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Table A.1

Offsets applied to combine data of the two observed epochs and the noise level of the obtained image.

Offsets (mas) Noise µJy bm−1
StarID α δ
BD17232 −0.45 +0.13 25
HIP 12545 −0.30 +0.22 13
HIP 12635 −0.41 +0.89 14
V 875 Per −0.32 +0.27 23
TYC 3301 −0.37 +0.79 15
HD 22213 −0.55 −0.23 17
HD 23524 −0.44 +0.76 19
HD 24681 −0.21 +0.43 12
HD 285281 +0.02 +0.07 13
HD 284135 +0.05 +0.11 14
HD 31281 −0.00 +0.03 21
BD 08995 −0.08 −0.05 16
HD 286264 −0.06 +0.12 16
HD 293857 −0.05 +0.06 15
TYC 7136611 +0.01 +0.25 10
TYC 59251547 −0.04 −0.03 12
AI Lep −0.04 −0.13 12
HD 62237 +0.05 −0.10 15
SAO 135659 +0.26 −0.15 16
WDS 09035+3750B +0.42 +4.74 19
HD 82159 +3.42 +0.14 38
HD 82558 +4.01 −3.24 22
GJ 2079 +2.75 +4.44 16
HD 135363 +1.02 −1.03 20
UCAC 4832 +1.02 −1.03 14
HD 199143 −0.37 +0.51 17
HD 358623 −0.38 +0.54 16
SAO 50350 −0.35 −0.93 14
GJ 4199 −0.28 −0.00 14
SAO 51891 −0.43 −0.45 18
SAO 108142 −0.29 +0.05 13

Notes. Offsets are as expected assuming the parallax and proper motions obtained from the optical results. Detected sources are highlighted with gray-shaded rows. The noise value was measured in the image of two combined epochs, that is, after applying the correction of the offsets.

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