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Table 2:

Summary of the photometric information (magnitudes and 1-$\sigma $ errors) for our source.
$U_{\rm VIMOS}$$^{\dag }$ B435 V606 R i775 z850 Js H Ks 3.6 $\mu{\rm m}$ 4.5 $\mu{\rm m}$ 5.8 $\mu{\rm m}$ 8.0 $\mu{\rm m}$ 24 $\mu{\rm m}$
29.49 29.86 27.86 27.11 25.22 24.61 24.68 24.80 24.21 22.82 23.00 23.37 23.18 22.61
1$\sigma $ l.m 1$\sigma $ l.m 0.179 0.195 0.039 0.031 0.116 0.151 0.140 0.014 0.024 0.235 0.198 1$\sigma $ l.m.

Notes.  $^{(\dag )}$ Other two WFI U bands are available, U35 and U38 with slightly different filter shape. The lower limits are 27.84 and 26.75, respectively much shallower than the limit provided by the  $U_{\rm VIMOS}$.


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