyło;P. Dabadie;T. D. Canton;S. Dall’Osso;G. D'alya;A. Dana;L. M. DaneshgaranBajastani;Beatrice D'Angelo;B. Danila;S. Danilishin;S. D’Antonio;K. Danzmann;C. Darsow-Fromm;A. Dasgupta;L. Datrier;S. Datta;V. Dattilo;I. Dave;M. Davier;D. Davis;M. Davis;E. Daw;P. Alarc'on;R. Dean;D. DeBra;M. Deenadayalan;J. Degallaix;M. D. Laurentis;S. Del'eglise;V. D. Favero;F. D. Lillo;N. D. Lillo;W. D. Pozzo;L. DeMarchi;F. Matteis;V. D'Emilio;N. Demos;T. Dent;A. Depasse;R. Pietri;R. Rosa;C. D. Rossi;R. DeSalvo;R. D. Simone;S. Dhurandhar;M. D'iaz;M. Diaz-Ortiz;N. Didio;T. Dietrich;L. Fiore;C. D. Fronzo;C. Giorgio;F. D. Giovanni;M. Giovanni;T. D. Girolamo;A. Lieto;B. Ding;S. D. Pace;I. Palma;F. Renzo;A. K. Divakarla;A. Dmitriev;Z. Doctor;L. D’Onofrio;F. Donovan;K. Dooley;S. Doravari;I. Dorrington;M. Drago;J. Driggers;Y. Drori;J. Ducoin;P. Dupej;O. Durante;D. D’Urso;P. Duverne;S. Dwyer;C. Eassa;P. Easter;M. Ebersold;T. Eckhardt;G. Eddolls;B. Edelman;T. Edo;O. Edy;A. Effler;S. Eguchi;J. Eichholz;S. Eikenberry;M. Eisenmann;R. Eisenstein;A. Ejlli;E. Engelby;Y. Enomoto;L. Errico;R. Essick;H. Estell'es;D. Estevez;Z. Etienne;T. Etzel;M. Evans;T. Evans;B. Ewing;V. Fafone;H. Fair;S. Fairhurst;A. M. Farah;S. Farinon;B. Farr;W. Farr;N. Farrow;E. Fauchon-Jones;G. Favaro;Marc Favata;M. Fays;M. Fazio;J. Feicht;M. Fejer;E. Fenyvesi;D. Ferguson;Á. Fernández-Galiana;I. Ferrante;T. A. Ferreira;F. Fidecaro;P. Figura;I. Fiori;M. Fishbach;R. Fisher;R. Fittipaldi;V. Fiumara;R. Flaminio;E. Floden;H. Fong;J. Font;B. Fornal;P. Forsyth;A. Franke;S. Frasca;F. Frasconi;C. Frederick;J. Freed;Z. Frei;A. Freise;R. Frey;P. Fritschel;V. Frolov;G. G. Fronz'e-G.;Y. Fujii;Y. Fujikawa;M. Fukunaga;M. Fukushima;P. Fulda;M. Fyffe;H. Gabbard;B. Gadre;J. Gair;J. Gais;S. Galaudage;R. Gamba;D. Ganapathy;A. Ganguly;D. Gao;S. Gaonkar;B. Garaventa;F. Garc'ia;C. Garc'ia-N'unez;C. Garc'ia-Quir'os;F. Garufi;B. Gateley;S. Gaudio;V. Gayathri;G. Ge;G. Gemme;A. Gennai;J. George;R. George;O. Gerberding;L. Gergely;P. Gewecke;S. Ghonge;A. Ghosh;A. Ghosh;Shaon Ghosh;Shrobana Ghosh;B. Giacomazzo;L. Giacoppo;J. Giaime;K. Giardina;D. Gibson;C. Gier;M. Giesler;P. Giri;F. Gissi;J. Glanzer;A. Gleckl;P. Godwin;E. Goetz;R. Goetz;N. Gohlke;J. Golomb;B. Goncharov;G. Gonz'alez;A. Gopakumar;M. Gosselin;R. Gouaty;D. Gould;B. Grace;A. Grado;M. Granata;V. Granata;A. Grant;S. Gras;P. Grassia;C. Gray;R. Gray;G. Greco;A. Green;R. Green;A. Gretarsson;E. Gretarsson;D. Griffith;W. Griffiths;H. L. Griggs;G. Grignani;A. Grimaldi;S. Grimm;H. Grote;S. Grunewald;P. Gruning;D. Guerra;G. Guidi;A. R. Guimaraes;G. Guix'e;H. Gulati;H.