Related papers: Gravitational wave optical counterpart searching b…

Electromagnetic follow-up of gravitational wave candidates: perspectives in INAF

The electromagnetic (EM) emission associated with a gravitational wave (GW) signal is one of the main goal of future astronomy. Merger of neutron stars and/or black holes and core-collapse of massive stars are expected to cause rapid…

High Energy Astrophysical Phenomena · Physics 2015-07-21 S. Piranomonte , E. Brocato , M. Branchesi , S. Campana , E. Cappellaro , S. Covino , A. Grado , E. Palazzi , L. Nicastro , E. Pian , G. Stratta , G. Greco , M. Castellano , G. Giuffrida , S. Marinoni , L. Pulone , A. Antonelli , M. G. Bernardini , P. D'avanzo , A. Melandri , L. Stella

Searching for electromagnetic counterparts of gravitational wave transients

A pioneering electromagnetic (EM) observation follow-up program of candidate gravitational wave (GW) triggers has been performed, Dec 17 2009 to Jan 8 2010 and Sep 4 to Oct 20 2010, during the recent LIGO/Virgo run. The follow-up program…

Instrumentation and Methods for Astrophysics · Physics 2019-08-15 M. Branchesi , A. Klotz , M. Laas-Bourez

On Discovering Electromagnetic Emission from Neutron Star Mergers: The Early Years of Two Gravitational Wave Detectors

We present the first simulation addressing the prospects of finding an electromagnetic (EM) counterpart to gravitational wave detections (GW) during the early years of only two advanced interferometers. The perils of such a search may have…

High Energy Astrophysical Phenomena · Physics 2015-06-17 Mansi M. Kasliwal , Samaya Nissanke

LOOC UP: Locating and observing optical counterparts to gravitational wave bursts

Gravitational wave (GW) bursts (short duration signals) are expected to be associated with highly energetic astrophysical processes. With such high energies present, it is likely these astrophysical events will have signatures in the EM…

Astrophysics · Physics 2009-06-23 Jonah Kanner , Tracy L. Huard , Szabolcs Marka , David C. Murphy , Jennifer Piscionere , Molly Reed , Peter Shawhan

Maximizing the Probability of Detecting an Electromagnetic Counterpart of Gravitational-wave Events

Compact binary coalescences are a promising source of gravitational waves for second-generation interferometric gravitational-wave detectors such as advanced LIGO and advanced Virgo. These are among the most promising sources for joint…

Instrumentation and Methods for Astrophysics · Physics 2016-08-03 Michael W. Coughlin , Christopher W. Stubbs

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

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

GWOPS: A VO-technology Driven Tool to Search for the Electromagnetic Counterpart of Gravitational Wave Event

The search and follow-up observation of electromagnetic (EM) counterparts of gravitational waves (GW) is a current hot topic of GW cosmology. Due to the limitation of the accuracy of the GW observation facility at this stage, we can only…

Instrumentation and Methods for Astrophysics · Physics 2020-09-10 Yunfei Xu , Dong Xu , Chenzhou Cui , Dongwei Fan , Zipei Zhu , Bangyao Yu , Changhua Li , Jun Han , Linying Mi , Shanshan Li , Boliang He , Yihan Tao , Hanxi Yang , Sisi Yang

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

Search for Electromagnetic Counterparts to LIGO-Virgo Candidates: Expanded Very Large Array

This paper summarizes a search for radio wavelength counterparts to candidate gravitational wave events. The identification of an electromagnetic counterpart could provide a more complete understanding of a gravitational wave event,…

Instrumentation and Methods for Astrophysics · Physics 2015-06-04 Joseph Lazio , Katie Keating , F. A. Jenet , N. E. Kassim , the LIGO Scientific Collaboration , the Virgo Collaboration

Speed of Gravitational Waves from Strongly Lensed Gravitational Waves and Electromagnetic Signals

We propose a new model-independent measurement strategy for the propagation speed of gravitational waves (GWs) based on strongly lensed GWs and their electromagnetic (EM) counterparts. This can be done in two ways: by comparing arrival…

