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Table 2

Barycentric Julian dates of each target, derived RVs, and final dispersion for each date it was observed.

Source MJD vrad [km s-1]  ⟨ σ ⟩  Source MJD vrad [km s-1]  ⟨ σ ⟩ 
nodded images
GSS 26 2 454 584.63565 –6.97198 HD129642 2 454 584.62788 –4.48490
2 454 584.63909 –6.93852 2 454 584.63176 –4.59242
2 454 584.63745 –6.94756 2 454 584.62387 –4.22596
2 454 584.64087 –6.96722 0.01 2 454 584.61976 –4.59242
2 454 595.81134 –6.93863 2 454 584.63573 –4.60915
2 454 595.81313 –7.03562 2 454 584.63931 –4.26827 0.09
2 454 595.81492 –6.95636 2 454 595.76527 –4.48264
2 454 595.81664 –6.89839 0.03 2 454 595.76193 -4.71534
2 454 700.50155 –6.98628 2 454 595.75729 –4.67921
2 454 700.50334 –6.99655 2 454 595.75303 –4.64180
2 454 700.50501 –6.94632 2 454 595.76937 –4.72930
2 454 700.50681 –6.86636 0.03 2 454 595.77303 –4.82873 0.06
GY23 2 454 584.66269 –11.74129 2 454 696.51517 –4.59595
2 454 584.66334 –11.91061 2 454 696.51934 –4.49518
2 454 584.66383 –11.61631 2 454 696.51108 –4.63937
2 454 584.66435 –11.92826 0.07 2 454 696.50713 -4.34328
2 454 595.80848 –6.86636 2 454 696.52319 –4.60013
2 454 595.80786 –6.99655 2 454 696.52733 –4.75527 0.07
2 454 595.80737 –6.94632 2 454 712.50231 –4.80776
2 454 595.80672 –6.82011 0.04 2 454 712.50480 –4.59263
2 454 710.51703 –10.14933 2 454 712.50349 –4.68273
2 454 710.51638 –9.97590 2 454 712.50343 –4.72138
2 454 710.51590 –10.23329 2 454 712.50391 –4.44132
2 454 710.51526 –10.11078 0.05 2 454 712.50429 –4.62820 0.07
Gl 406 2 454 890.64318 19.73374 HD105671 2 454 795.13436 –4.20193
2 454 890.64215 19.72979 2 454 795.13447 –4.22028 0.01
2 454 890.64125 19.74171
2 454 890.64024 19.70016 0.01
combined images
GY 51 2 454 584.67379 –10.75198 0.22 L 1689 SNO2 2 454 699.66023 –7.76361 0.76
2 454 595.83890 –9.44251 0.35 2 454 873.87196 –7.26417 0.56
2 454 597.72588 –6.26190 0.25 2 454 884.87905 –5.76223 0.92
2 454 710.527356 –10.18371 0.73
VSSG 18 2 454 597.88737 –15.89123 0.28 IRS 34 2 454 597.80272 –7.36514 0.63
2 454 612.72451 –13.73072 0.32 2 454 612.80033 –7.17129 0.80
2 454 733.55090 –17.12639 0.44 2 454 712.56017 –7.25198 1.22
WL 17 2 454 597.75984 –5.62187 0.65
2 454 610.76480 –6.12428 1.10

Notes. In the upper table the results from each nodded image are presented. In the lower panel we show the RV measurements in images of sources that yielded an insufficiently S/N after telluric removal and that had to be combined for better precision.

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