\begin{table}%t1 \caption{\label{sas}Solar analogue stars used to obtain the reflectance spectra of the asteroids of this survey.} %%\centering \par \begin{tabular}{lcccccccl} \hline\hline \noalign{\smallskip} Star & $\alpha$ (J2000) & $\delta$ (J2000) & $V$ & $B-V$ & $V-K$ & $J-H$ & $H-K$ & Spectral type \\ \hline Hyades 64\tablefootmark{a} & 04:26:40.1 & +16:44:49 & 8.090 & 0.657 & 1.543 & 0.250 & 0.096 & G2 V \\ Landolt SA 93-101 & 01:53:18.0 & +00:22:25 & 9.720\tablefootmark{b} & 0.650$^b$ & 1.548 & 0.309 & 0.098 & G5 \\ Landolt SA 98-978 & 06:51:34.0 & --00:11:28 & 10.570\tablefootmark{c} & 0.609$^c$ & 1.399 & 0.255 & 0.084 & F8 \\ Landolt SA 102-1081 & 10:57:04.4 & --00:13:10 & 9.903\tablefootmark{c} & 0.664\tablefootmark{c} & & & & G2\tablefootmark{b}\\ Landolt SA 107-684 & 15:37:18.1 & --00:09:50 & 8.433\tablefootmark{d} & 0.619$^d$ & 1.603 & 0.263 & 0.122 & G0 \\ Landolt SA 107-998 & 15:38:16.4 & +00:15:23 & 10.440\tablefootmark{b} & 0.630\tablefootmark{b} & 1.600 & 0.255 & 0.117 & G3\tablefootmark{b} \\ Landolt SA 110-361 & 18:42:45.0 & +00:08:04 & 12.425\tablefootmark{c} & 0.632\tablefootmark{c} & 1.565 & 0.285 & 0.066 & \\ Landolt SA 112-1333 & 20:43:11.8 & +00:26:15 & 9.990\tablefootmark{b} & 0.620\tablefootmark{b} & 1.526 & 0.248 & 0.115 & F8 \\ Landolt SA 115-271 & 23:42:41.8 & +00:45:10 & 9.695\tablefootmark{c} & 0.615\tablefootmark{c} & 1.557 & 0.258 & 0.121 & F8 \\ \hline P330E & 16:31:33.8 & +30:08:47 & 13.010 & 0.620 & 1.500 & 0.280 & 0.060 & G0 V \\ \hline Hardorp\tablefootmark{e} & -- & -- & -- & 0.663 & 1.490 & 0.310 & 0.060 & \\ \hline {\bf Sun}\tablefootmark{f} & & & & & & & & G2 V \\ C85& -- & -- & -- & -- & 1.486 & 0.310 & 0.060 & \\ C96& -- & -- & -26.75 & 0.630 & 1.500 & 0.310 & 0.060 & \\ HD02& -- & -- & -- & 0.641 & 1.486 & 0.230 & 0.060 & \\ H80& -- & -- & -26.71 & 0.665 & -- & -- & -- & \\ \hline \end{tabular} \tablefoot {\tablefoottext{a}{Solar analogue star Hyades 64 belongs to class~1 following Hardorp (\cite{hardorp78}), i.e., it~is considered as perfect solar analogue. $V$~magnitude and $B-V$~colour for this star were taken from that paper;} \tablefoottext{b}{data extracted from Landolt (\cite{landolt73});} \tablefoottext{c}{colours extracted from Landolt (\cite{landolt});} \tablefoottext{d}{colours extracted from Landolt (\cite{landolt83});} \tablefoottext{e}{mean values from the list of Campins et~al. (\cite{campins85}) of solar analogue stars belonging to Hardorp's class~1;} \tablefoottext{f}{colours of the Sun following different authors: C85~$\equiv$ Campins et~al. (\cite{campins85}); C96~$\equiv$ Colina et~al. (\cite{colina96}); H02~$\equiv$ Hainaut \& Delsanti (\cite{hainaut02}); H80~$\equiv$ Hardorp (\cite{hardorp80}).} } \vspace*{3mm} \end{table}