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Cited article:

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HE 0107−5240, a Chemically Ancient Star. I. A Detailed Abundance Analysis

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Abundances In Very Metal‐Poor Dwarf Stars

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Infrared Properties of a Sub-Sample of Late-Type Stars Provided by the First Byurakan Spectral Sky Survey

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First Byurakan Spectral Sky Survey. Stars of Late-Spectral Types. XIV. Zone +13° ≤ δ ≤ +33°

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Statistical methods of automatic spectral classification and their application to the Hamburg/ESO Survey

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First Byurakan Spectral Sky Survey. Stars of Late-Spectral Types. XIII. Zone +1° ≤ δ ≤ +13°

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