Statistics of Quasars Multiply Imaged by Galaxy Clusters

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, , Citation Joseph F. Hennawi et al 2007 ApJ 654 93 DOI 10.1086/509094

0004-637X/654/1/93

Abstract

We compute the expected number of quasars multiply imaged by cluster-size dark halos for current wide-field quasar surveys by carrying out a large ensemble of ray-tracing simulations through clusters from a cosmological N-body simulation of the ΛCDM cosmology, with power spectrum normalization σ8 = 0.95. Our calculation predicts ~4 quasar lenses with splittings θ > 10'' in the SDSS spectroscopic quasar sample, consistent with the recent discovery of the wide separation lens SDSS J1004+4112, which has θ = 14.6''. The SDSS faint photometric quasar survey will contain ~12 multiply imaged quasars with splittings θ > 10''. Of these, ~2 will be lenses with θ > 30'', and ~2 will be at high redshift (zs ~ 4).

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10.1086/509094