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Table 9:

$z_{\rm phot}$ accuracy derived from simulations for galaxies in the spectroscopic sample, based on the GR code.
Clusters Redshift interval Galaxy type $\langle \Delta_z \rangle$ $\sigma_z$ $\sigma_{z,\rm MAD}$ $\sigma (\Delta z/(1+z))$ $l\%$ $g\%$
Low-z 0.3 $\le$  $z_{\rm phot}$ $\le$ 1 all 0.008 0.150 0.104 0.063 0.9 7.7
High-z 0.3 $\le$  $z_{\rm phot}$  $\le$ 1 all -0.072 0.164 0.167 0.100 10.6 20.3
High-z 0.45 $\le$  $z_{\rm phot}$  $\le$ 1 all -0.092 0.158 0.151 0.088 6.5 21.5
Low-z 0.3 $\le$ $z_{\rm phot}$  $\le$ 1 E/S0 -0.140 0.129 0.184 0.110 4.2 6.3
    Sbc -0.077 0.117 0.136 0.082 0.8 9.9
    Scd 0.013 0.076 0.070 0.041 0.0 4.3
    Im 0.024 0.077 0.075 0.045 0.0 5.9
    SB 0.098 0.117 0.121 0.076 0.1 9.8
High-z 0.3 $\le$  $z_{\rm phot}$  $\le$ 1 E/S0 -0.227 0.153 0.370 0.226 12.2 31.6
    Sbc -0.101 0.161 0.232 0.134 17.3 28.0
    Scd -0.025 0.093 0.086 0.052 2.7 16.2
    Im 0.024 0.126 0.123 0.074 5.9 6.7
    SB -0.045 0.063 0.077 0.047 2.3 13.5

Notes: the accuracy reached for the different spectral types of galaxies is also presented. The information given is the same as in Table 4 and Table 1, for the current spectroscopic sample.

Source LaTeX | All tables | In the text

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