Table 4: Projected separation of the main IRS 13E sources. From the astrometry the precision on the distance betwen two sources is $\pm$ 15 AU.
   Sources Ang. sep. Distance (AU)

  E1-E2 0.241 $^{\prime \prime }$ 1930

  E1-E4 0.330 $^{\prime \prime }$ 2630

  E2-E4 0.327 $^{\prime \prime }$ 2600

  E2-E3A 0.200 $^{\prime \prime }$ 1600

E3A-E3B 0.073 $^{\prime \prime }$ 590

**Table 4:** Projected separation of the main IRS 13E sources. From the astrometry the precision on the distance betwen two sources is $\pm$ 15 AU.
Sources	Ang. sep.	Distance (AU)
E1-E2	0.241 $^{\prime \prime }$	1930
E1-E4	0.330 $^{\prime \prime }$	2630
E2-E4	0.327 $^{\prime \prime }$	2600
E2-E3A	0.200 $^{\prime \prime }$	1600
E3A-E3B	0.073 $^{\prime \prime }$	590

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