Fig. 6.
Multiplicative bias μ as a function of seeing for simulated galaxies with 20 < i < 22.5. The red points correspond to the KSB estimates, which are significantly biased and depend upon image quality. The corrected biases are shown as grey (per-galaxy bias correction) and black (seeing-averaged bias correction) points. The histogram shows the seeing distribution for the CFHTLS W3 data.
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