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.
main star case A case B case C

K-band mag. $\Delta m_0$ $\Delta \Theta _{\rm r}$ $\Delta m_{\rm r}$ $\Delta m_0$ $\Delta \Theta _{\rm r}$ $\Delta m_{\rm r}$ $\Delta m_0$ $\Delta \Theta _{\rm r}$ $\Delta m_{\rm r}$

10 5 20% 3.5 3.5 20% 2 3 22% 2.5

12 4 10% 2.8 3 20% 2 3 22% 2.5

14 3.5 10% 2.5 3 20% 1.8 2.5 22% 2.3

15 3 10% 2.3 2.5 10% 1.7 2.5 22% 2

17 2.5 10% 1.7 2 0% 1.4 1.5 10% 1

**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.
main star	case A	case B	case C
K-band mag.	$\Delta m_0$	$\Delta \Theta _{\rm r}$	$\Delta m_{\rm r}$	$\Delta m_0$	$\Delta \Theta _{\rm r}$	$\Delta m_{\rm r}$	$\Delta m_0$	$\Delta \Theta _{\rm r}$	$\Delta m_{\rm r}$
10	5	20%	3.5	3.5	20%	2	3	22%	2.5
12	4	10%	2.8	3	20%	2	3	22%	2.5
14	3.5	10%	2.5	3	20%	1.8	2.5	22%	2.3
15	3	10%	2.3	2.5	10%	1.7	2.5	22%	2
17	2.5	10%	1.7	2	0%	1.4	1.5	10%	1

Source LaTeX | All tables | In the text

	1 Introduction
	2 The super-resolving algorithm
	3 Image generation
	4 Numerical results
	5 Discussion
	References