Table 2: Photometry of the white dwarf COMBO-17 J1143. A minimum photometric error of $0\hbox{$.\!\!^{\rm m}$ }03$ was assumed to take calibration uncertainties into account.

$\lambda_{\rm {\rm cen}}$/ fwhm
Vega-mag ABmag

365/36
U     $22.65 \pm 0.04$ 23.44
458/97 B $22.45 \pm 0.03$ 22.34
538/89 V $21.86 \pm 0.03$ 21.86
648/160 R $21.46 \pm 0.03$ 21.67
857/147 I $21.60 \pm 0.04$ 22.11
  J <21.6 <22.57
418/27   $22.70 \pm 0.05$ 22.54
462/13   $22.45 \pm 0.03$ 22.29
486/31   $22.15 \pm 0.03$ 22.11
519/16   $21.93 \pm 0.03$ 21.89
572/25   $21.71 \pm 0.03$ 21.77
605/21   $21.66 \pm 0.03$ 21.79
645/30   $21.45 \pm 0.03$ 21.69
696/21   $21.36 \pm 0.03$ 21.65
753/18   $21.38 \pm 0.03$ 21.77
816/21   $21.47 \pm 0.04$ 21.96
857/15   $21.66 \pm 0.13$ 22.24
914/26   $21.83 \pm 0.06$ 22.35

$(g-r)_{\rm SDSS}$
    $ 0.71 \pm 0.12$
$(r-i)_{\rm SDSS}$     $-0.23 \pm 0.17$
$(g-r)_{\rm COMBO-17}$     $ 0.53 \pm 0.05$
$(r-i)_{\rm COMBO-17}$     $-0.12 \pm 0.05$


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