Arnouts et al. (2001) astro-ph/0103071 (ESO Chandra) I_AB [2-15] 16.80 1.76 17.30 1.78 17.80 2.18 18.30 2.29 18.80 2.56 19.30 2.75 19.80 2.99 20.30 3.21 20.80 3.43 21.30 3.59 21.80 3.73 22.30 3.87 22.80 4.02 23.30 4.15 SLOAN Commissioning Yasuda et al (2001) astro-ph/0105545 i* [18-31] 13.25 -0.574 0.05 0.05 13.75 -0.372 0.04 0.04 14.25 0.120 0.02 0.02 14.75 0.401 0.01 0.01 15.25 0.636 0.01 0.01 15.75 0.955 0.01 0.01 16.25 1.226 0.01 0.01 16.75 1.507 0.01 0.01 17.25 1.766 0.01 0.01 17.75 2.026 0.01 0.01 18.25 2.268 0.01 0.01 18.75 2.503 0.01 0.01 19.25 2.718 0.01 0.01 19.75 2.913 0.01 0.01 20.25 3.048 0.01 0.01 WHDF 16x16 I-band assuming 7.25x10-2 sq.deg. i_ab=I+0.5 [35-48] 17.75 2.219 18.25 2.538 18.75 2.617 19.25 2.918 19.75 3.074 20.25 3.226 20.75 3.341 21.25 3.546 21.75 3.687 22.25 3.801 22.75 3.973 23.25 4.119 23.75 4.214 24.25 3.941 Capak et al. (2004) I_AB [51-63] 19.25 2.53 0.05 0.06 19.75 2.76 0.04 0.04 20.25 3.08 0.03 0.03 20.75 3.32 0.02 0.02 21.25 3.49 0.02 0.02 21.75 3.70 0.01 0.01 22.25 3.88 0.01 0.01 22.75 4.04 0.01 0.01 23.25 4.18 0.01 0.01 23.75 4.35 0.01 0.01 24.25 4.51 0.01 0.01 24.75 4.66 0.01 0.01 25.25 4.71 0.01 0.01 Kashikawa et al. (2004) SDF i'_AB [66-82] 18.250 2.607 2.280 18.750 2.739 2.394 19.250 2.848 2.504 19.750 2.955 2.678 20.250 3.149 3.000 20.750 3.360 3.258 21.250 3.529 3.472 21.750 3.697 3.651 22.250 3.882 3.848 22.750 4.011 3.986 23.250 4.177 4.181 23.750 4.354 4.367 24.250 4.516 4.549 24.750 4.661 4.698 25.250 4.781 4.846 25.750 4.873 5.007 26.250 4.932 5.179 McCracken et al. A&A 410, 17 (2003) VVDS Deep i_ab=I+0.5 [85-98] 18.75 2.45 0.02 0.02 19.25 2.59 0.02 0.02 19.75 2.84 0.02 0.02 20.25 2.99 0.02 0.02 20.75 3.20 0.01 0.01 21.25 3.37 0.01 0.01 21.75 3.55 0.01 0.01 22.25 3.76 0.01 0.01 22.75 3.93 0.01 0.01 23.25 4.06 0.01 0.01 23.75 4.23 0.01 0.01 24.25 4.39 0.01 0.01 24.75 4.53 0.01 0.01 25.25 4.60 0.01 0.01 Capak et al. ApJS 172, 99 (2007) COSMOS i+_AB [101-135] 17.375 1.577 0.07 0.07 17.625 1.756 0.06 0.06 17.875 1.888 0.05 0.05 18.125 2.123 0.04 0.04 18.375 2.254 0.03 0.03 18.625 2.419 0.03 0.03 18.875 2.548 0.02 0.02 19.125 2.639 0.02 0.02 19.375 2.749 0.02 0.02 19.625 2.886 0.02 0.02 19.875 2.995 0.01 0.02 20.125 3.095 0.01 0.01 20.375 3.197 0.01 0.01 20.625 3.310 0.01 0.01 20.875 3.389 0.01 0.01 21.125 3.499 0.01 0.01 21.375 3.583 0.01 0.01 21.625 3.686 0.01 0.01 21.875 3.811 0.01 0.01 22.125 3.896 0.01 0.01 22.375 3.969 0.01 0.01 22.625 4.054 0.01 0.01 22.875 4.134 0.01 0.01 23.125 4.217 0.01 0.01 23.375 4.306 0.01 0.01 23.625 4.392 0.01 0.01 23.875 4.477 0.01 0.01 24.125 4.569 0.01 0.01 24.375 4.656 0.01 0.01 24.625 4.739 0.01 0.01 24.875 4.820 0.01 0.01 25.125 4.907 0.01 0.01 25.375 4.989 0.01 0.01 25.625 5.065 0.01 0.01 25.875 5.122 0.01 0.01 Metcalfe et al. 2000 MNRAS in press, WHT Herschel Deep Field Ikc uncorrected i_ab=I+0.5 [138-150] 19.75 3.220 3.22 0.08 0.10 20.25 2.840 2.84 0.12 0.17 20.75 3.070 3.07 0.09 0.12 21.25 3.521 3.52 0.06 0.07 21.75 3.588 3.59 0.05 0.06 22.25 3.737 3.74 0.04 0.05 22.75 3.937 3.94 0.04 0.04 23.25 4.151 4.19 0.03 0.03 23.75 4.291 4.34 0.03 0.03 24.25 4.456 4.54 0.02 0.03 24.75 4.530 4.63 0.02 0.02 25.25 4.634 4.79 0.02 0.02 25.75 4.607 4.93 0.02 0.02