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Table 3

Results obtained from LI observations after applying the LIST algorithm for astrometric measurements of the separation and position angle between the detected components.

WDS Telescope ρ¯$\bar \rho$ Jaccard θ¯$\bar \theta$ Jaccard
(α,δ,J2000.0) (″) index (◦) index
(1) (2) (3) (4) (5) (6)
08585+3548 NOT 0.098 0.08 42 0.29
08585+3548 TCS 0.099 0.08 45 0.29
10083+3136 NOT 0.092 0.43 168 0.13
10083+3136 TCS 0.085 0.25 343 0.10
10116+1321 NOT 0.092 0.64 280 0.21
10116+1321 TCS 0.085 0.43 270 0.36
15245+3723 NOT 0.101 0.07 268 0.14
15245+3723 TCS 0.080 0 279 0.09

Notes. Columns: (1) is the WDS number and (2) the telescope used. (3) shows the angular separation measured in arcseconds and (4) the Jaccard index for this variable. (5) the position angle between the two components obtained in the images, and (6) the Jaccard index for this variable.

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