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Field Parameter u ∗ g r i y z<br />

W1 Nb stacks 72 72 72 56 16 72<br />

Seeing ["] 0.84 ± 0.11 0.77 ± 0.10 0.70 ± 0.07 0.65 ± 0.08 0.66 ± 0.10 0.69 ± 0.13<br />

80% Compl. (stellar) 25.27 ± 0.21 25.52 ± 0.18 25.03 ± 0.16 24.73 ± 0.18 24.82 ± 0.22 23.90 ± 0.26<br />

80% Compl. (extended) 24.45 ± 0.15 24.67 ± 0.14 24.00 ± 0.10 23.69 ± 0.13 23.78 ± 0.20 22.91 ± 0.15<br />

Int. astrom. err. (0.031",0.029") (0.031",0.029") (0.025",0.022") (0.020",0.017") (0.020",0.017") (0.025",0.022")<br />

Ext. astrom. err. (0.237",0.227") (0.254",0.244") (0.259",0.247") (0.252",0.243") (0.272",0.254") (0.260",0.247")<br />

Mag. err. [mag.] 0.05 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.04 ± 0.01<br />

CFHTLS-SDSS 〈δm〉 [mag.] −0.020 ± 0.015 +0.003 ± 0.006 +0.041 ± 0.014 +0.000 ± 0.007 −0.002 ± 0.008 +0.015 ± 0.011<br />

W2 Nb stacks 25 25 25 23 2 25<br />

Seeing ["] 0.88 ± 0.10 0.79 ± 0.08 0.72 ± 0.09 0.64 ± 0.08 0.59 ± 0.05 0.72 ± 0.09<br />

80% Compl. (stellar) 25.16 ± 0.20 25.51 ± 0.18 25.04 ± 0.18 24.81 ± 0.13 24.96 ± 0.15 23.88 ± 0.16<br />

80% Compl. (extended) 24.36 ± 0.17 24.66 ± 0.16 24.00 ± 0.13 23.76 ± 0.10 23.84 ± 0.09 22.94 ± 0.11<br />

Int. astrom. err. (0.024",0.021") (0.024",0.021") (0.024",0.021") (0.024",0.021") (0.024",0.021") (0.024",0.021")<br />

Ext. astrom. err. (0.183",0.186") (0.208",0.211") (0.211",0.213") (0.207",0.210") (0.224",0.228") (0.211",0.212")<br />

Mag. err. [mag.] 0.05 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.04 ± 0.01<br />

CFHTLS-SDSS 〈δm〉 [mag.] −0.040 ± 0.011 −0.008 ± 0.005 +0.007 ± 0.004 −0.007 ± 0.005 – +0.018 ± 0.012<br />

W3 Nb stacks 49 49 49 42 7 42<br />

Seeing ["] 0.85 ± 0.11 0.81 ± 0.09 0.75 ± 0.08 0.66 ± 0.08 0.59 ± 0.08 0.67 ± 0.09<br />

80% Compl. (stellar) 25.20 ± 0.22 25.48 ± 0.16 24.99 ± 0.15 24.67 ± 0.16 24.95 ± 0.15 23.93 ± 0.22<br />

80% Compl. (extended) 24.35 ± 0.21 24.64 ± 0.12 23.98 ± 0.10 23.63 ± 0.12 23.89 ± 0.11 22.92 ± 0.17<br />

Int. astrom. err. (0.036",0.035") (0.036",0.035") (0.036",0.035") (0.036",0.035") (0.036",0.035") (0.036",0.035")<br />

Ext. astrom. err. (0.235",0.225") (0.248",0.242") (0.258",0.249") (0.246",0.242") (0.275",0.269") (0.258",0.250")<br />

Mag. err. [mag.] 0.05 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.04 ± 0.01<br />

CFHTLS-SDSS 〈δm〉 [mag.] −0.012 ± 0.009 +0.003 ± 0.004 +0.010 ± 0.005 −0.013 ± 0.004 +0.000 ± 0.004 +0.001 ± 0.005<br />

W4 Nb stacks 25 25 25 18 7 25<br />

Seeing ["] 0.81 ± 0.11 0.75 ± 0.06 0.67 ± 0.07 0.61 ± 0.07 0.59 ± 0.06 0.64 ± 0.10<br />

80% Compl. (stellar) 25.22 ± 0.21 25.57 ± 0.17 25.02 ± 0.16 24.81 ± 0.19 24.97 ± 0.11 23.91 ± 0.20<br />

80% Compl. (extended) 24.35 ± 0.17 24.71 ± 0.15 23.94 ± 0.12 23.73 ± 0.19 23.88 ± 0.08 22.90 ± 0.13<br />

Int. astrom. err. (0.023",0.020") (0.023",0.020") (0.023",0.020") (0.023",0.020") (0.023",0.020") (0.023",0.020")<br />

Ext. astrom. err. (0.193",0.186") (0.218",0.213") (0.222",0.217") (0.217",0.215") (0.221",0.217") (0.214",0.212")<br />

Mag. err. [mag.] 0.05 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.03 ± 0.01 0.04 ± 0.01<br />

CFHTLS-SDSS 〈δm〉 [mag.] −0.030 ± 0.009 +0.009 ± 0.003 +0.010 ± 0.007 −0.001 ± 0.006 – +0.022 ± 0.005<br />

Table 6: Summary of the W1, W2, W3 and W4 mean survey parameters. The i and y data have been combined. "80% Compl." is the 80% completeness limit.<br />

The seeing is the median FWHM and the errors is the field-to-field scatter. Astrometric errors are given along the two (X,Y)=(NS,EW) axes. The internal astrometric<br />

errors are from the (global) astrometric calibration errors step; the external astrometric errors are from the (ensemble average) astrometric accuracy of CFHTLS stacks.<br />

The "CFHTLS-SDSS 〈δm〉 mag." denotes the mean magnitude offset between the CFHTLS and the SDSS surveys, averaged over a Wide field. It is derived from a sample of<br />

common stars to both surveys in W1, W3 and W4 (no data for W2). The "Mag. err." is estimated from the external and internal magnitude errors discussed in the<br />

document. For W2, it is based on the internal mag. error and extrapolated from the W1, W3 and W4 CFHTLS-SDSS comparisons.<br />

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