Abstract:Abstract. The programme contains 445 subdwarfs, metal-deficient giants, RHB and CH stars. The aim of the programme is to obtain very accurate trigonometric parallaxes (±0."002-^±0."004) and proper motions (±0."002-j-±0."004/year) for these stars, to significantly improve the determination of their positions in t lie HR diagram and to calculate accurate kinematical parameters. About half of the programme stars are measured in the Vilnius photometric system. For all stars, the colour indices B-V have been compil… Show more
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