Table 1.
Observational properties of the late-type sample from the VFTS.
VFTS ID | α | δ | V | I | J | H | Ks | AV | RV (LR02) | Notes |
---|---|---|---|---|---|---|---|---|---|---|
(J2000) | (J2000) | (mag) | (mag) | (mag) | (mag) | (mag) | (mag, r < 1.5′) | (km s−1) | ||
023 | 05 37 16.08 | −69 08 52.86 | 15.63 | 13.44 | 11.814 | 10.814 | 10.484 | 2.42 ± 0.46 | 267.3 ± 2.6 | |
081 | 05 37 35.99 | −69 12 29.93 | 13.71 | 11.69 | 10.279 | 9.363 | 9.067 | 1.96 ± 0.25 | 283.2 ± 2.4 | K4 (GF15) |
198 | 05 37 54.64 | −69 09 03.36 | 14.02 | 11.82 | 10.301 | 9.391 | 9.067 | 1.67 ± 0.52 | 255.0 ± 1.4 | K4.5 Iab (GF15) |
222 | 05 38 00.57 | −69 09 41.64 | 14.86 | 12.93 | 11.456 | 10.588 | 10.312 | 1.40 ± 0.33 | 250.4 ± 1.0 | |
236 | 05 38 06.61 | −69 03 45.25 | 13.80 | 11.90 | 10.536 | 9.677 | 9.413 | 1.14 ± 0.25 | 258.5 ± 0.9 | Hodge 301 candidate |
275 | 05 38 16.00 | −69 10 11.39 | 14.22 | 11.47 | 9.308 | 8.336 | 7.867 | 1.28 ± 0.22 | 286.7 ± 1.0 | M4 (GF15), M1.5 (L07) |
281 | 05 38 16.68 | −69 04 14.09 | 13.99 | 11.38 | 9.786 | 8.906 | 8.552 | 1.14 ± 0.25 | 260.3 ± 1.6 | Hodge 301 member |
289 | 05 38 17.64 | −69 04 12.03 | 13.96 | 12.13 | 10.848 | 10.011 | 9.722 | 1.14 ± 0.25 | 258.1 ± 1.7 | Hodge 301 member |
341 | 05 38 26.69 | −69 08 52.70 | 14.02 | 11.66 | 9.782 | 8.754 | 8.340 | 2.18 ± 0.81 | 278.7 ± 2.9 | K5 (GF15) |
655 | 05 38 51.19 | −69 06 41.29 | 15.13 | 13.02 | 11.497 | 10.598 | 10.260 | 2.00 ± 0.55 | 282.0 ± 0.9 | |
744 | 05 39 07.13 | −69 01 52.77 | 15.63 | 13.23 | 11.688 | 10.668 | 10.363 | 1.92 ± 0.91 | 248.2 ± 3.1 | |
793 | 05 39 28.18 | −69 05 50.49 | 13.58 | 12.33 | 11.422 | 10.735 | 10.616 | 1.75 ± 0.30 | 187.4 ± 1.0 | Foreground, K I (GF15) |
828 | 05 39 39.41 | −69 11 52.05 | 14.52 | 11.60 | 9.864 | 8.965 | 8.524 | 2.50 ± 0.30 | 247.0 ± 1.1 | SL 639 member, M (GF15) |
839 | 05 39 41.78 | −69 11 31.01 | 14.64 | 12.03 | 10.280 | 9.352 | 8.935 | 2.50 ± 0.30 | 248.0 ± 1.2 | SL 639 member |
852 | 05 39 52.39 | −69 09 41.26 | 14.30 | 12.21 | 10.682 | 9.733 | 9.407 | 2.15 ± 0.21 | 243.2 ± 3.0 | SL 639 candidate |
2002 | 05 37 13.50 | −69 08 34.65 | 14.21 | 11.57 | 9.720 | 8.721 | 8.292 | 2.46 ± 0.55 | 284.3 ± 3.4 | M3 (GF15) |
2028 | 05 37 58.67 | −69 14 24.07 | 13.27 | 11.06 | 9.532 | 8.716 | 8.383 | 1.20 ± 0.33 | 274.0 ± 2.5 | G5 Ia (GF15) |
2090 | 05 40 07.01 | −69 11 41.50 | 14.88 | 12.65 | 11.035 | 10.067 | 9.717 | 2.50 ± 0.30 | 247.1 ± 1.0 | SL 639 candidate |
WB97 5 | 05 38 17.01 | −69 04 00.98 | 13.60 | 11.58 | 10.077 | 9.193 | 8.866 | 1.17 ± 0.24 | ... | Hodge 301 member |
Mk 9 | 05 38 48.48 | −69 05 32.58 | 13.62 | 10.86 | 9.173 | 8.297 | 7.869 | 1.92 ± 0.30 | ... | M3.5 Ia (GF15) |
Notes. The final column indicates membership of Hodge 301 or SL 639, and published spectral classifications from González-Fernández et al. (2015; GF15) and Levesque et al. (2007; L07). Radial velocity (RV) estimates are the averages from the VFTS observations with the LR02 setting.
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