The universal Einstein radius distribution from 10 000 SDSS clusters

We present results from strong-lens modelling of 10,000 SDSS clusters, to estab-lish the universal distribution of Einstein radii. Detailed lensing analyses have shown that the inner mass distribution of clusters can be accurately modelled by assuming light traces mass, successfully uncovering large numbers of multiple-images. Approx-imate critical curves and the effective Einstein radius of each cluster can therefore be readily calculated, from the distribution of member galaxies and scaled by their luminosities. We use a subsample of 10 well-studied clusters covered by both SDSS and HST to calibrate and test this method, and show that an accurate determina-tion of the Einstein radius and mass can be achieved by this approach “blindly”, in an automated way, and without requiring multiple images as input. We present the results of the first 10,000 clusters analysed in the range 0.1 < z < 0.55, and compare them to theoretical expectations. We find that for this all-sky representative sample the Einstein radius distribution is log-normal in shape, with 〈Log(θe′′) 〉 = 0.73+0.02−0.03, σ = 0.316+0.004−0.002, and with higher abundance of large θe clusters than predicted by

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