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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 4.

ACS image reconstruction of the most probable model with a source grid of 64 × 64 pixels. Top left: observed ACS F814W image. Top middle: predicted lensed image of the background AGN host galaxy. Top right: predicted light of the lensed AGNs and the lens galaxies. Bottom left: predicted image from all components, which is a sum of the top-middle and top-right panels. Bottom middle: image residual, normalized by the estimated 1σ uncertainty of each pixel. Bottom right: the reconstructed host galaxy of the AGN in the source plane. Our lens model reproduces the global features of the data.

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