Measuring the Hubble constant with a sample of kilonovae

Kilonovae observations can be used to out constraints on the Hubble constant (H0). Here, the authors show H0 measurements by combining light curves of four short gamma-ray burts with GW170817 are about a factor of 2-3 more precise than the standard-siren measurements using only gravitational-waves.

Guardado en:
Detalles Bibliográficos
Autores principales: Michael W. Coughlin, Sarah Antier, Tim Dietrich, Ryan J. Foley, Jack Heinzel, Mattia Bulla, Nelson Christensen, David A. Coulter, Lina Issa, Nandita Khetan
Formato: article
Lenguaje:EN
Publicado: Nature Portfolio 2020
Materias:
Q
Acceso en línea:https://doaj.org/article/b1add878d9284675bd2674b4004eb31d
Etiquetas: Agregar Etiqueta
Sin Etiquetas, Sea el primero en etiquetar este registro!
id oai:doaj.org-article:b1add878d9284675bd2674b4004eb31d
record_format dspace
spelling oai:doaj.org-article:b1add878d9284675bd2674b4004eb31d2021-12-02T18:01:15ZMeasuring the Hubble constant with a sample of kilonovae10.1038/s41467-020-17998-52041-1723https://doaj.org/article/b1add878d9284675bd2674b4004eb31d2020-08-01T00:00:00Zhttps://doi.org/10.1038/s41467-020-17998-5https://doaj.org/toc/2041-1723Kilonovae observations can be used to out constraints on the Hubble constant (H0). Here, the authors show H0 measurements by combining light curves of four short gamma-ray burts with GW170817 are about a factor of 2-3 more precise than the standard-siren measurements using only gravitational-waves.Michael W. CoughlinSarah AntierTim DietrichRyan J. FoleyJack HeinzelMattia BullaNelson ChristensenDavid A. CoulterLina IssaNandita KhetanNature PortfolioarticleScienceQENNature Communications, Vol 11, Iss 1, Pp 1-9 (2020)
institution DOAJ
collection DOAJ
language EN
topic Science
Q
spellingShingle Science
Q
Michael W. Coughlin
Sarah Antier
Tim Dietrich
Ryan J. Foley
Jack Heinzel
Mattia Bulla
Nelson Christensen
David A. Coulter
Lina Issa
Nandita Khetan
Measuring the Hubble constant with a sample of kilonovae
description Kilonovae observations can be used to out constraints on the Hubble constant (H0). Here, the authors show H0 measurements by combining light curves of four short gamma-ray burts with GW170817 are about a factor of 2-3 more precise than the standard-siren measurements using only gravitational-waves.
format article
author Michael W. Coughlin
Sarah Antier
Tim Dietrich
Ryan J. Foley
Jack Heinzel
Mattia Bulla
Nelson Christensen
David A. Coulter
Lina Issa
Nandita Khetan
author_facet Michael W. Coughlin
Sarah Antier
Tim Dietrich
Ryan J. Foley
Jack Heinzel
Mattia Bulla
Nelson Christensen
David A. Coulter
Lina Issa
Nandita Khetan
author_sort Michael W. Coughlin
title Measuring the Hubble constant with a sample of kilonovae
title_short Measuring the Hubble constant with a sample of kilonovae
title_full Measuring the Hubble constant with a sample of kilonovae
title_fullStr Measuring the Hubble constant with a sample of kilonovae
title_full_unstemmed Measuring the Hubble constant with a sample of kilonovae
title_sort measuring the hubble constant with a sample of kilonovae
publisher Nature Portfolio
publishDate 2020
url https://doaj.org/article/b1add878d9284675bd2674b4004eb31d
work_keys_str_mv AT michaelwcoughlin measuringthehubbleconstantwithasampleofkilonovae
AT sarahantier measuringthehubbleconstantwithasampleofkilonovae
AT timdietrich measuringthehubbleconstantwithasampleofkilonovae
AT ryanjfoley measuringthehubbleconstantwithasampleofkilonovae
AT jackheinzel measuringthehubbleconstantwithasampleofkilonovae
AT mattiabulla measuringthehubbleconstantwithasampleofkilonovae
AT nelsonchristensen measuringthehubbleconstantwithasampleofkilonovae
AT davidacoulter measuringthehubbleconstantwithasampleofkilonovae
AT linaissa measuringthehubbleconstantwithasampleofkilonovae
AT nanditakhetan measuringthehubbleconstantwithasampleofkilonovae
_version_ 1718379009198260224