An Astrometric Study of Procyon

By G. Gatewood, I. Han. 2006

210 citations recorded by the source corpus.

Subfields: Astronomy and Astrophysics

View Paper: https://www.semanticscholar.org/paper/a4ab3bbef16691596ca87c24507d38e15f39b649

How researchers see this paper

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In Astronomy and Astrophysics

1. T. Bedding
2. M. Endl
3. C. Soubiran
4. F. Th'evenin
5. Paulina Jofré
6. A. Korn
7. P. Quirion
8. D. Paulson

Citations in the corpus

• Gaia FGK benchmark stars: Effective temperatures and surface gravities (2015, background): “The mass of Procyon was determined by Girard et al. (2000) and Gatewood & Han (2006) from astrometric measurements of the 40-year orbit with its white-dwarf companion.”
• The Extrasolar Planet ϵ Eridani b: Orbit and Mass (2006, methodology): “MAP observations of the brightest stars use either a specially filtered 12th channel (e.g., Gatewood & Han 2006) or a divideby-16 feature on channel 2, which reduces the count sufficiently for the 16 bit counters.”
• Accurate fundamental parameters for 23 bright solar-type stars (2010, background): “This is possible for four of the stars in our sample: Procyon A (Girard et al. 2000; Gatewood & Han 2006),α Cen A and B (Pourbaix et al. 2002), and 70 Oph A (Eggenberger et al. 2008).”