Table 3: Positions and magnitudes of optical point sources closest to the radio positions of two MSPs. The limiting magnitudes are also provided for $3.5 \sigma $ detection at the central pixel in the exposure times used here for PSR J1744-1134.
Object Magnitude PSR pos. - Obj. pos.
    $ \delta$ RA $ \delta$ Dec
J1744-1134 $B\geq26.9$, $V\geq26.3$, 0 $.\!\!^{\prime\prime}$0 0 $.\!\!^{\prime\prime}$0
(upper lim.) $R\geq26.0$    
1744-Br B=22.86, V=21.34, $+0\hbox{$.\!\!^{\prime\prime}$ }4$ $-2\hbox{$.\!\!^{\prime\prime}$ }0$
  R=20.61    
1024-Br U=22.11, V=19.82, $+0\hbox{$.\!\!^{\prime\prime}$ }1$ $-0\hbox{$.\!\!^{\prime\prime}$ }2$
  R=18.89, I=18.17    
1024-Fnt U=23.8, V=24.9, $-0\hbox{$.\!\!^{\prime\prime}$ }2$ $+1\hbox{$.\!\!^{\prime\prime}$ }5$
  R=24.4, I=24.2    


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