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Two Accurate Time-delay Distances from Strong Lensing: Implications for Cosmology

  • Authors: S. H. Suyu, M. W. Auger, S. Hilbert, P. J. Marshall, M. Tewes, T. Treu, C. D. Fassnacht, L. V. E. Koopmans, D. Sluse, R. D. Blandford, F. Courbin, and G. Meylan

Suyu et al. 2013 The Astrophysical Journal 766 70.

  • Provider: AAS Journals

Caption: Figure 6.

Effective prior probability distribution for the external convergence κ ext from combining ray tracing through the Millennium Simulation with (1) the galaxy count around the lens system relative to the average number of galaxy counts, and/or (2) the modeled external shear of 0.089  ±  0.006. Dashed line: the convergence distribution for all lines of sight; dot-dashed line: the convergence distribution for lines of sight with relative galaxy count n r = 1.4  ±  0.05; dotted line: the convergence distribution for all lines of sight weighted by the likelihood for γ ext from the lens model; solid line: the γ ext-weighted convergence distribution for lines of sight with n r = 1.4  ±  0.05. The effective prior for κ ext used in the final cosmological parameter inference is described by this most informative distribution.

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