Free Access

Table 5

Radial velocities for RGB-GIRAFFE targets.

Cluster members Cluster nonmembers
Star RV σ Comments Star RV σ Comments
[km s-1] [km s-1] [km s-1] [km s-1]

M003 –94.65 0.66 M130 –4.198 3.98 See Sect. 4.1
M012 –98.08 0.64 M138 +11.24 0.89
M061 –101.4 0.88 M171 –29.01 0.93
M098 –104.9 0.99 1 rej M211 –82.82 0.79
M111 –109.0 1.39 M213 –51.61 0.72
M115 –101.8 0.74 M222 –27.92 1.08
M120 –115.6 0.72 M227 See Sect. 4.1 13 spectra
M126 –99.52 1.32 5 spectra M232 –30.0 0.94
M151 –95.39 0.79 M238 +70.63 3.25 See Sect. 4.1
M152 –109.9 0.76 18 spectra M240 –142.4 2.91 See Sect. 4.1
M160 –109.5 0.67 1 rej M250 –54.72 0.59
M193 –107.8 0.19 M253 –72.37 0.72 19 spectra
M199 –102.8 0.47 M256 –69.14 0.73 19 spectra
M204 –110.0 0.80 19 spectra M264 –76.72 0.58
M228 –108.2 1.31 M276 –85.43 1.09
M230 –106.2 0.79 M285 –42.35 1.13
M235 –103.4 0.95 M291 +61.45 1.05
M244 –105.6 3.00 See Sect. 4.1 19 spectra M295 –74.93 0.57
M248 –111.5 0.60 M297 –56.41 0.92
M252 –98.51 0.76 18 spectra M303 –47.3 0.77
M255 –104.8 1.11 M304 +8.44 0.69
M258 –99.11 0.63 M320 –17.7 0.55
M260 –99.67 0.75 M321 –138.0 0.76 1 rej
M263 –100.9 0.84 M322 –49.1 2.14 18 spectra
M267 –101.8 1.04 M323 –130.6 0.66 19 spectra
M270 –108.6 0.84 M327 –54.9 0.66 19 spectra
M273 –105.6 0.73 M328 –45.3 1.46 17 spectra
M284 –106.5 1.24 M330 –27.1 0.59 19 spectra
M299 –105.8 1.01 M333 +20.3 0.66 1 rej
M300 –106.1 1.18 19 spectra M335 –65.1 0.82
M305 –97.61 0.56 M341 –36.5 1.96 See Sect. 4.1
M308 –110.3 0.71 19 spectra M349 –53.0 9.11 See Sect. 4.1
M319 –106.6 0.84 M356 –20.4 0.69
M326 –107.1 1.31 M360 –141.6 0.28
M339 –101.8 0.89 19 spectra M362 –8.8 0.42
M342 –102.9 0.70 M383 –61.0 0.62
M351 –106.4 0.74
M354 –93.3 0.92
M357 –101.5 0.87 1 rej

Notes. Both member stars in NGC 5927 (left column) as well as nonmembers (right panel) are listed. The first and fifth columns list the ID for the star. The second and sixth columns give our final radial velocity for the star and the third and seventh column lists the sigma of the 20 individual measurements that the radial velocity is based on. For some stars one spectrum were rejected from the final averaged spectrum. For some stars less than 20 spectra were available (e.g., due to faulty fibres or miss-placements). The number of available spectra is noted in case it is less than 20. Stars discussed individually in Sect. 4.1 are also indicated.

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.