Table 2
Basic data for candidate TO stars observed with GIRAFFE in NGC 5927.
| Star | RA | Dec | RV | V 606 | (V606 − I814) | |||||||||||
| (fibre) | (fibre) | [km s-1] | ||||||||||||||
|
|
||||||||||||||||
| TO001 | 15 27 49.25 | –50 41 08.00 | –103.74 | 20.11 | –0.097 | |||||||||||
| TO004 | 15 27 50.70 | –50 39 46.40 | –107.32 | 20.23 | –0.105 | |||||||||||
| TO012 | 15 27 51.21 | –50 40 41.10 | –106.90 | 19.81 | –0.088 | |||||||||||
| TO013 | 15 27 52.64 | –50 39 02.20 | –98.06 | 20.05 | –0.101 | |||||||||||
| TO014 | 15 27 51.24 | –50 41 13.50 | –99.88 | 20.24 | –0.092 | |||||||||||
| TO015 | 15 27 52.31 | –50 39 43.10 | –96.88 | 19.80 | –0.048 | |||||||||||
| TO016 | 15 27 51.12 | –50 41 48.70 | –118.28 | 20.16 | –0.109 | |||||||||||
| TO021 | 15 27 53.81 | –50 39 44.20 | –111.05 | 19.97 | –0.104 | |||||||||||
| TO022 | 15 27 54.42 | –50 38 57.60 | –102.84 | 19.89 | –0.060 | |||||||||||
| TO033 | 15 27 53.58 | –50 41 13.30 | –110.28 | 20.04 | –0.097 | |||||||||||
| TO036 | 15 27 54.61 | –50 40 46.50 | –105.18 | 19.99 | –0.148 | |||||||||||
| TO037 | 15 27 53.72 | –50 42 05.10 | –99.15 | 19.85 | –0.025 | |||||||||||
| TO051† | 15 27 59.47 | –50 41 40.70 | –105.33 | |||||||||||||
| TO052 | 15 28 1.45 | –50 39 27.30 | –102.29 | 20.04 | –0.090 | |||||||||||
| TO054 | 15 28 0.52 | –50 41 49.00 | –105.52 | 20.05 | –0.068 | |||||||||||
| TO056 | 15 28 2.62 | –50 39 33.50 | –110.10 | 20.09 | –0.101 | |||||||||||
| TO064 | 15 28 5.51 | –50 39 25.70 | –99.61 | 19.88 | –0.091 | |||||||||||
| TO070 | 15 28 6.40 | –50 39 34.60 | –104.23 | 20.00 | –0.047 | |||||||||||
| TO083 | 15 28 6.97 | –50 41 50.20 | –106.09 | 20.15 | –0.088 | |||||||||||
| TO084 | 15 28 7.43 | –50 41 32.50 | –105.61 | 20.07 | –0.053 | |||||||||||
| TO086 | 15 28 7.93 | –50 41 10.50 | –103.21 | 19.97 | –0.092 | |||||||||||
| TO088 | 15 28 7.43 | –50 42 24.90 | –93.08 | 20.14 | –0.085 | |||||||||||
| TO090 | 15 28 9.62 | –50 40 30.50 | –103.40 | 20.26 | –0.115 | |||||||||||
| TO101 | 15 28 10.67 | –50 40 10.00 | –107.09 | 19.80 | –0.071 | |||||||||||
| TO103 | 15 28 11.03 | –50 39 55.70 | –108.89 | 20.08 | –0.122 | |||||||||||
| TO106 | 15 28 11.14 | –50 40 22.60 | –95.77 | 19.95 | –0.089 | |||||||||||
|
|
||||||||||||||||
| TO020 | 15 27 53.96 | –50 39 24.90 | 13.82 | 19.74 | –0.028 | |||||||||||
| TO042 | 15 27 55.43 | –50 42 8.20 | 15.37 | 20.09 | –0.073 | |||||||||||
| TO058 | 15 28 1.78 | –50 41 56.60 | 9.71 | 19.86 | –0.044 | |||||||||||
| TO078 | 15 28 6.25 | –50 42 6.80 | 32.98 | 20.18 | –0.117 | |||||||||||
Notes. Fibre coordinates are given in columns two and three. Column four contains the heliocentric radial velocity derived from the combined spectrum (see Sect. 4). The last columns contain the in-flight ACS magnitudes (T. Brown, priv. comm.). The first 26 lines contain the stars with a radial velocity that makes them likely members of NGC 5927. The last four entries are the stars that fall more than 3σ outside the mean cluster radial velocity.
Star T051 has no detection in the Brown photometry within 1.5 arcsec. There are two sources within 1.7 arcsec. We cannot unambiguously associate colors from Brown et al. (2005) with our target source.
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