**Table 3:** Measured parameters of all candidate triple/quadruple systems resolved in our survey, with their apparent multiplicity in the projected separation range 0 $.\!\!^{\prime\prime}$ 07-12 $^{\prime \prime }$ . Also quoted in last column is the probable and assumed multiplicity of this systems in this separation range based on the chance projection analysis of Sect. 4.5.
$\begin{displaymath}\begin{tabular}{lcc@{\hspace{3mm}}r@{~$\pm$~}l@{\hspace{2mm}}... ....05 & 0.05 & \multicolumn{2}{c}{...} & \\ \hline \end{tabular}\end{displaymath}$ ^a Includes the edge-on disk LkH $\alpha$ 262/263C (Jayawardhana et al. 2002; Chauvin et al. 2002) undetected in our survey. ^b Sz 41 C was unambiguously identified as a background giant (Walter 1992). Notes: multiplicity abbreviations are B = Binary, T = Triple and Q = Quadruple. Multiplicity references: (1) This work. (2) RZ93. (3) Brandeker et al. (2001). (4) Duchêne (1999). (5) White & Ghez (2001). (6) Simon et al. (1992). (7) Leinert et al. (1993). (8) Ghez et al. (1993). (9) Ghez et al. (1997a). (10) Brandner et al. (1996). (11) Leinert et al. (1991). (12) Jayawardhana et al. (2002). (13) Chauvin et al. (2002). (14) Simon et al. (1995). (15) Walter (1992).

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