Gravitational-wave Electromagnetic Counterpart Korean Observatory (GECKO): GECKO Follow-up Observation of GW190425

One of the keys to the success of multimessenger astronomy is the rapid identification of the electromagnetic wave counterpart, kilonova (KN), of the gravitational-wave (GW) event. Despite its importance, it is hard to find a KN associated with a GW event, due to a poorly constrained GW localization...

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Главные авторы:	Gregory S. H. Paek, Myungshin Im, Joonho Kim, Gu Lim, Bomi Park, Changsu Choi, Sophia Kim, Claudio Barbieri, Om Sharan Salafia, Insu Paek, Suhyun Shin, Jinguk Seo, Hyung Mok Lee, Chung-Uk Lee, Seung-Lee Kim, Hyun-Il Sung
Формат:	Artigo
Язык:	Inglês
Опубликовано:	IOP Publishing 2024-01-01
Серии:	The Astrophysical Journal
Предметы:	High energy astrophysics Time domain astronomy Transient sources Stellar mergers Gravitational wave sources Gravitational waves
Online-ссылка:	https://doi.org/10.3847/1538-4357/ad0238
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