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Table 2:

Basic data for SGB-a stars studied in this paper.

ID
RA Dec. A(Li) S/N $T_{\rm eff}$(K)
120117 13:27:15.18 -47:29:52.13 <1.50 38 5654
213295 13:26:42.67 -47:32:54.29 <1.42 32 5490
213952 13:26:23.23 -47:32:45.23 <1.23 45 5479
215700 13:26:30.16 -47:32:21.81 <1.33 44 5542
216031 13:26:27.23 -47:32:17.22 <1.00 33 5081
223861 13:26:22.04 -47:30:31.76 <1.36 51 5330
224921 13:27:08.47 -47:30:15.98 <1.39 37 5528
243327 13:26:32.84 -47:26:03.91 <0.92 46 5148
247798 13:26:31.46 -47:25:03.30 <1.30 44 5503
248814 13:27:05.20 -47:24:48.71 <1.28 43 5465

Notes. For each star, we report ID, coordinates, and the derived upper limits to the lithium abundances. The spectra signal-to-noise and the H$_\alpha$-based effective temperatures are also reported. A metallicity of [Fe/H]=-1.5 was assumed.


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