GECKO: Network of Telescopes and Follow-up Observation of GW190425

GW190425 is the second gravitational wave (GW) event caused by a binary neutron star (BNS) merger. We report the result of the follow-up observation of GW190425 by the Gravitational-wave Electromagnetic-wave (EM) Counterpart Korean Observatory (GECKO). Our observation demonstrates that GECKO can det...

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Published in:Proceedings of the International Astronomical Union 2020-06, Vol.16 (S363), p.356-357
Main Authors: Paek, Gregory S.H., Im, Myungshin, Kim, Joonho, Lim, Gu
Format: Article
Language:English
Subjects:
Astronomy
Binary stars
Geckos
Gravitational waves
Neutron stars
Poster Paper
Telescopes
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creator Paek, Gregory S.H.
Im, Myungshin
Kim, Joonho
Lim, Gu
description GW190425 is the second gravitational wave (GW) event caused by a binary neutron star (BNS) merger. We report the result of the follow-up observation of GW190425 by the Gravitational-wave Electromagnetic-wave (EM) Counterpart Korean Observatory (GECKO). Our observation demonstrates that GECKO can detect EM counterpart of a GW170817-like event.
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subjects Astronomy
Binary stars
Geckos
Gravitational waves
Neutron stars
Poster Paper
Telescopes
title GECKO: Network of Telescopes and Follow-up Observation of GW190425
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