\begin{table}%t1
\caption{\label{tab_CC}The estimated $(J-H)_{\rm in}$ and $(H-K_{\rm s})_{\rm in}$ intrinsic colours for main sequence stars.}
\par
%\centerline
{
\begin{tabular}{llccrrr}
\hline\hline
Sp.&$M_{K}$&$(J-H)_{\rm in}$&$(H-K_{\rm s})_{\rm in}$&$\sigma_{(JH)_{\rm o}}$&$\sigma_{(HK)_{\rm o}}$&$N^{\star}$\\
\hline  
A0V&   0.65&  -0.026&  0.029&0.030&0.028&50 \\
A1V&   1.00&  -0.014&  0.036&0.037&0.032&45 \\
A2V&   1.17&  -0.004&  0.043&0.044&0.035&43 \\
A3V&   1.35&   0.020&  0.048&0.049&0.032&58 \\
A4V&   1.49&   0.042&  0.050&0.044&0.026&23 \\
A5V&   1.60&   0.050&  0.052&0.040&0.029&24 \\
A6V&   1.62&   0.058&  0.051&0.037&0.024&12 \\
A7V&   1.63&   0.075&  0.054&0.039&0.031&23 \\
A8V&   1.64&   0.084&  0.055&0.047&0.032&8  \\
A9V&   1.72&   0.090&  0.059&0.033&0.026&37 \\
F0V&   1.86&   0.119&  0.062&0.042&0.026&105\\
F1V&   2.00&   0.142&  0.062&0.040&0.026&9  \\
F2V&   2.15&   0.162&  0.064&0.035&0.025&141\\
F3V&   2.26&   0.170&  0.065&0.032&0.029&269\\
F4V&   2.38&   0.175&  0.064&0.037&0.028&28 \\
F5V&   2.49&   0.195&  0.068&0.036&0.027&492\\
F6V&   2.62&   0.211&  0.072&0.036&0.027&390\\
F7V&   2.75&   0.228&  0.069&0.034&0.032&387\\
F8V&   2.88&   0.235&  0.069&0.038&0.029&308\\
F9V&   3.04&   0.252&  0.080&0.030&0.028&30 \\
G0V&   3.19&   0.257&  0.076&0.033&0.028&396\\
G1V&   3.24&  0.265&  0.078&0.035&0.028&242\\
G2V&   3.29&  0.276&  0.079&0.036&0.026&320\\
G3V&   3.34&  0.285&  0.083&0.036&0.029&477\\
G4V&   3.45&  0.302&  0.084&0.032&0.031&8  \\
G5V&   3.56&  0.303&  0.085&0.035&0.030&499\\
G6V&   3.68&  0.325&  0.090&0.040&0.028&188\\
G8V&   3.90&  0.347&  0.093&0.048&0.030&259\\
G9V&   4.03&  0.363&  0.094&0.074&0.021&9  \\
K0V&   4.15&  0.388&  0.098&0.048&0.031&207\\
K1V&   4.13&  0.406&  0.094&0.046&0.032&93 \\
K2V&   4.15&  0.453&  0.115&0.053&0.028&140\\
K3V&   4.15&  0.473&  0.120&0.046&0.039&137\\
K4V&   4.22&  0.529&  0.130&0.057&0.037&43 \\
K5V&   4.35&  0.555&  0.142&0.051&0.031&108\\
K7V&   4.83&  0.604&  0.160&0.031&0.035&54 \\
\hline	
\end{tabular}}
\par
\medskip
$N^{\star}$ the number of stars used to estimate the colours.
\end{table}