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.
main star Case A Case B Case C

K-band mag. Sep. [ $\lambda /B$ ] Sep. [ $\lambda /B$ ] Sep. [ $\lambda /B$ ]

10 3/20 3/20 3/20

11 3/20 3/20 1/5

12 3/20 3/20 1/4

13 3/20 3/20 1/4

14 3/20 1/4 1/4

15 3/20 1/4 1/4

16 1/5 1/4 1/4

17 1/5 1/4 1/4

**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.
main star	Case A	Case B	Case C
K-band mag.	Sep. [ $\lambda /B$ ]	Sep. [ $\lambda /B$ ]	Sep. [ $\lambda /B$ ]
10	3/20	3/20	3/20
11	3/20	3/20	1/5
12	3/20	3/20	1/4
13	3/20	3/20	1/4
14	3/20	1/4	1/4
15	3/20	1/4	1/4
16	1/5	1/4	1/4
17	1/5	1/4	1/4

Source LaTeX | All tables | In the text

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