Luo Ding-jiang, Zhu Yuan-xian, Xiao Nai-yuan, Miao Yong-kuan, Lin Zhao-fen
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Abstract
Using the results of our latitude and time programs obtained with the impersonal astrolabe (OPL No. 30) of the Peking Observatory, we have calculated the corrections to individual star positions and the systematic corrections Δαδ and Δδδ to catalogue positions.
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