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COSMOGRAIL: Measuring Time Delays of Gravitationally Lensed Quasars to Constrain Cosmology

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dc.contributor.author Tewes, M
dc.contributor.author Courbin, F
dc.contributor.author Meylan, G
dc.contributor.author Kochanek, C. S
dc.contributor.author Eulaers, E
dc.contributor.author Cantale, N
dc.contributor.author Mosquera, A. M
dc.contributor.author Asfandiyarov, I
dc.contributor.author Magain, P
dc.contributor.author Van Winckel, H
dc.contributor.author Sluse, D
dc.contributor.author Keerthi, R. K. S
dc.contributor.author Stalin, C. S
dc.contributor.author Prabhu, T. P
dc.contributor.author Saha, P
dc.contributor.author Dye, S
dc.date.accessioned 2013-04-26T11:38:25Z
dc.date.available 2013-04-26T11:38:25Z
dc.date.issued 2012-12
dc.identifier.citation The Messenger, Vol. 150, pp. 49-52 en
dc.identifier.issn 1209-7233
dc.identifier.uri http://hdl.handle.net/2248/6035
dc.description Open Access en
dc.description.abstract COSMOGRAIL is a long-term programme for the photometric monitoring of gravitationally lensed quasars. It makes use of several medium-size telescopes to derive long and well-sampled light curves of lensed quasars, in order to measure the time delays between the quasar images. These delays directly relate to the Hubble constant H0, without any need for secondary distance calibrations. COSMOGRAIL was initiated in 2004, and has now secured almost a decade of data, resulting in cosmological constraints that are very complementary to other cosmological probes. en
dc.language.iso en en
dc.publisher ESO en
dc.relation.uri http://www.eso.org/sci/publications/messenger/archive/no.150-dec12/messenger-no150-49-52.pdf en
dc.rights © ESO en
dc.title COSMOGRAIL: Measuring Time Delays of Gravitationally Lensed Quasars to Constrain Cosmology en
dc.type Article en


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