General Relativity and Quantum Cosmology · Physics 2017-04-05 Xi-Long Fan , Kai Liao , Marek Biesiada , Aleksandra Piorkowska-Kurpas , Zong-Hong Zhu

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

Finding and Using Electromagnetic Counterparts of Gravitational Wave Sources

The principal goal of this whitepaper is not so much to demonstrate that gravitational wave detectors like LIGO and LISA will help answer many central questions in astronomy and astrophysics, but to make the case that they can help answer a…

Cosmology and Nongalactic Astrophysics · Physics 2009-03-03 E. S. Phinney

Towards improving the prospects for coordinated gravitational-wave and electromagnetic observations

We discuss two approaches to searches for gravitational-wave (GW) and electromagnetic (EM) counterparts of binary neutron star mergers. The first approach relies on triggering archival searches of GW detector data based on detections of EM…

High Energy Astrophysical Phenomena · Physics 2015-06-03 Ilya Mandel , Luke Z. Kelley , Enrico Ramirez-Ruiz

GERry: A Code to Optimise the Hunt for the Electromagnetic Counter-parts to Gravitational Wave Events

The search for the electromagnetic counterparts to gravitational wave (GW) events has been rapidly gathering pace in recent years thanks to the increasing number and capabilities of both gravitational wave detectors and wide field survey…

Instrumentation and Methods for Astrophysics · Physics 2024-07-30 David O'Neill , Joseph Lyman , Kendall Ackley , Danny Steeghs , Duncan Galloway , Vik Dhillon , Paul O'Brien , Gavin Ramsay , Kanthanakorn Noysena , Rubina Kotak , Rene Breton , Laura Nuttall , Enric Pallé , Don Pollacco , Krzysztof Ulaczyk , Martin Dyer , Felipe Jiménez-Ibarra , Tom Killestein , Amit Kumar , Lisa Kelsey , Ben Godson , Dan Jarvis

Localizing gravitational wave sources with optical telescopes and combining electromagnetic and gravitational wave data

Neutron star binaries, which are among the most promising sources for the direct detection of gravitational waves (GW) by ground based detectors, are also potential electromagnetic (EM) emitters. Gravitational waves will provide a new…

General Relativity and Quantum Cosmology · Physics 2015-06-19 Shaon Ghosh , Gijs Nelemans

Where and when: optimal scheduling of the electromagnetic follow-up of gravitational-wave events based on counterpart lightcurve models

The electromagnetic (EM) follow-up of a gravitational wave (GW) event requires to scan a wide sky region, defined by the so called "skymap", for the detection and identification of a transient counterpart. We propose a novel method that…

High Energy Astrophysical Phenomena · Physics 2017-09-19 Om S. Salafia , Monica Colpi , Marica Branchesi , Eric Chassande-Mottin , Giancarlo Ghirlanda , Gabriele Ghisellini , Susanna Vergani

Electromagnetic follow-up of gravitational wave transient signal candidates

Pioneering efforts aiming at the development of multi-messenger gravitational wave and electromagnetic astronomy have been made. An electromagnetic observation follow-up program of candidate gravitational wave events has been performed (Dec…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 M. Branchesi

From Localization to Discovery: Bayesian Ranking of Electromagnetic Counterparts to Gravitational-Wave Events

The robust association of electromagnetic candidates discovered during follow-up of gravitational-wave alerts is challenging, not only due to the large sky areas and broad distance uncertainties, but also due to the tens to hundreds of…

High Energy Astrophysical Phenomena · Physics 2025-10-20 Kendall Ackley

Gravitational Waves and Electromagnetic Transients

The advanced gravitational wave (GW) detector network has started {routine detection of } signals from merging compact binaries. Data indicate that in a fair fraction of these sources, at least one component was a neutron star, bringing…

High Energy Astrophysical Phenomena · Physics 2022-09-29 Akshat Singhal , Sourav Palit , Suman Bala , Gaurav Waratkar , Harsh Kumar , Varun Bhalerao