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Table 4

Photometric stellar parameters derived using the calibrations by Alonso et al. (1999) for VI, VK, JK, bolometric corrections computed by adopting the V,I derived temperature, bolometric magnitudes, and corresponding gravity log g, and final spectroscopic parameters.



star T V − I T VK T JK T VK T JK BCV M bol log g T eff BCV log g log g [FeI/H] [FeII/H] [Fe/H] v t
2MASS VVV
(K) (K) (K) (K) (K) (K) km s-1

2115 4196.6 −0.702 −0.18 1.95 4530 0.457 1.99 2.00 0.98 1.02 1.00 1.45
2461 4735.2 4217.9 4506.5 −0.368 −0.14 2.04 4780 0.323 2.04 2.05 1.13 1.09 1.11 1.90
2939 4274.4 4025.1 4423.3 −0.638 −0.12 1.98 4525 0.440 2.01 2.00 1.07 1.07 1.07 1.55
3514 4496.6 4249.4 4624.0 4855.9 −0.487 0.08 2.09 4590 0.349 2.06 2.00 1.18 1.19 1.18 1.90
5037 4481.9 4254.3 4418.0 4324.0 4576.4 −0.496 −0.15 1.99 4570 0.429 2.05 2.15 0.98 1.03 1.0 1.20
5485 4920.4 4499.6 4197.0 4812.7 5152.4 −0.298 0.14 2.08 4920 0.282 2.09 2.07 1.18 1.18 1.18 1.80

Notes. A reddening of E(BV) = 1.12 is assumed. For each star the last columns give the spectroscopic parameters from UVES spectra (present work).

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