\begin{table}%t2 \par \caption{\label{table.binaries}Companions in visual binary and multiple systems with incorrect USNO-B1 proper motions.} \small%\centering \par \begin{tabular}{ccc ccc} \hline \hline \noalign{\smallskip} No. & $\rho$ & $\theta$ & $\mu_\alpha \cos{\delta}$ & $\mu_\delta$ & $J$ \\ & [arcsec] & [deg] & [mas~a$^{-1}$] & [mas~a$^{-1}$] & [mag] \\ \noalign{\smallskip} \hline \noalign{\smallskip} 02\tablefootmark{a}& 7.2 & 242 & +3.9~$\pm$~0.7 & --2.3~$\pm$~0.7 & 14.53~$\pm$~0.03 \\ 04\tablefootmark{b}& 8.1 & 168 & +6.1~$\pm$~0.9 & --8.1~$\pm$~1.2 & 16.08~$\pm$~0.08 \\ 09 & 5.3 & 182 & --8.2~$\pm$~1.4 & --13.6~$\pm$~1.0 & 15.19~$\pm$~0.05 \\ 12 & 6.0 & 335 & +10.5~$\pm$~1.3 & --7.7~$\pm$~0.8 & 16.27~$\pm$~0.08 \\ 18 & 6.6 & 292 & +5.4~$\pm$~1.8 & --17.2~$\pm$~2.1 & 14.49~$\pm$~0.04 \\ 20 & 4.8 & 234 & --2.0~$\pm$~1.0 & --11.5~$\pm$~1.0 & 15.16~$\pm$~0.04 \\ 21 & 7.5 & 152 & +4.6~$\pm$~0.7 & --16.3~$\pm$~1.1 & 13.07~$\pm$~0.03 \\ 22 & 5.6 & 311 & +1.0~$\pm$~0.7 & --4.5~$\pm$~0.6 & 14.36~$\pm$~0.04 \\ 38 & 6.6 & 324 & --9.6~$\pm$~0.6 & +9.7~$\pm$~0.6 & 14.47~$\pm$~0.03 \\ 42$^{c}$& 4.5 & 237 & +1.3~$\pm$~1.9 & --10.6~$\pm$~0.8 & 16.78~$\pm$~0.03 \\ \hline \end{tabular} \tablefoot{\tablefoottext{a}{The visual companion to star No.~02 is appreciably brighter in the visible ($\overline{B_J} = 18.7$~mag versus $\overline{B_J} = 19.8$~mag) and fainter in the near infrared ($K_{\rm s} = 15.41 \pm0.08$~mag versus $K_{\rm s} = 13.59 \pm 0.04$~mag) than the star No.~02.}\\ \tablefoottext{b}{There is an additional visual companion to star No.~04. It is a faint, blue source at $\rho \sim 4.1$~arcsec, $\theta \sim 217$~deg, only resolved by 2MASS and UKIDSS ($J = 16.43\pm0.10$~mag), with similarly low proper motion.}\\ \tablefoottext{c}{UKIDSS $J$-band magnitude transformed into the 2MASS one by adding the offset $J_{\rm 2MASS} - J_{\rm UKIDSS}$ measured for Mayrit~1610344. There are two additional visual companions to this star: USNO-A2.0~0825--01615246, a relatively blue star at 7.8~arcsec to the southwest and with a proper motion ($\mu_\alpha \cos{\delta}$, $\mu_\delta) = (+2.9\pm1.2$, $-7.6 \pm0.7$)~mas~a$^{-1}$, and a faint red source at about 3~arcsec to the southeast only resolved by UKIDSS ($K \approx 16.3$~mag).}} \end{table}