Related papers: Towards improving the prospects for coordinated gr…

The Challenges Ahead for Multimessenger Analyses of Gravitational Waves and Kilonova: a Case Study on GW190425

In recent years, there have been significant advances in multi-messenger astronomy due to the discovery of the first, and so far only confirmed, gravitational wave event with a simultaneous electromagnetic (EM) counterpart, as well as…

High Energy Astrophysical Phenomena · Physics 2021-12-15 Geert Raaijmakers , Samaya Nissanke , Francois Foucart , Mansi M. Kasliwal , Mattia Bulla , Rodrigo Fernandez , Amelia Henkel , Tanja Hinderer , Kenta Hotokezaka , Kamilė Lukošiūtė , Tejaswi Venumadhav , Sarah Antier , Michael W. Coughlin , Tim Dietrich , Thomas D. P. Edwards

Host galaxies and electromagnetic counterparts to binary neutron star mergers across the cosmic time: Detectability of GW170817-like events

The detection of electromagnetic radiation (EM) accompanying the gravitational wave (GW) signal from the binary neutron star (BNS) merger GW170817 has revealed that these systems constitute at least a fraction of the progenitors of short…

High Energy Astrophysical Phenomena · Physics 2022-03-30 Rosalba Perna , M. Celeste Artale , Yi-Han Wang , Michela Mapelli , Davide Lazzati , Cecilia Sgalletta , Filippo Santoliquido

Viewing angle of binary neutron star mergers

The joint detection of the gravitational wave (GW) GW170817 and its electromagnetic (EM) counterparts GRB170817A and kilonova AT 2017gfo has triggered extensive study of the EM emission of binary neutron star mergers. A parameter which is…

High Energy Astrophysical Phenomena · Physics 2019-08-28 Hsin-Yu Chen , Salvatore Vitale , Ramesh Narayan

Prospects for joint observations of gravitational waves and gamma rays from merging neutron star binaries

The detection of the events GW150914 and GW151226, both consistent with the merger of a binary black hole system (BBH), opened the era of gravitational wave (GW) astronomy. Besides BBHs, the most promising GW sources are the coalescences of…

High Energy Astrophysical Phenomena · Physics 2016-12-07 Barbara Patricelli , Massimiliano Razzano , Giancarlo Cella , Francesco Fidecaro , Elena Pian , Marica Branchesi , Antonio Stamerra

Electromagnetic transients as triggers in searches for gravitational waves from compact binary mergers

The detection of an electromagnetic transient which may originate from a binary neutron star merger can increase the probability that a given segment of data from the LIGO-Virgo ground-based gravitational-wave detector network contains a…

Instrumentation and Methods for Astrophysics · Physics 2013-06-27 Luke Zoltan Kelley , Ilya Mandel , Enrico Ramirez-Ruiz

Probing neutron stars with gravitational waves

Within the next decade gravitational-wave (GW) observations by Advanced LIGO in the United States, Advanced Virgo and GEO HF in Europe, and possibly other ground-based instruments will provide unprecedented opportunities to look directly…

Solar and Stellar Astrophysics · Physics 2009-03-17 Benjamin J. Owen

Joint analysis of gravitational-wave and electromagnetic data of mergers: breaking an afterglow model degeneracy in GW170817 and in future events

On August 17, 2017, Advanced LIGO and Virgo observed GW170817, the first gravitational-wave (GW) signal from a binary neutron star merger. It was followed by a short-duration gamma-ray burst, GRB 170817A, and by a non-thermal afterglow…

High Energy Astrophysical Phenomena · Physics 2023-06-14 Giulia Gianfagna , Luigi Piro , Francesco Pannarale , Hendrik Van Eerten , Fulvio Ricci , Geoffrey Ryan , Eleonora Troja

Distinguishing the nature of comparable-mass neutron star binary systems with multimessenger observations: GW170817 case study

The discovery of GW170817 with gravitational waves (GWs) and electromagnetic (EM) radiation is prompting new questions in strong-gravity astrophysics. Importantly, it remains unknown whether the progenitor of the merger comprised two…

High Energy Astrophysical Phenomena · Physics 2020-03-16 Tanja Hinderer , Samaya Nissanke , Francois Foucart , Kenta Hotokezaka , Trevor Vincent , Mansi Kasliwal , Patricia Schmidt , Andrew R. Williamson , David Nichols , Matthew Duez , Lawrence E. Kidder , Harald P. Pfeiffer , Mark A. Scheel

