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Fig. 19
Comparison between the template-fitting method and the neural network for CFHTLS data. The bias, the rms of the distribution of Δz / (1 + zs), and the parameter η are displayed as functions of the true redshift for the CFHTLS data. Data points are reported only if the number of galaxies in the sample is greater than ten.
This figure is made of several images, please see below:
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