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We present a cadence optimization strategy to unveil a large population of kilonovae using optical imaging alone. These transients are generated during binary neutron star and potentially neutron star-black hole mergers and are…

Kilonovae, the ultraviolet/optical/infrared counterparts to binary neutron star mergers, are an exceptionally rare class of transients. Optical follow-up campaigns are plagued by contaminating transients, which may mimic kilonovae, but do…

Gravitational waves were discovered with the detection of binary black hole mergers and they should also be detectable from lower mass neutron star mergers. These are predicted to eject material rich in heavy radioactive isotopes that can…

High Energy Astrophysical Phenomena · Physics 2017-10-18 S. J. Smartt , T. -W. Chen , A. Jerkstrand , M. Coughlin , E. Kankare , S. A. Sim , M. Fraser , C. Inserra , K. Maguire , K. C. Chambers , M. E. Huber , T. Kruhler , G. Leloudas , M. Magee , L. J. Shingles , K. W. Smith , D. R. Young , J. Tonry , R. Kotak , A. Gal-Yam , J. D. Lyman , D. S. Homan , C. Agliozzo , J. P. Anderson , C. R. Angus C. Ashall , C. Barbarino , F. E. Bauer , M. Berton , M. T. Botticella , M. Bulla , J. Bulger , G. Cannizzaro , Z. Cano , R. Cartier , A. Cikota , P. Clark , A. De Cia , M. Della Valle , L. Denneau , M. Dennefeld , L. Dessart , G. Dimitriadis , N. Elias-Rosa , R. E. Firth , H. Flewelling , A. Flors , A. Franckowiak , C. Frohmaier , L. Galbany , S. Gonzalez-Gaitan , J. Greiner , M. Gromadzki , A. Nicuesa Guelbenzu , C. P. Gutierrez , A. Hamanowicz , L. Hanlon , J. Harmanen , K. E. Heintz , A. Heinze , M. -S. Hernandez , S. T. Hodgkin , I. M. Hook , L. Izzo , P. A. James , P. G. Jonker , W. E. Kerzendorf , S. Klose , Z. Kostrzewa-Rutkowska , M. Kowalski , M. Kromer , H. Kuncarayakti , A. Lawrence , T. B. Lowe , E. A. Magnier , I. Manulis , A. Martin-Carrillo , S. Mattila , O. McBrien , A. Muller , J. Nordin , D. O'Neill , F. Onori , J. T. Palmerio , A. Pastorello , F. Patat , G. Pignata , Ph. Podsiadlowski , M. L. Pumo , S. J. Prentice , A. Rau , A. Razza , A. Rest , T. Reynolds , R. Roy , A. J. Ruiter , K. A. Rybicki , L. Salmon , P. Schady , A. S. B. Schultz , T. Schweyer , I. R. Seitenzahl , M. Smith , J. Sollerman , B. Stalder , C. W. Stubbs , M. Sullivan , H. Szegedi , F. Taddia , S. Taubenberger , G. Terreran , B. van Soelen , J. Vos , R. J. Wainscoat , N. A. Walton , C. Waters , H. Weiland , M. Willman , P. Wiseman , D. E. Wright , L. Wyrzykowski , O. Yaron

The mergers of double neutron star (NS-NS) and black hole (BH)-NS binaries are promising gravitational wave (GW) sources for Advanced LIGO and future GW detectors. The neutron-rich ejecta from such merger events undergoes rapid neutron…

High Energy Astrophysical Phenomena · Physics 2017-07-19 Brian D. Metzger

The third observing run of the LIGO-Virgo collaboration has resulted in about hundred gravitational-wave triggers including the binary neutron star merger GW190425. However, none of these events have been accompanied with an electromagnetic…

We present the results from a search for the electromagnetic counterpart of the LIGO/Virgo event S190510g using the Dark Energy Camera (DECam). S190510g is a binary neutron star (BNS) merger candidate of moderate significance detected at a…

An advanced LIGO and Virgo's third observing run brought another binary neutron star merger (BNS) and the first neutron-star black hole mergers. While no confirmed kilonovae were identified in conjunction with any of these events, continued…

Kilonovae are the scientifically rich, but observationally elusive, optical transient phenomena associated with compact binary mergers. Only a handful of events have been discovered to date, all through multi-wavelength (gamma ray) and…

We present Very Large Array (VLA) and Atacama Large Millimeter/sub-millimeter Array ALMA radio observations of GW\,170817, the first Laser Interferometer Gravitational-wave Observatory (LIGO)/Virgo gravitational wave (GW) event from a…

With the epochal first detection of gravitational waves from a binary neutron star (NS) merger with the GW170817 event, and its direct confirmation that NS-NS mergers are significant sources of the of the r-process nucleosynthesis of heavy…

Searches for electromagnetic counterparts of gravitational-wave signals have redoubled since the first detection in 2017 of a binary neutron star merger with a gamma-ray burst, optical/infrared kilonova, and panchromatic afterglow. Yet, one…

We present near-infrared follow-up observations of the International Gravitational Wave Network (IGWN) event S250206dm with the Wide-Field Infrared Transient Explorer (WINTER). WINTER is a near-infrared time-domain survey designed for…