Radio Remnants of Compact Binary Mergers - the Electromagnetic Signal that will follow the Gravitational Waves

The question "what is the observable electromagnetic (EM) signature of a compact binary merger?" is an intriguing one with crucial consequences to the quest for gravitational waves (GW). Compact binary mergers are prime sources of GW,…

High Energy Astrophysical Phenomena · Physics 2015-03-18 Ehud Nakar , Tsvi Piran

Implementation and testing of the first prompt search for gravitational wave transients with electromagnetic counterparts

Aims. A transient astrophysical event observed in both gravitational wave (GW) and electromagnetic (EM) channels would yield rich scientific rewards. A first program initiating EM follow-ups to possible transient GW events has been…

Instrumentation and Methods for Astrophysics · Physics 2015-05-30 The LIGO Scientific Collaboration , Virgo Collaboration , J. Abadie , B. P. Abbott , R. Abbott , T. D. Abbott , M. Abernathy , T. Accadia , F. Acernese , C. Adams , R. Adhikari , C. Affeldt , P. Ajith , B. Allen , G. S. Allen , E. Amador Ceron , D. Amariutei , R. S. Amin , S. B. Anderson , W. G. Anderson , K. Arai , M. A. Arain , M. C. Araya , S. M. Aston , P. Astone , D. Atkinson , P. Aufmuth , C. Aulbert , B. E. Aylott , S. Babak , P. Baker , G. Ballardin , S. Ballmer , D. Barker , F. Barone , B. Barr , P. Barriga , L. Barsotti , M. Barsuglia , M. A. Barton , I. Bartos , R. Bassiri , M. Bastarrika , A. Basti , J. Batch , J. Bauchrowitz , Th. S. Bauer , M. Bebronne , B. Behnke , M. G. Beker , A. S. Bell , A. Belletoile , I. Belopolski , M. Benacquista , J. M. Berliner , A. Bertolini , J. Betzwieser , N. Beveridge , P. T. Beyersdorf , I. A. Bilenko , G. Billingsley , J. Birch , R. Biswas , M. Bitossi , M. A. Bizouard , E. Black , J. K. Blackburn , L. Blackburn , D. Blair , B. Bland , M. Blom , O. Bock , T. P. Bodiya , C. Bogan , R. Bondarescu , F. Bondu , L. Bonelli , R. Bonnand , R. Bork , M. Born , V. Boschi , S. Bose , L. Bosi , B. Bouhou , S. Braccini , C. Bradaschia , P. R. Brady , V. B. Braginsky , M. Branchesi , J. E. Brau , J. Breyer , T. Briant , D. O. Bridges , A. Brillet , M. Brinkmann , V. Brisson , M. Britzger , A. F. Brooks , D. A. Brown , A. Brummit , T. Bulik , H. J. Bulten , A. Buonanno , J. Burguet--Castell , O. Burmeister , D. Buskulic , C. Buy , R. L. Byer , L. Cadonati , G. Cagnoli , J. Cain , E. Calloni , J. B. Camp , P. Campsie , J. Cannizzo , K. Cannon , B. Canuel , J. Cao , C. D. Capano , F. Carbognani , S. Caride , S. Caudill , M. Cavaglià , F. Cavalier , R. Cavalieri , G. Cella , C. Cepeda , E. Cesarini , O. Chaibi , T. Chalermsongsak , E. Chalkley , P. Charlton , E. Chassande-Mottin , S. Chelkowski , Y. Chen , A. Chincarini , A. Chiummo , H. Cho , N. Christensen , S. S. Y. Chua , C. T. Y. Chung , S. Chung , G. Ciani , F. Clara , D. E. Clark , J. Clark , J. H. Clayton , F. Cleva , E. Coccia , P. -F. Cohadon , C. N. Colacino , J. Colas , A. Colla , M. Colombini , A. Conte , R. Conte , D. Cook , T. R. Corbitt , M. Cordier , N. Cornish , A. Corsi , C. A. Costa , M. Coughlin , J. -P. Coulon , P. Couvares , D. M. Coward , D. C. Coyne , J. D. E. Creighton , T. D. Creighton , A. M. Cruise , A. Cumming , L. Cunningham , E. Cuoco , R. M. Cutler , K. Dahl , S. L. Danilishin , R. Dannenberg , S. D'Antonio , K. Danzmann , V. Dattilo , B. Daudert , H. Daveloza , M. Davier , G. Davies , E. J. Daw , R. Day , T. Dayanga , R. De Rosa , D. DeBra , G. Debreczeni , J. Degallaix , W. Del Pozzo , M. del Prete , T. Dent , V. Dergachev , R. DeRosa , R. DeSalvo , V. Dhillon , S. Dhurandhar , L. Di Fiore , A. Di Lieto , I. Di Palma , M. Di Paolo Emilio , A. Di Virgilio , M. Díaz , A. Dietz , F. Donovan , K. L. Dooley , S. Dorsher , M. Drago , R. W. P. Drever , J. C. Driggers , Z. Du , J. -C. Dumas , S. Dwyer , T. Eberle , M. Edgar , M. Edwards , A. Effler , P. Ehrens , G. Endrőczi , R. Engel , T. Etzel , K. Evans , M. Evans , T. Evans , M. Factourovich , V. Fafone , S. Fairhurst , Y. Fan , B. F. Farr , W. Farr , D. Fazi , H. Fehrmann , D. Feldbaum , I. Ferrante , F. Fidecaro , L. S. Finn , I. Fiori , R. P. Fisher , R. Flaminio , M. Flanigan , S. Foley , E. Forsi , L. A. Forte , N. Fotopoulos , J. -D. Fournier , J. Franc , S. Frasca , F. Frasconi , M. Frede , M. Frei , Z. Frei , A. Freise , R. Frey , T. T. Fricke , J. K. Fridriksson , D. Friedrich , P. Fritschel , V. V. Frolov , P. J. Fulda , M. Fyffe , M. Galimberti , L. Gammaitoni , M. R. Ganija , J. Garcia , J. A. Garofoli , F. Garufi , M. E. Gáspár , G. Gemme , R. Geng , E. Genin , A. Gennai , L. Á. Gergely , S. Ghosh , J. A. Giaime , S. Giampanis , K. D. Giardina , A. Giazotto , C. Gill , E. Goetz , L. M. Goggin , G. González , M. L. Gorodetsky , S. Goßler , R. Gouaty , C. Graef , M. Granata , A. Grant , S. Gras , C. Gray , N. Gray , R. J. S. Greenhalgh , A. M. Gretarsson , C. Greverie , R. Grosso , H. Grote , S. Grunewald , G. M. Guidi , C. Guido , R. Gupta , E. K. Gustafson , R. Gustafson , T. Ha , B. Hage , J. M. Hallam , D. Hammer , G. Hammond , J. Hanks , C. Hanna , J. Hanson , J. Harms , G. M. Harry , I. W. Harry , E. D. Harstad , M. T. Hartman , K. Haughian , K. Hayama , J. -F. Hayau , T. Hayler , J. Heefner , A. Heidmann , M. C. Heintze , H. Heitmann , P. Hello , M. A. Hendry , I. S. Heng , A. W. Heptonstall , V. Herrera , M. Hewitson , S. Hild , D. Hoak , K. A. Hodge , K. Holt , J. Homan , T. Hong , S. Hooper , D. J. Hosken , J. Hough , E. J. Howell , B. Hughey , S. Husa , S. H. Huttner , T. Huynh-Dinh , D. R. Ingram , R. Inta , T. Isogai , A. Ivanov , K. Izumi , M. Jacobson , H. Jang , P. Jaranowski , W. W. Johnson , D. I. Jones , G. Jones , R. Jones , L. Ju , P. Kalmus , V. Kalogera , I. Kamaretsos , S. Kandhasamy , G. Kang , J. B. Kanner , E. Katsavounidis , W. Katzman , H. Kaufer , K. Kawabe , S. Kawamura , F. Kawazoe , W. Kells , D. G. Keppel , Z. Keresztes , A. Khalaidovski , F. Y. Khalili , E. A. Khazanov , B. Kim , C. Kim , D. Kim , H. Kim , K. Kim , N. Kim , Y. -M. Kim , P. J. King , M. Kinsey , D. L. Kinzel , J. S. Kissel , S. Klimenko , K. Kokeyama , V. Kondrashov , R. Kopparapu , S. Koranda , W. Z. Korth , I. Kowalska , D. Kozak , V. Kringel , S. Krishnamurthy , B. Krishnan , A. Królak , G. Kuehn , R. Kumar , P. Kwee , M. Laas-Bourez , P. K. Lam , M. Landry , M. Lang , B. Lantz , N. Lastzka , C. Lawrie , A. Lazzarini , P. Leaci , C. H. Lee , H. M. Lee , N. Leindecker , J. R. Leong , I. Leonor , N. Leroy , N. Letendre , J. Li , T. G. F. Li , N. Liguori , P. E. Lindquist , N. A. Lockerbie , D. Lodhia , M. Lorenzini , V. Loriette , M. Lormand , G. Losurdo , J. Luan , M. Lubinski , H. Lück , A. P. Lundgren , E. Macdonald , B. Machenschalk , M. MacInnis , D. M. Macleod , M. Mageswaran , K. Mailand , E. Majorana , I. Maksimovic , N. Man , I. Mandel , V. Mandic , M. Mantovani , A. Marandi , F. Marchesoni , F. Marion , S. Márka , Z. Márka , A. Markosyan , E. Maros , J. Marque , F. Martelli , I. W. Martin , R. M. Martin , J. N. Marx , K. Mason , A. Masserot , F. Matichard , L. Matone , R. A. Matzner , N. Mavalvala , G. Mazzolo , R. McCarthy , D. E. McClelland , P. McDaniel , S. C. McGuire , G. McIntyre , D. J. A. McKechan , G. D. Meadors , M. Mehmet , T. Meier , A. Melatos , A. C. Melissinos , G. Mendell , D. Menendez , R. A. Mercer , L. Merill , S. Meshkov , C. Messenger , M. S. Meyer , H. Miao , C. Michel , L. Milano , J. Miller , Y. Minenkov , V. P. Mitrofanov , G. Mitselmakher , R. Mittleman , O. Miyakawa , B. Moe , P. Moesta , M. Mohan , S. D. Mohanty , S. R. P. Mohapatra , D. Moraru , G. Moreno , N. Morgado , A. Morgia , T. Mori , S. Mosca , K. Mossavi , B. Mours , C. M. Mow--Lowry , C. L. Mueller , G. Mueller , S. Mukherjee , A. Mullavey , H. Müller-Ebhardt , J. Munch , P. G. Murray , A. Mytidis , T. Nash , L. Naticchioni , R. Nawrodt , V. Necula , J. Nelson , G. Newton , E. Nishida , A. Nishizawa , F. Nocera , D. Nolting , L. Nuttall , E. Ochsner , J. O'Dell , E. Oelker , G. H. Ogin , J. J. Oh , S. H. Oh , R. G. Oldenburg , B. O'Reilly , R. O'Shaughnessy , C. Osthelder , C. D. Ott , D. J. Ottaway , R. S. Ottens , H. Overmier , B. J. Owen , A. Page , G. Pagliaroli , L. Palladino , C. Palomba , Y. Pan , C. Pankow , F. Paoletti , M. A. Papa , M. Parisi , A. Pasqualetti , R. Passaquieti , D. Passuello , P. Patel , D. Pathak , M. Pedraza , P. Peiris , L. Pekowsky , S. Penn , C. Peralta , A. Perreca , G. Persichetti , M. Phelps , M. Pickenpack , F. Piergiovanni , M. Pietka , L. Pinard , I. M. Pinto , M. Pitkin , H. J. Pletsch , M. V. Plissi , R. Poggiani , J. Pöld , F. Postiglione , M. Prato , V. Predoi , L. R. Price , M. Prijatelj , M. Principe , S. Privitera , R. Prix , G. A. Prodi , L. Prokhorov , O. Puncken , M. Punturo , P. Puppo , V. Quetschke , F. J. Raab , D. S. Rabeling , I. Rácz , H. Radkins , P. Raffai , M. Rakhmanov , C. R. Ramet , B. Rankins , P. Rapagnani , S. Rapoport , V. Raymond , V. Re , K. Redwine , C. M. Reed , T. Reed , T. Regimbau , S. Reid , D. H. Reitze , F. Ricci , R. Riesen , K. Riles , N. A. Robertson , F. Robinet , C. Robinson , E. L. Robinson , A. Rocchi , S. Roddy , C. Rodriguez , M. Rodruck , L. Rolland , J. Rollins , J. D. Romano , R. Romano , J. H. Romie , D. Rosińska , C. Röver , S. Rowan , A. Rüdiger , P. Ruggi , K. Ryan , H. Ryll , P. Sainathan , M. Sakosky , F. Salemi , L. Sammut , L. Sancho de la Jordana , V. Sandberg , S. Sankar , V. Sannibale , L. Santamaría , I. Santiago-Prieto , G. Santostasi , B. Sassolas , B. S. Sathyaprakash , S. Sato , M. Satterthwaite , P. R. Saulson , R. L. Savage , R. Schilling , S. Schlamminger , R. Schnabel , R. M. S. Schofield , B. Schulz , B. F. Schutz , P. Schwinberg , J. Scott , S. M. Scott , A. C. Searle , F. Seifert , D. Sellers , A. S. Sengupta , D. Sentenac , A. Sergeev , D. A. Shaddock , M. Shaltev , B. Shapiro , P. Shawhan , D. H. Shoemaker , A. Sibley , X. Siemens , D. Sigg , A. Singer , L. Singer , A. M. Sintes , G. Skelton , B. J. J. Slagmolen , J. Slutsky , J. R. Smith , M. R. Smith , N. D. Smith , R. J. E. Smith , K. Somiya , B. Sorazu , J. Soto , F. C. Speirits , L. Sperandio , M. Stefszky , A. J. Stein , E. Steinert , J. Steinlechner , S. Steinlechner , S. Steplewski , A. Stochino , R. Stone , K. A. Strain , S. Strigin , A. S. Stroeer , R. Sturani , A. L. Stuver , T. Z. Summerscales , M. Sung , S. Susmithan , P. J. Sutton , B. Swinkels , M. Tacca , L. Taffarello , D. Talukder , D. B. Tanner , S. P. Tarabrin , J. R. Taylor , R. Taylor , P. Thomas , K. A. Thorne , K. S. Thorne , E. Thrane , A. Thüring , C. Titsler , K. V. Tokmakov , A. Toncelli , M. Tonelli , O. Torre , C. Torres , C. I. Torrie , E. Tournefier , F. Travasso , G. Traylor , M. Trias , K. Tseng , L. Turner , D. Ugolini , K. Urbanek , H. Vahlbruch , G. Vajente , M. Vallisneri , J. F. J. van den Brand , C. Van Den Broeck , S. van der Putten , A. A. van Veggel , S. Vass , M. Vasuth , R. Vaulin , M. Vavoulidis , A. Vecchio , G. Vedovato , J. Veitch , P. J. Veitch , C. Veltkamp , D. Verkindt , F. Vetrano , A. Viceré , A. E. Villar , J. -Y. Vinet , S. Vitale , S. Vitale , H. Vocca , C. Vorvick , S. P. Vyatchanin , A. Wade , S. J. Waldman , L. Wallace , Y. Wan , X. Wang , Z. Wang , A. Wanner , R. L. Ward , M. Was , P. Wei , M. Weinert , A. J. We , R. Weiss , L. Wen , S. Wen , P. Wessels , M. West , T. Westphal , K. Wette , J. T. Whelan , S. E. Whitcomb , D. White , B. F. Whiting , C. Wilkinson , P. A. Willems , H. R. Williams , L. Williams , B. Willke , L. Winkelmann , W. Winkler , C. C. Wipf , A. G. Wiseman , H. Wittel , G. Woan , R. Wooley , J. Worden , J. Yablon , I. Yakushin , H. Yamamoto , K. Yamamoto , H. Yang , D. Yeaton-Massey , S. Yoshida , P. Yu , M. Yvert , A. Zadroźny , M. Zanolin , J. -P. Zendri , F. Zhang , L. Zhang , W. Zhang , Z. Zhang , C. Zhao , N. Zotov , M. E. Zucker , J. Zweizig , C. Akerlof , M. Boer , R. Fender , N. Gehrels , A. Klotz , E. O. Ofek , M. Smith , M. Sokolowski , B. W. Stappers , I. Steele , J. Swinbank , R. A. M. J. Wijers , W. Zheng

