Table 1.

Observed stars: the K magnitudes are obtained from 2MASS photometry while I and V are from Kleyna et al. (1998). The preliminary estimates for the photometric temperature T(phot) from (V−I) and the surface gravity are calculated assuming a metallicity of [Fe/H] = −2 dex, mass of 0.8 M and distance of 68 kpc. The T(spec), log g, vmic and [Fe/H] are the values found by iteration of the best atmospheric models used to calculate the spectroscopic abundances (see the text for details).

TargetIVKα J2000δ (J2000)Teff (phot)Teff (spec)log gvmic[Fe/H]vr (km s−1)
UMI71816.3017.4614.96715:02:25.5866:55:25.39456345401.12.25−2.12−247.6
UMI39615.5916.9414.01815:05:52.0466:41:30.05431242900.52.35−2.13−228
UMI44616.9618.0715.13115:02:01.5366:49:22.36464045801.62.80−2.67−246
TargetIVKα J2000δ (J2000)Teff (phot)Teff (spec)log gvmic[Fe/H]vr (km s−1)
UMI71816.3017.4614.96715:02:25.5866:55:25.39456345401.12.25−2.12−247.6
UMI39615.5916.9414.01815:05:52.0466:41:30.05431242900.52.35−2.13−228
UMI44616.9618.0715.13115:02:01.5366:49:22.36464045801.62.80−2.67−246
Table 1.

Observed stars: the K magnitudes are obtained from 2MASS photometry while I and V are from Kleyna et al. (1998). The preliminary estimates for the photometric temperature T(phot) from (V−I) and the surface gravity are calculated assuming a metallicity of [Fe/H] = −2 dex, mass of 0.8 M and distance of 68 kpc. The T(spec), log g, vmic and [Fe/H] are the values found by iteration of the best atmospheric models used to calculate the spectroscopic abundances (see the text for details).

TargetIVKα J2000δ (J2000)Teff (phot)Teff (spec)log gvmic[Fe/H]vr (km s−1)
UMI71816.3017.4614.96715:02:25.5866:55:25.39456345401.12.25−2.12−247.6
UMI39615.5916.9414.01815:05:52.0466:41:30.05431242900.52.35−2.13−228
UMI44616.9618.0715.13115:02:01.5366:49:22.36464045801.62.80−2.67−246
TargetIVKα J2000δ (J2000)Teff (phot)Teff (spec)log gvmic[Fe/H]vr (km s−1)
UMI71816.3017.4614.96715:02:25.5866:55:25.39456345401.12.25−2.12−247.6
UMI39615.5916.9414.01815:05:52.0466:41:30.05431242900.52.35−2.13−228
UMI44616.9618.0715.13115:02:01.5366:49:22.36464045801.62.80−2.67−246
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