TY - JOUR

T1 - The universal Einstein radius distribution from 10000 SDSS clusters

AU - Zitrin, Adi

AU - Broadhurst, Tom

AU - Bartelmann, Matthias

AU - Rephaeli, Yoel

AU - Oguri, Masamune

AU - Benítez, Narciso

AU - Hao, Jiangang

AU - Umetsu, Keiichi

PY - 2012/7

Y1 - 2012/7

N2 - We present results from strong lens modelling of 10000 Sloan Digital Sky Survey (SDSS) clusters, to establish 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. Approximate 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 Hubble Space Telescope (HST) to calibrate and test this method, and show that an accurate determination 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 10000 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 lognormal in shape, with , , and with higher abundance of large θe clusters than predicted by Λ cold dark matter. We visually inspect each of the clusters with (zs= 2) and find that ~20 percent are boosted by various projection effects detailed here, remaining with ~40 real giant-lens candidates, with a maximum of (zs= 2) for the most massive candidate, in agreement with semi-analytic calculations. The results of this work should be verified further when an extended calibration sample is available.

AB - We present results from strong lens modelling of 10000 Sloan Digital Sky Survey (SDSS) clusters, to establish 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. Approximate 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 Hubble Space Telescope (HST) to calibrate and test this method, and show that an accurate determination 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 10000 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 lognormal in shape, with , , and with higher abundance of large θe clusters than predicted by Λ cold dark matter. We visually inspect each of the clusters with (zs= 2) and find that ~20 percent are boosted by various projection effects detailed here, remaining with ~40 real giant-lens candidates, with a maximum of (zs= 2) for the most massive candidate, in agreement with semi-analytic calculations. The results of this work should be verified further when an extended calibration sample is available.

KW - Cosmology: observations

KW - Cosmology: theory

KW - Dark matter

KW - Galaxies: clusters: general

KW - Galaxies: luminosity function, mass function

KW - Gravitational lensing: strong

UR - http://www.scopus.com/inward/record.url?scp=85028093642&partnerID=8YFLogxK

U2 - 10.1111/j.1365-2966.2012.21041.x

DO - 10.1111/j.1365-2966.2012.21041.x

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AN - SCOPUS:85028093642

SN - 0035-8711

VL - 423

SP - 2308

EP - 2324

JO - Monthly Notices of the Royal Astronomical Society

JF - Monthly Notices of the Royal Astronomical Society

IS - 3

ER -