Testing gravity with gravitational waves $\times$ electromagnetic probes cross-correlations

In a General Relativistic framework, Gravitational Waves (GW) and Electromagnetic (EM) waves are expected to respond in the same way to the effects of matter perturbations between the emitter and the observer. A different behaviour might be…

Cosmology and Nongalactic Astrophysics · Physics 2023-02-14 Giulio Scelfo , Maria Berti , Alessandra Silvestri , Matteo Viel

The Gravitational Wave Treasure Map: A Tool to Coordinate, Visualize, and Assess the Electromagnetic Follow-Up of Gravitational Wave Events

We present the Gravitational Wave Treasure Map, a tool to coordinate, visualize, and assess the electromagnetic follow-up of gravitational wave (GW) events. With typical GW localization regions of hundreds to thousands of square degrees and…

High Energy Astrophysical Phenomena · Physics 2020-05-20 Samuel D. Wyatt , Aaron Tohuvavohu , Iair Arcavi , Michael J. Lundquist , D. Andrew Howell , David J. Sand

The H.E.S.S. Gravitational Wave and Gamma-Ray Burst Follow-Up Programs

Multi-wavelength and multi-messenger astrophysics have experienced rapid growth over the past decade, seeking a complete picture of different cosmic phenomena. Transient sources, in particular, benefit from the input of multi-messenger…

High Energy Astrophysical Phenomena · Physics 2025-10-06 Bernardo Cornejo , Halim Ashkar , Matteo Cerruti , Ilja Jaroschewski , Pierre Pichard , Santiago Pita , Fabian Schussler

Where to find Electromagnetic Wave Counterparts of stellar-mass binary black hole mergers?

Multi-messenger astronomy combining Gravitational Wave (GW) and Electromagnetic Wave (EM) observation brings huge impact on physics, astrophysics and cosmology. However, the majority of sources to be detected with currently running…

High Energy Astrophysical Phenomena · Physics 2019-10-16 Shu-Xu Yi , K. S. Cheng

Merger and Mass Ejection of Neutron-Star Binaries

Mergers of binary neutron stars and black hole-neutron star binaries are one of the most promising sources for the ground-based gravitational-wave (GW) detectors and also a high-energy astrophysical phenomenon as illustrated by the…

High Energy Astrophysical Phenomena · Physics 2019-08-08 Masaru Shibata , Kenta Hotokezaka

Prospects for the detection of electromagnetic counterparts to gravitational wave events

Various models for electromagnetic emissions correlated with the gravitational wave signals expected to be detectable by the current and planned gravitational wave detectors are studied. The position error on the location of a gravitational…

Astrophysics · Physics 2009-11-07 Julien Sylvestre

Searches for counterparts of gravitational waves at very high energies with H.E.S.S

The recent milestones in multi-messenger astronomy have opened new ways to study the Unverse. The unprecedented gravitational wave (GW) follow-up campaigns established the power that the combination of different messengers has to identify…

High Energy Astrophysical Phenomena · Physics 2019-08-20 Monica Seglar-Arroyo , Halim Ashkar , Simon Bonnefoy , Francois Brun , Kathrin Egberts , Matthias Füßling , Clemens Hoischen , Thomas Murach , Stefan Ohm , Gerd Pühlhofer , Gavin Rowell , Fabian Schüssler , Andrew Taylor

Bayesian Multi-Messenger Search Method for Common Sources of Gravitational Waves and High-Energy Neutrinos

Multi-messenger astrophysics is undergoing a transition towards low-latency searches based on signals that could not individually be established as discoveries. The rapid identification of signals is important in order to initiate timely…

High Energy Astrophysical Phenomena · Physics 2019-10-30 Imre Bartos , Doga Veske , Azadeh Keivani , Zsuzsa Marka , Stefan Countryman , Erik Blaufuss , Chad Finley , Szabolcs Marka

Localization of binary mergers with gravitational-wave detectors of second and third generation

The observation of gravitational wave signals from binary black hole mergers has established the field of gravitational wave astronomy. It is expected that future networks of gravitational wave detectors will possess great potential in…

General Relativity and Quantum Cosmology · Physics 2018-06-06 Joseph Mills , Vaibhav Tiwari , Stephen Fairhurst

Electromagnetic counterparts to gravitational wave events from Gaia

The recent discoveries of gravitational wave events and in one case also its electromagnetic (EM) counterpart allow us to study the Universe in a novel way. The increased sensitivity of the LIGO and Virgo detectors has opened the…

Instrumentation and Methods for Astrophysics · Physics 2020-04-24 Z. Kostrzewa-Rutkowska , P. G. Jonker , S. T. Hodgkin , D. Eappachen , D. L. Harrison , S. E. Koposov , G. Rixon , L. Wyrzykowski , A. Yoldas , E. Breedt , A. Delgado , M. van Leeuwen , T. Wevers , P. W. Burgess , F. De Angeli , D. W. Evans , P. J. Osborne , M. Riello