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Please use this identifier to cite or link to this item: http://hdl.handle.net/20.500.12128/7158
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dc.contributor.authorBiesiada, Marek-
dc.contributor.authorPiórkowska, Aleksandra-
dc.contributor.authorMalec, Beata-
dc.date.accessioned2018-11-20T13:07:54Z-
dc.date.available2018-11-20T13:07:54Z-
dc.date.issued2011-
dc.identifier.citationActa Physica Polonica B, Vol. 42, no. 11 (2011), s. 2287-2295pl_PL
dc.identifier.issn0587-4254-
dc.identifier.urihttp://hdl.handle.net/20.500.12128/7158-
dc.description.abstractThe accelerating expansion of the Universe is a great challenge for both physics and cosmology. From the observational point of view, it is crucial to have various methods to assess cosmic expansion history, which can be alternative to standard candles (SNIa in cosmological context). Strongly gravitationally lensed systems create such a new opportunity by combining stellar kinematics with lensing geometry. Using strong gravitational lenses as probes of cosmic expansion is becoming attractive in light of ongoing surveys like SLACS based on different protocols than older searches focused on potential sources. In this approach, pursued recently by the authors, strongly lensed systems with known central velocity dispersions act as “standard rulers” — Einstein radius being standardized by stellar kinematics.pl_PL
dc.language.isoenpl_PL
dc.rightsUznanie autorstwa 3.0 Polska*
dc.rights.urihttp://creativecommons.org/licenses/by/3.0/pl/*
dc.subjectsoczewki grawitacyjnepl_PL
dc.subjectkosmologiapl_PL
dc.subjectstała Hubble'apl_PL
dc.titleGravitational Lenses as Standard Rulers in Cosmologypl_PL
dc.typeinfo:eu-repo/semantics/articlepl_PL
dc.identifier.doi10.5506/APhysPolB.42.2287-
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