All Tables

Table 1: Summary of the results obtained in the case where the magnitude difference between the two stars is zero - monolithic case. Sep. is the minimum separation, in units of $\lambda /D$ , allowing for detection and characterization of the binary system.
Table 2: Summary of the results obtained in the case where the angular separation of the two stars is $\frac{1}{2}\lambda/D$ . The quantities $\Delta m_0$ , $\Delta \Theta _{\rm r}$ , and $\Delta m_{\rm r}$ are defined in the text.
Table 3: Summary of the results obtained in the case where the magnitude difference between the two stars is zero - interferometric case. Sep. is the minimum separation obtained in units of $\lambda /B$ , where B is the maximum baseline of LBT.
Table 4: Summary of the results obtained in the case where the angular separation of the two stars is $\frac{1}{2}\lambda/B$ , where B is the maximum baseline of LBT.