-K. Guo;Y. Guo;Anchal Gupta;Anuradha Gupta;P. Gupta;E. Gustafson;R. Gustafson;F. Guzmán;S. Ha;L. Haegel;A. Hagiwara;S. Haino;O. Halim;E. Hall;E. Hamilton;G. Hammond;W. Han;M. Haney;J. Hanks;C. Hanna;M. Hannam;O. Hannuksela;H. Hansen;T. Hansen;J. Hanson;T. Harder;T. Hardwick;K. Haris;J. Harms;G. Harry;I. Harry;D. Hartwig;K. Hasegawa;B. Haskell;R. Hasskew;C. Haster;K. Hattori;K. Haughian;H. Hayakawa;K. Hayama;F. Hayes;J. Healy;A. Heidmann;A. Heidt;M. Heintze;J. Heinze;J. Heinzel;H. Heitmann;F. Hellman;P. Hello;A. Helmling-Cornell;G. Hemming;M. Hendry;I. Heng;E. Hennes;J. Hennig;M. Hennig;A. Hernandez;F. Vivanco;M. Heurs;S. Hild;P. Hill;Y. Himemoto;A. Hines;Y. Hiranuma;N. Hirata;E. Hirose;S. Hochheim;D. Hofman;J. Hohmann;D. Holcomb;N. Holland;I. J. Hollows;Z. J. Holmes;K. Holt;D. Holz;Z. Hong;P. Hopkins;J. Hough;S. Hourihane;E. Howell;C. Hoy;D. Hoyland;A. Hreibi;B. Hsieh;Y. Hsu;G-Z. Huang;H. Huang;P. Huang;Y. Huang;Y. Huang;Y. Huang;M. Hubner;A. Huddart;B. Hughey;D. Hui;V. Hui;S. Husa;S. Huttner;R. Huxford;T. Huynh--Dinh-T.-Huynh--Dinh-1381195806;S. Ide;B. Idzkowski;A. Iess;B. Ikenoue;S. Imam;K. Inayoshi;C. Ingram;Y. Inoue;K. Ioka;M. Isi;K. Isleif;K. Ito;Y. Itoh;B. Iyer;K. Izumi;V. JaberianHamedan;T. Jacqmin;S. Jadhav;S. Jadhav;A. James;A. Jan;K. Jani;J. Janquart;K. Janssens;N. Janthalur;P. Jaranowski;D. Jariwala;R. Jaume;A. Jenkins;K. Jenner;C. Jeon;M. Jeunon;W. Jia;H. Jin;G. Johns;N. Johnson-McDaniel;A. Jones;D. Jones;J. Jones;P. Jones;R. Jones;R. Jonker;L. Ju;P. Jung;K. Jung;J. Junker;V. Juste;K. Kaihotsu;T. Kajita;M. Kakizaki;C. Kalaghatgi;V. Kalogera;B. Kamai;M. Kamiizumi;N. Kanda;S. Kandhasamy;G. Kang;J. Kanner;Y. Kao;S. Kapadia;D. Kapasi;S. Karat;C. Karathanasis;S. Karki;R. Kashyap;M. Kasprzack;W. Kastaun;S. Katsanevas;E. Katsavounidis;W. Katzman;T. Kaur;K. Kawabe;K. 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Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;P. Puppo;M. Purrer;H. Qi;V. Quetschke;R. Quitzow-James;N. Qutob;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;A. Ray;V. Raymond;N. Raza;M. Razzano;J. Read;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. Reid;D. Reitze;P. Relton;A. Renzini;P. Rettegno;A. Reza;M. Rezac;F. Ricci;D. Richards;J. Richardson;L. Richardson;G. Riemenschneider;K. Riles;S. Rinaldi;K. Rink;M. Rizzo;N. Robertson;R. Robie;F. Robinet;A. Rocchi;S. Rodriguez;L. Rolland;J. Rollins;M. Romanelli;R. Romano;C. Romel;A. Romero-Rodr'iguez;I. Romero-Shaw;J. Romie;S. Ronchini;L. Rosa;C. Rose;D. Rosi'nska;M. Ross;S. Rowan;S. Rowlinson;S. Roy;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;Joaquín