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Fig. 10

image

Magnification measurements of the dropout high-z galaxies found and analyzed by Hall et al. (2012). We find that average magnification of those dropouts estimated by our mass model is 43% smaller than predicated by Hall et al. (2012). This is expected since high redshift critical lines of our mass model lie closer to the center of the cluster than those of Bradač et al. (2009).

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