RX J0911+05: A Massive Cluster Lens at z=0.769

dc.creatorKneib, Jean-Paul
dc.creatorCohen, Judith G.
dc.creatorHjorth, Jens
dc.date2000-06-08
dc.date.accessioned2026-07-07T01:53:54Z
dc.date.available2026-07-07T01:53:54Z
dc.descriptionWe report the detection of a massive high-redshift cluster of galaxies near the quadruple quasar RX J0911+05, using the LRIS instrument on the Keck-II telescope. The cluster is found to have a mean redshift of <z>=0.7689+/-0.002 and a velocity dispersion of sigma=836{+180-200} km/s, based on redshift measurements for 24 member galaxies. This massive high-redshift cluster is the origin of the unusually large external shear required by lensing models of the quadruple quasar system. We predict the expected time delay depending on the exact contribution of the cluster. A measurement of the time delay and further deep lensing and X-ray observations will unravel useful properties of this serendipitously discovered high-redshift cluster, and may put interesting cosmological constraints on H0.
dc.descriptionSubmitted to ApJL, 7 pages, 5 figures
dc.identifierhttps://arxiv.org/abs/astro-ph/0006106
dc.identifierhttp://arxiv.org/abs/astro-ph/0006106
dc.identifierAstrophys.J. 544 (2000) L35-L39
dc.identifierdoi:10.1086/317285
dc.identifier.urihttp://salesiana.dossiersoluciones.com/handle/123456789/1138
dc.subjectAstrophysics
dc.titleRX J0911+05: A Massive Cluster Lens at z=0.769
dc.typetext

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