Free Access

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).

(a)

New with respect to Fraternali et al. (2009).

(b)

In common with the P91-FORS2 dataset.

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.