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.
Main star Case A Case B Case C

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

10 3/20 1/4 1/4

11 3/20 1/4 3/10

12 3/20 3/10 3/10

13 3/20 3/10 3/10

14 3/20 3/10 3/10

15 3/20 3/10 3/10

16 1/4 3/10 3/10

17 1/4 3/5 3/10

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

Source LaTeX | All tables | In the text

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