Sánchez;L. Sanchez;N. Sanchis-Gual;J. Sanders;A. Sanuy;T. R. Saravanan;N. Sarin;B. Sassolas;H. Satari;B. Sathyaprakash;S. Sato;T. Sato;O. Sauter;R. Savage;T. Sawada;D. Sawant;H. Sawant;S. Sayah;D. Schaetzl;M. Scheel;J. Scheuer;M. Schiworski;P. Schmidt;S. Schmidt;R. Schnabel;M. Schneewind;R. Schofield;A. Schonbeck;B. Schulte;B. Schutz;E. Schwartz;J. Scott;S. Scott;M. Seglar-Arroyo;T. Sekiguchi;Y. Sekiguchi;D. Sellers;A. Sengupta;D. Sentenac;E. Seo;V. Sequino;A. Sergeev;Y. Setyawati;T. Shaffer;M. Shahriar;B. Shams;L. Shao;A. Sharma;P. Sharma;P. Shawhan;N. Shcheblanov;S. Shibagaki;M. Shikauchi;R. Shimizu;T. Shimoda;K. Shimode;H. Shinkai;T. Shishido;A. Shoda;D. Shoemaker;D. Shoemaker;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;J. Soldateschi;S. Somala;K. Somiya;E. Son;K. Soni;S. Soni;V. Sordini;F. Sorrentino;N. Sorrentino;H. Sotani;R. Soulard;T. Souradeep;E. Sowell;V. Spagnuolo;A. 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Walsh;J. Wang;J. Wang;W. H. Wang;R. Ward;J. Warner;M. Was;T. Washimi;N. Y. Washington;J. Watchi;B. Weaver;S. Webster;M. Weinert;A. Weinstein;R. Weiss;C. Weller;F. Wellmann;L. Wen;P. Wessels;K. Wette;J. Whelan;D. White;B. Whiting;C. Whittle;D. Wilken;D. Williams;M. Williams;N. Williams;A. Williamson;J. Willis;B. Willke;D. Wilson;W. Winkler;C. Wipf;T. Włodarczyk;G. Woan;J. Woehler;J. Wofford;I. C. Wong;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;Y. Yang;Yang Yang-Yang;Z. Yang;M. Yap;D. Yeeles;A. Yelikar;M. Ying;K. Yokogawa;J. Yokoyama;T. Yokozawa;J. Yoo;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;T. Zhang;Y. Zhang;C. Zhao;G. Zhao;Y. Zhao;Yue Zhao;Y. Zheng;R. Zhou;Z. Zhou;X. Zhu;Z. Zhu;A. Zimmerman;Y. Zlochower;M. Zucker;J. Zweizig

Search for Gravitational Waves Associated with Fast Radio Bursts Detected by CHIME/FRB during the LIGO–Virgo Observing Run O3a

• DOI: 10.3847/1538-4357/acd770
• 发表时间: 2023-09
• 期刊: The Astrophysical Journal
• 作者: B. Lane;R. Lang;J. Lange;B. Lantz;I. L. Rosa;A. Lartaux-Vollard;P. Lasky;M. Laxen;A. Lazzarini;C. Lazzaro;P. Leaci;S. Leavey;Y. Lecoeuche;H. Lee;H. Lee;H. W. Lee;J. Lee;K. Lee;Ray-Kuang Lee;J. Lehmann;A. Lemaitre;M. Leonardi;N. Leroy;N. Letendre;C. Lévesque;Y. Levin;J. Leviton;K. Leyde;A. Li;B. Li;J. Li;K. Li;T. G. F. Li;X. Li;C.Y. Lin;F. Lin;F. Lin;H. Lin;L. Lin;F. Linde;S. Linker;J. Linley;T. Littenberg;G. Liu;J. Liu;K. Liu;X. Liu;F. Llamas;M. Llorens-Monteagudo;R. K. Lo;A. Lockwood;L. London;A. Longo;D. Lopez;M. Portilla;M. Lorenzini;V. Loriette;M. Lormand;G. Losurdo;T. Lott;J. Lough;C. Lousto;G. Lovelace;J. F. Lucaccioni;H. Lück;D. Lumaca;A. Lundgren;L. Luo;J. Lynam;R. Macas;M. Macinnis;D. Macleod;I. MacMillan;A. Macquet;I. M. Hernandez;C. Magazzù;R. Magee;R. Maggiore;M. Magnozzi;S. Mahesh;E. Majorana;C. Makarem;I. Maksimovic;S. Maliakal;A. Malik;N. Man;V. Mandic;V. Mangano;J. Mango;G. Mansell;M. Manske;M. Mantovani;M. Mapelli;F. Marchesoni;M. Marchiò;F. Marion;Z. Mark;S. Márka;Z. Márka;C. Markakis;A. Markosyan