Table C.2.
Properties of observed P69-FORS2 dataset in the Tucana dSph.
Slit | RA, Dec (J2000) | V ± δV | I ± δI | vhel ± δvhel | [Fe/H] ± δ[Fe/H] | S/N | P |
||
---|---|---|---|---|---|---|---|---|---|
[deg] | [km s−1] | [dex] | [pxl−1] | P1 | P2 | P3 | |||
1 | 340.4472, −64.42209 | 22.44 ± 0.02 | 20.97 ± 0.02 | 180.4 ± 4.8 | −1.07 ± 0.17 | 20.4 | 0.99 | 0.99 | 0.99 |
2 | 340.4532, −64.42234 | 22.48 ± 0.02 | 21.26 ± 0.02 | 176.3 ± 6.8 | −1.56 ± 0.29 | 15.0 | 0.99 | 0.99 | 0.99 |
3 | 340.4586, −64.39465 | 22.22 ± 0.02 | 20.96 ± 0.02 | 144.2 ± 5.2 | −1.52 ± 0.22 | 19.8 | 0.17 | 0.01 | 0.02 |
4 | 340.4647, −64.4236 | 22.64 ± 0.01 | 21.22 ± 0.01 | 186.8 ± 7.4 | −1.61 ± 0.16 | 19.4 | 0.99 | 0.99 | 0.99 |
5 (a) | 340.4698, −64.43846 | 23.26 ± 0.03 | 21.50 ± 0.05 | 130.4 ± 10.1 | −1.37 ± 0.20 | 11.9 | 0.13 | 0.04 | 0.04 |
6 | 340.4748, −64.41809 | 22.39 ± 0.01 | 20.87 ± 0.01 | 184.8 ± 4.6 | −1.96 ± 0.10 | 29.8 | 0.99 | 0.99 | 0.99 |
7 | 340.4799, −64.40572 | 22.28 ± 0.02 | 20.85 ± 0.02 | 178.9 ± 4.8 | −1.92 ± 0.17 | 24.5 | 0.99 | 0.99 | 0.99 |
8 | 340.4881, −64.41732 | 22.73 ± 0.03 | 21.19 ± 0.03 | 177.7 ± 6.2 | −1.64 ± 0.13 | 18.9 | 0.99 | 0.99 | 0.99 |
9 (b) | 340.4920, −64.42341 | 22.61 ± 0.02 | 21.35 ± 0.02 | 232.8 ± 8.0 | −1.28 ± 0.22 | 15.4 | Ph | ||
10 | 340.4963, −64.41156 | 22.45 ± 0.02 | 21.01 ± 0.02 | 225.0 ± 7.2 | −2.00 ± 0.18 | 19.8 | Ph | ||
11 | 340.5012, −64.41237 | 22.73 ± 0.01 | 21.49 ± 0.01 | 166.8 ± 5.4 | −1.19 ± 0.35 | 13.0 | 0.99 | 0.99 | 0.99 |
12 | 340.5069, −64.40718 | 22.28 ± 0.02 | 20.86 ± 0.02 | 181.8 ± 8.3 | −1.87 ± 0.18 | 21.8 | 0.99 | 0.99 | 0.99 |
13 | 340.5105, −64.42116 | 22.31 ± 0.02 | 20.83 ± 0.02 | 209.9 ± 7.6 | −1.96 ± 0.16 | 18.3 | 0.99 | 0.96 | 0.96 |
14 | 340.5140, −64.41146 | 22.49 ± 0.03 | 20.96 ± 0.02 | 191.7 ± 5.3 | −1.41 ± 0.14 | 23.9 | 0.99 | 0.99 | 0.99 |
23 (b) | 340.5695, −64.3833 | 22.41 ± 0.03 | 20.65 ± 0.04 | 179.5 ± 5.7 | −1.95 ± 0.16 | 25.2 | 0.79 | ||
24 | 340.5742, −64.37577 | 0.0 ± 0.0 | 0.0 ± 0.0 | 4.2 ± 4.8 | / | 32.8 | 0.00 | 0.00 | 0.00 |
25 (a),(b) | 340.5836, −64.43902 | 22.95 ± 0.02 | 21.46 ± 0.03 | 236.4 ± 14.1 | −2.01 ± 0.26 | 17.4 | 0.63 | ||
31 | 340.3294, −64.4244 | 21.78 ± 0.02 | 20.59 ± 0.02 | 208.6 ± 5.2 | / | 23.5 | Ph | ||
33 (a) | 340.3435, −64.39041 | 22.61 ± 0.02 | 21.33 ± 0.02 | 110.3 ± 14.9 | −2.42 ± 0.28 | 14.6 | 0.00 | 0.00 | 0.00 |
35 | 340.3536, −64.41425 | 22.59 ± 0.02 | 21.0 ± 0.02 | 76.6 ± 7.3 | −1.77 ± 0.15 | 21.4 | 0.00 | 0.00 | 0.00 |
39 (a),(b) | 340.3762, −64.4242 | 22.69 ± 0.02 | 21.38 ± 0.02 | 197.3 ± 8.3 | −2.11 ± 0.21 | 12.9 | 0.99 | ||
40 | 340.3820, −64.45349 | 0.0 ± 0.0 | 0.0 ± 0.0 | 25.6 ± 11.1 | / | 27.0 | 0.00 | 0.00 | 0.00 |
43 (b) | 340.3973, −64.41121 | 22.45 ± 0.02 | 20.98 ± 0.02 | 207.8 ± 7.3 | −1.14 ± 0.17 | 21.3 | Ph | ||
44 | 340.4024, −64.41617 | 22.27 ± 0.02 | 20.77 ± 0.02 | 180.1 ± 5.2 | −2.20 ± 0.12 | 25.7 | 0.99 | 0.99 | 0.99 |
45 | 340.4100, −64.40206 | 22.41 ± 0.02 | 21.03 ± 0.02 | 174.9 ± 5.9 | −2.12 ± 0.15 | 21.3 | 0.99 | 0.99 | 0.99 |
46 (a) | 340.4163, −64.40805 | 21.09 ± 0.01 | 20.36 ± 0.01 | −160.6 ± 4.8 | / | 31.7 | Ph | ||
47 | 340.4206, −64.41588 | 22.68 ± 0.02 | 21.28 ± 0.02 | 195.7 ± 6.0 | −1.33 ± 0.20 | 14.7 | 0.99 | 0.99 | 0.99 |
49 | 340.4348, −64.40812 | 22.37 ± 0.03 | 21.01 ± 0.02 | 172.5 ± 6.8 | −1.97 ± 0.18 | 24.3 | 0.99 | 0.99 | 0.99 |
Notes. Column (1) slit aperture: numbers < 30 indicate observed targets from chip-1, otherwise from chip-2 – numbers counted from bottom to top of the CCD; (2) RA-Dec coordinated in J2000; (3) V band magnitude with error from VLT/FORS2 photometric catalog; (4) I band magnitude with error from same catalog; (5) l.o.s. heliocentric velocity with error; (6) metallicity with error; (7) S/N in pxl−1 (the conversion factor to Å−1 is 1.08); (8) probability of membership according to the best-fitting kinematic model – the three columns indicate the probabilities obtained using the P69 dataset alone (P1), combining with the P91 (P2) and further adding the FLAMES data (P3). In the P columns, stars marked as “Ph” are nonmembers, excluded according to their magnitudes and colors, or because their measurements proved to be unreliable (see Sect. 4 and Appendix A for full description).
New with respect to Fraternali et al. (2009).
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