Table 1: A summary of the photometric data of the GOODS-South field used in this work.
FILTER $\lambda_{\rm c}$ $\Delta \lambda$ EXPTIME FWHMa PIXSCALE ZP AREA MAGLIMb
  Å Å s arcsec arcsec/px AB $\rm arcmin^2$ 90$\%$
U35 3590 222 53 654 0.90 0.23 28.520 143.2 25.5
U38 3680 170 75 100 1.10 0.23 28.755 143.2 24.5
UVIMOS 3780 197 10 000 0.80 0.20 32.500 90.2 26.5
B (F435W) 4330 508 7200 0.12 0.03 25.65288 143.2 27.5
V (F606W) 5940 1168 6000 0.12 0.03 26.49341 143.2 27.5
i (F775W) 7710 710 6000 0.12 0.03 25.64053 143.2 26.5
z (F850LP) 8860 554 12 000 0.12 0.03 24.84315 143.2 26.0
$J_{\rm ISAAC}$ 12 550 1499 12 600c 0.45c 0.15 26.000 143.2 24.5
$H_{\rm ISAAC}$ 16 560 1479 18 000c 0.45c 0.15 26.000 78.0 24.3
$Ks_{\rm ISAAC}$ 21 630 1383 23 400c 0.45c 0.15 26.000 143.2 23.8
$CH1_{\rm IRAC}$ 35 620 3797 82 800 1.60 0.60 22.416 143.2 24.0
$CH2_{\rm IRAC}$ 45 120 5043 82 800 1.70 0.60 22.195 143.2 23.4
$CH3_{\rm IRAC}$ 56 860 6846 82 800 1.90 0.60 20.603 143.2 22.0
$CH4_{\rm IRAC}$ 79 360 14 797 82 800 2.00 0.60 21.781 143.2 22.0
a For ground-based images, $\it FWHM$ corresponds to the seeing, while for space-based data it is the PSF of the instrument.
b The limiting magnitudes (at 90% completeness) are the mean values on the field, averaged on the positions and areas of every object.
c For J, H, and Ks filters, we report only the mean value of seeing and exposure time: detailed values can be found in Vandame et al. (in preparation).

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