;A. Markowitz;E. Maros;A. Marquina;S. Marsat;F. Martelli;I. Martin;R. Martin;M. Martínez;V. Martínez;V. Martínez;K. Martinovic;D. Martynov;E. J. Marx;H. Masalehdan;K. Mason;E. Massera;A. Masserot;T. Massinger;M. Masso-Reid;S. Mastrogiovanni;A. Matas;M. Mateu-Lucena;F. Matichard;M. Matiushechkina;N. Mavalvala;J. McCann;R. Mccarthy;D. McClelland;P. McClincy;S. Mccormick;L. McCuller;G. McGhee;S. Mcguire;C. McIsaac;J. McIver;T. McRae;S. McWilliams;D. Meacher;M. Mehmet;A. Mehta;Q. Meijer;A. Melatos;D. Melchor;G. Mendell;A. Menéndez-Vázquez;C. Menoni;R. Mercer;L. Mereni;K. Merfeld;E. Merilh;J. D. Merritt;M. 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;A. Miller;B. Miller;M. Millhouse;J. Mills;E. Milotti;O. Minazzoli;Y. Minenkov;N. Mio;L. Mir;M. Miravet-Tenés;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;E. Moguel;K. Mogushi;S. Mohapatra;S. Mohite;I. Molina;M. Molina-Ruiz;M. Mondin;M. Montani;C. Moore;D. Moraru;F. Morawski;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;S. Mukherjee;N. Mukund;A. Mullavey;J. Munch;E. Muniz;P. Murray;R. Musenich;S. Muusse;S. Nadji;K. Nagano;S. Nagano;A. Nagar;K. Nakamura;H. Nakano;M. Nakano;R. Nakashima;Y. Nakayama;V. Napolano;I. Nardecchia;T. Narikawa;L. Naticchioni;B. Nayak;R. Nayak;R. Negishi;B. Neil;J. Neilson;G. Nelemans;T. Nelson;M. Nery;P. Neubauer;A. Neunzert;K. Ng;S. Ng;C. Nguyen;P. Nguyen;T. Nguyen;L. Quynh;S. Nichols;A. Nishizawa;S. Nissanke;E. Nitoglia;F. Nocera;Manuel Norman;S. Nozaki;L. Nuttall;J. Oberling;B. O'Brien;Y. Obuchi;J. O'Dell;E. Oelker;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;O. Palashov;C. Palomba;H. Pan;K. Pan;P. Panda;H. Pang;C. Pankow;F. Pannarale;F. Panther;F. Paoletti;A. Paoli;A. Paolone;A. Parisi;H. Park;J. Park;W. Parker;D. Pascucci;A. Pasqualetti;R. Passaquieti;D. Passuello;M. Patel;M. Pathak;B. Patricelli;A. S. Patron;S. Patrone;S. Paul;E. Payne;M. Pedraza;M. Pegoraro;A. Pele;F. Arellano;S. Penn;A. Perego;A. Pereira;T. Pereira;C. Perez;C. Périgois;C. Perkins;A. Perreca;S. Perriès;J. Petermann;D. Petterson;H. Pfeiffer;K. A. Pham;K. S. Phukon;O. Piccinni;M. Piendibene;F. Piergiovanni;L. Pierini;V. Pierro;G. Pillant;M. Pillas;F. Pilo;L. Pinard;M. Pinto;B. Piotrzkowski;K. Piotrzkowski;M. Pirello;E. Placidi;L. Planas;W. Plastino;C. Pluchar;R. Poggiani;E. Polini;R. Poulton;J. Powell;M. Pracchia;T. Pradier;A. K. Prajapati;K. Prasai;R. Prasanna;G. Pratten;L. Prokhorov;P. Prosposito;L. Prudenzi;A. Puecher;M. Punturo;F. Puosi;V. Quetschke;F. Raab;G. Raaijmakers;N. Radulesco;P. Raffai;S. Raja;C. Rajan;K. Ramirez;J. Rana;P. Rapagnani;U. Rapol;A. Ray;V. Raymond;M. Razzano;L. A. Rees;T. Regimbau;L. Rei;S. Reid;S. Reid;D. Reitze;P. Relton;A. Renzini;P. Rettegno;M. Rezac;F. Ricci