\begin{table}%t3
\caption{The sample of cool WDs from the GSC-II survey:
photometry, classification, source telescope, WD ID in other
catalogues.}
\label{tab:objects2}
%\centerline
{
\begin{tabular}{llcccccr}      
\hline\hline
ID         & &$B_{J}$ & $R_{\rm F}$ & $B_{J}-R_{\rm F}$ & Type & Source & WDs ID\\
\hline
GSC2U J003209.6$-$025402  & &17.78& 16.51  &  1.27  &   DA  & $^a$  &  WD 0029-032\\
GSC2U J003536.0+015314  & &15.78  & 15.70   &  0.08  &   DA  & TNG & WD 0033+016\\
GSC2U J010456.6+212002  & &18.60   & 17.42  &  1.18 &  DC  & TNG & WD 0102+210A\\
GSC2U J010458.1+212021  & &18.90 & 17.52  &  1.38  & DC  & TNG& WD 0102+210B\\
GSC2U J025936.9+172533  & &19.61 & 19.06  &  0.55  &  DA  & TNG&\\
GSC2U J030339.2+140805  & & 20.63  & 19.54 & 1.09   &  DA+dM & TNG&\\
GSC2U J031000.4+163022  & &18.04 & 17.85  &  0.19  &  DA  & TNG&\\
GSC2U J071858.8+551406  & &20.84 & 19.71  & 1.13  & DC  &WHT &\\
GSC2U J113524.7+271741  & & 19.13  & 18.22  &  0.91 &  DC &TNG&\\
GSC2U J114625.7-013635  & & 16.53 & 15.98 &  0.55  &  DA &TNG& SDSS J114625.77-013636.9\\
GSC2U J122810.3+415003  & &19.24& 18.42  &  0.82  &  DC & TNG&\\
GSC2U J123752.6+415622  & &17.83& 16.70  &  1.13  &  DQ & TNG/INT&\\
GSC2U J123915.4+452520  & &16.83& 16.27  &  0.56  &  DA & TNG & WD 1236+457\\
GSC2U J124212.6+295801  & &18.34& 17.75  &  0.58  &  DA & TNG&\\
GSC2U J125313.0+343712  & &19.90& 18.41  &  1.49 &  DC  &TNG&\\
GSC2U J125509.6+465520  & &19.49& 18.28  &  1.21 & DC   &TNG&\\
GSC2U J125946.8+273404  & & 15.55& 15.13  &  0.42 & DA & TNG& WD 1257+278\\
GSC2U J131147.2+292348  & &19.56& 18.04  &  1.52 &  Peculiar DQ$^{b}$ &WHT&\\
GSC2U J131749.0+215715  & & 17.30&16.59     &  0.71 &  DC  &TNG &\\
GSC2U J132325.2+303615  & & 19.89& 19.35  &  0.54 &  DA  &TNG &\\
GSC2U J132857.4+445034  & & 18.57& 18.04  &  0.53 &  DC  &TNG &\\
GSC2U J132909.6+310947  & & 21.23&  19.32 &  1.91 &  DC  &TNG/WHT &\\
GSC2U J133059.8+302955  & & 16.62& 15.75  &  0.87 &  Peculiar DZ$^{c}$ &TNG & WD 1328+307 \\
GSC2U J133250.9+011707  & & 17.34 & 16.65 &  0.69 & DC+DA$^d$ & TNG  &WD 1330+015 (A+B) \\
GSC2U J133360.0+001654  & & 19.50& 17.98  &  1.52 & DQ  &TNG/INT &WD1331+005\\
GSC2U J133616.1+001733  & & 17.72& 16.73  &  0.99  &  DA+dM &TNG&SDSS J133616.05+001732.7\\
GSC2U J133620.4+364829  & &18.21& 17.40  &  0.81   &  DA  &TNG &\\
GSC2U J134043.4+020348  & & 18.38& 17.60  &  0.78  & DA   &TNG &SDSS J134043.35+020348.3\\
GSC2U J134107.9+415004  & & 17.95& 17.52  &  0.43 &  DA   &TNG &\\
GSC2U J135118.4+425317  & &17.14& 16.52 & 0.62  &  DC   &TNG &\\
GSC2U J155611.5+115351  & &  20.51&18.94  &  1.57 &  DC   &TNG &\\
GSC2U J155721.8+141212  & & 19.43& 18.06  &  1.37  &  DC &TNG  &\\
GSC2U J162242.0+670112  & & 18.89& 18.99  & --0.10 &  DA   & TNG/WHT &\\
GSC2U J165237.4$-$011354  & & 17.87& 16.69   &  1.18 &    DA &TNG  &\\
GSC2U J222233.1+122140  & & 19.74& 17.87  &  1.87  & DC  & TNG& SDSS J222233.90+122143.0\\
GSC2U J224011.2$-$030316  & & 18.95&17.79  &  1.16  &   DC  &TNG &\\
GSC2U J231518.5$-$020942  & & 16.39& 16.00  &  0.39  &  DZ &  TNG&WD 2312-024\\
GSC2U J232115.4+010214  & &19.62& 18.65  &  0.97   & DA  &TNG &WD 2318+007A\\
GSC2U J232116.8+010227  & &20.23& 18.79  &  1.44   & DC &TNG &WD 2318+007B\\
GSC2U J233539.1+123048  & &18.81& 18.45  &  0.36  &  DC & TNG &\\
GSC2U J233707.4+003240  & &18.58& 17.61  &  0.97  & DA  &TNG &SDSS J233707.68+003242.3\\
\hline
\end{tabular}}
\smallskip
$^{a}$ Classification from Monet et~al. (1992) and Bergeron et~al. (1997).\\
$^{b}$ Peculiar DQ with extremely strong C$_2$ bands (Carollo et~al. 2002, 2003).\\
$^{c}$ Heavily blanketed DZ (G 165-7) (Wehrse \& Liebert 1980). \\
$^{d}$ Unresolved binary (DC + magnetic DA) modeled by Bergeron et~al. (1997).
\end{table}