Current and future optical and near-infrared wide-field surveys have the potential of finding kilonovae, the optical and infrared counterparts to neutron star mergers, independently of gravitational-wave or high-energy gamma-ray burst…

GW190425 was the second gravitational wave (GW) signal compatible with a binary neutron star (BNS) merger detected by the Advanced LIGO and Advanced Virgo detectors. Since no electromagnetic counterpart was identified, whether the…

High Energy Astrophysical Phenomena · Physics 2024-01-25 A. Camilletti , L. Chiesa , G. Ricigliano , A. Perego , L. C. Lippold , S. Padamata , S. Bernuzzi , D. Radice , D. Logoteta , F. M. Guercilena

On 2019 August 14, the LIGO and Virgo interferometers detected a high-significance event labelled S190814bv. Preliminary analysis of the GW data suggests that the event was likely due to the merger of a compact binary system formed by a BH…

Solar and Stellar Astrophysics · Physics 2020-11-11 K. Ackley , L. Amati , C. Barbieri , F. E. Bauer , S. Benetti , M. G. Bernardini , K. Bhirombhakdi , M. T. Botticella , M. Branchesi , E. Brocato , S. H. Bruun , M. Bulla , S. Campana , E. Cappellaro , A. J. Castro-Tirado , K. C. Chambers , S. Chaty , T. -W. Chen , R. Ciolfi , A. Coleiro , C. M. Copperwheat , S. Covino , R. Cutter , F. D'Ammando , P. D'Avanzo , G. De Cesare , V. D'Elia , M. Della Valle , L. Denneau , M. De Pasquale , V. S. Dhillon , M. J. Dyer , N. Elias-Rosa , P. A. Evans , R. A. J. Eyles-Ferris , A. Fiore , M. Fraser , A. S. Fruchter , J. P. U. Fynbo , L. Galbany , C. Gall , D. K. Galloway , F. I. Getman , G. Ghirlanda , J. H. Gillanders , A. Gomboc , B. P. Gompertz , C. González-Fernández , S. González-Gaitán , A. Grado , G. Greco , M. Gromadzki , P. J. Groot , C. P. Gutiérrez , T. Heikkilä , K. E. Heintz , J. Hjorth , Y. -D. Hu , M. E. Huber , C. Inserra , L. Izzo , J. Japelj , A. Jerkstrand , Z. P. Jin , P. G. Jonker , E. Kankare , D. A. Kann , M. Kennedy , S. Kim , S. Klose , E. C. Kool , R. Kotak , H. Kuncarayakti , G. P. Lamb , G. Leloudas , A. J. Levan , F. Longo , T. B. Lowe , J. D. Lyman , E. Magnier , K. Maguire , E. Maiorano , I. Mandel , M. Mapelli , S. Mattila , O. R. McBrien , A. Melandri , M. J. Michałowski , B. Milvang-Jensen , S. Moran , L. Nicastro , M. Nicholl , A. Nicuesa Guelbenzu , L. Nuttal , S. R. Oates , P. T. O'Brien , F. Onori , E. Palazzi , B. Patricelli , A. Perego , M. A. P. Torres , D. A. Perley , E. Pian , G. Pignata , S. Piranomonte , S. Poshyachinda , A. Possenti , M. L. Pumo , J. Quirola-Vásquez , F. Ragosta , G. Ramsay , A. Rau , A. Rest , T. M. Reynolds , S. S. Rosetti , A. Rossi , S. Rosswog , N. B. Sabha , A. Sagués Carracedo , O. S. Salafia , L. Salmon , R. Salvaterra , S. Savaglio , L. Sbordone , P. Schady , P. Schipani , A. S. B. Schultz , T. Schweyer , S. J. Smartt , K. W. Smith , M. Smith , J. Sollerman , S. Srivastav , E. R. Stanway , R. L. C. Starling , D. Steeghs , G. Stratta , C. W. Stubbs , N. R. Tanvir , V. Testa , E. Thrane , J. L. Tonry , M. Turatto , K. Ulaczyk , A. J. van der Horst , S. D. Vergani , N. A. Walton , D. Watson , K. Wiersema , K. Wiik , L. Wyrzykowski , S. Yang , S. -X. Yi , D. R. Young

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

We present a subthreshold search for gravitational-wave inspirals from binary neutron stars using data from the first part of the fourth observing run of the LIGO-Virgo-KAGRA Collaboration. To enhance sensitivity to this targeted…

The detection of the gravitational wave event GW230529, presumably a neutron star-black hole (NSBH) merger, by the LIGO-Virgo-KAGRA (LVK) Collaboration marks an exciting discovery for multimessenger astronomy. The black hole (BH) has a high…

High Energy Astrophysical Phenomena · Physics 2025-10-14 Keerthi Kunnumkai , Antonella Palmese , Mattia Bulla , Tim Dietrich , Amanda M. Farah , Peter T. H. Pang

Binary neutron star mergers and neutron star-black hole mergers are multi-messenger sources that can be detected in gravitational waves and in electromagnetic radiation. The low electron fraction of neutron star merger ejecta favors the…