Rapid Generation of Kilonova Light Curves Using Conditional Variational Autoencoder

The discovery of the optical counterpart, along with the gravitational waves (GWs) from GW170817, of the first binary neutron star merger has opened up a new era for multimessenger astrophysics. Combining the GW data with the optical counterpart, also known as AT 2017gfo and classified as a kilonova...

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Veröffentlicht in:	The Astrophysical journal Jg. 961; H. 2; S. 165 - 178
Hauptverfasser:	Saha, Surojit, Williams, Michael J., Datrier, Laurence, Hayes, Fergus, Nicholl, Matt, Kong, Albert K. H., Hendry, Martin, Heng, IK Siong, Lamb, Gavin P., Lin, En-Tzu, Williams, Daniel
Format:	Journal Article
Sprache:	Englisch
Veröffentlicht:	Philadelphia The American Astronomical Society 01.02.2024 IOP Publishing
Schlagworte:	Astronomy Astrophysics Binary stars Compact objects Equations of state Gravitational waves Kilonovae Light Light curve Light curves Neural networks Neutron stars Neutrons Optical counterparts (astronomy) Parameters Physical properties Star mergers
ISSN:	0004-637X, 1538-4357
Online-Zugang:	Volltext
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