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This paper presents rigorous equations, useful with computer reduction of celestial sights, which correct the Greenwich Hour Angle and declination of a celestial body for the motion of a vessel. Advancing a circle of position in this way maintains the relationship between the geographical position of the body and the vessel, and hence is the best method for advancing an observation.
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Stored only when both papers are in the corpus — 5 citations exist upstream.
Papers that cite the same references — the relational fallback while embeddings are still backfilling.
Imported from OpenAlex (CC0) — nothing here is generated.