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dc.contributor.authorDiego Rodríguez, José María 
dc.contributor.authorGoicoechea Santamaría, Luis Julián 
dc.contributor.authorMartínez Arrizabalaga, Joseba
dc.contributor.otherUniversidad de Cantabriaes_ES
dc.date.accessioned2024-04-30T17:39:19Z
dc.date.available2024-04-30T17:39:19Z
dc.date.issued2024-02
dc.identifier.issn0004-6361
dc.identifier.issn1432-0746
dc.identifier.otherPID2020- 118990GB-I00es_ES
dc.identifier.urihttps://hdl.handle.net/10902/32717
dc.description.abstractWe present a free-form lens model for the multiply lensed quasar in the galaxy cluster SDSS J1004+4112. Our lens model draws minimal assumptions on the distribution of mass in the lens plane. We have paid particular attention to the model uncertainties on the predicted time delay originating from the particular configuration of model variables. Taking into account this uncertainty, we obtained a value of the Hubble constant of H₀ = 74+⁹−₁₃ km s−¹ Mpc−¹, which is consistent with recent independent estimates. The predicted time delay between the central image E and image C (the first to arrive) is ∆TE−C = 3200 ± 200 days for the estimated Hubble constant. Future measurements of ∆TE−C will allow for a tighter constraint to be imposed on H0 in this cluster-QSO system.es_ES
dc.description.sponsorshipLuis J. Goicoechea acknowledges the support from the grant PID2020-118990GB-I00 funded by MCIN/AEI/10.13039/501100011033.es_ES
dc.format.extent7 p.es_ES
dc.language.isoenges_ES
dc.publisherEDP Scienceses_ES
dc.rightsOpen Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.es_ES
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/*
dc.sourceAstronomy and Astrophysics, 2024, 682, A187es_ES
dc.subject.otherGravitationes_ES
dc.subject.otherGravitational lensing: stronges_ES
dc.subject.otherMethods: statisticales_ES
dc.subject.otherGalaxies: clusters: individual: SDSS J1004+4112es_ES
dc.subject.otherCosmological parameterses_ES
dc.subject.otherCosmology: theoryes_ES
dc.titleParameter-free Hubble constant from the quadruply lensed quasar SDSS J1004+4112es_ES
dc.typeinfo:eu-repo/semantics/articlees_ES
dc.relation.publisherVersionhttps://doi.org/10.1051/0004-6361/202348066es_ES
dc.rights.accessRightsopenAccesses_ES
dc.identifier.DOI10.1051/0004-6361/202348066
dc.type.versionpublishedVersiones_ES


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Mostrar el registro sencillo

Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.Excepto si se señala otra cosa, la licencia del ítem se describe como Open Access article, published by EDP Sciences, under the terms of the Creative Commons Attribution License (https://creativecommons.org/licenses/by/4.0), which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited. This article is published in open access under the Subscribe to Open model. Subscribe to A&A to support open access publication.