Measuring the Hubble constant with a sample of kilonovae

Kilonovae produced by the coalescence of compact binaries with at least one neutron star are promising standard sirens for an independent measurement of the Hubble constant (H(0)). Through their detection via follow-up of gravitational-wave (GW), short gamma-ray bursts (sGRBs) or optical surveys, a...

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Detalles Bibliográficos
Autores principales: Coughlin, Michael W., Antier, Sarah, Dietrich, Tim, Foley, Ryan J., Heinzel, Jack, Bulla, Mattia, Christensen, Nelson, Coulter, David A., Issa, Lina, Khetan, Nandita
Formato: Online Artículo Texto
Lenguaje:English
Publicado: Nature Publishing Group UK 2020
Materias:
Article
Acceso en línea:https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7431580/
https://www.ncbi.nlm.nih.gov/pubmed/32807780
http://dx.doi.org/10.1038/s41467-020-17998-5

Internet

https://www.ncbi.nlm.nih.gov/pmc/articles/PMC7431580/
https://www.ncbi.nlm.nih.gov/pubmed/32807780
http://dx.doi.org/10.1038/s41467-020-17998-5

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