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Table 1.

Multiple systems observed with lucky spectroscopy in this paper.

Name PC SC WDS ID BP Even. date Det. nexp nused texp. d PA ΔB
(YYMMDD) (s) (″) (°) (mag)
FN CMa A B J07067−1118 5.8 190220 EEV 120 60 1.00 0.57 109 1.2
190917 EEV 100 15 1.00 0.57 109 1.2
6 Cas A B J23488+6213 6.3 180729 EEV 143 65 1.00 1.50 194 2.3
α Sco A B J16294−2626 2.8 120708 EEV 15 15 4.33 2.57 297 0.0
180730 EEV 100 23 1.00 2.70 273 3.6
σ Sco Aa Ab J16212−2536 3.2 180730 EEV 100 13 1.00 0.47 242 2.1
CS Cam A B J03291+5956 4.6 190917 EEV 100 66 1.00 2.30 159 4.2
σ Ori Aa,Ab B J05387−0236 4.4 170907 EEV 100 7 1.00 0.26 84 1.2
181203 EEV 100 12 1.00 0.25 67 1.2
190917 EEV 100 10 1.00 0.26 84 1.2
HD 5005 A B J00528+5638 8.6 181219 QUC 1004 100–402 1.00 1.53 82 1.6
190906 EEV 100 58 1.00 1.53 82 1.6
HD 51 756 A B J06585−0301 7.8 181219 QUC 1004 26–51 1.00 0.63 100 0.3
HD 218 195 A B J23052+5815 8.7 181220 QUC 502 216–365 1.00 0.94 81 2.7
HD 219 460 A B J23152+6027 11.0 181220 QUC 502 423–499 1.00 1.38 127 0.3
HD 8768 A B J01281+6317 9.3 181220 QUC 502 138–247 1.00 0.66 28 2.8
BD +60 544 A B J02411+6108 10.4 181220 QUC 502 403–502 1.00 1.91 170 0.8
HD 17 520 A B J02512+6023 10.3 181220 QUC 502 262–279 1.00 0.32 298 0.7
HD 24 431 A B J03556+5238 7.2 181220 QUC 502 209–273 1.00 0.72 177 2.9
HD 164 492 A B J18024−2302 7.6 190914 EEV 100 71 1.00 6.19 20 3.6
HD 168 021 A B J18187−1837 7.4 190421 EEV 100 33 1.00 0.48 137 1.0
HD 193 443 A B J20189+3817 8.3 190731 EEV 100 13 1.00 0.14 258 0.3
HD 194 649 A B J20254+4014 10.6 190914 EEV 100 95 1.00 0.30 214 0.7
HD 191 201 A B J20074+3543 7.8 190914 EEV 100 47 1.00 1.00 84 1.8

Notes. PC and SC refer to the primary and secondary visual components, respectively, and BP is the B-band magnitude of the primary. For each observation we give the evening date, the detector used (EEV for EEV12, QUC for QUCAM3), the number of total exposures, the number of exposures used for lucky spectroscopy (single value for EEV12, range for QUCAM3), the exposure time (for one exposure), the separation d (measured from the data), the position angle used for the slit (which may be different from the one for the system), and the magnitude difference in B (measured from the data).

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