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Table 2:

Companions in visual binary and multiple systems with incorrect USNO-B1 proper motions.

No.
$\rho$ $\theta$ $\mu_\alpha \cos{\delta}$ $\mu_\delta$ J
  [arcsec] [deg] [mas a-1] [mas a-1] [mag]

02a
7.2 242 +3.9 $\pm$ 0.7 -2.3 $\pm$ 0.7 14.53 $\pm$ 0.03
04b 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
42c 4.5 237 +1.3 $\pm$ 1.9 -10.6 $\pm$ 0.8 16.78 $\pm$ 0.03

Notes. (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.
(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.
(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).


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