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

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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Bibliographic Details
Main Authors: 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
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
High energy astrophysics
Time domain astronomy
Transient sources
Stellar mergers
Gravitational wave sources
Gravitational waves
Online Access:https://doi.org/10.3847/1538-4357/ad0238

Internet

https://doi.org/10.3847/1538-4357/ad0238

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