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Article Dans Une Revue Memorie della Societa astronomica italiana Année : 2006

Infrared surface brightness distances to Cepheids: a comparison of Bayesian and linear-bisector calculations.

Thomas G. Barnes
  • Fonction : Auteur
Jesper Storm
William H. Jefferys
  • Fonction : Auteur
Wolfgang P. Gieren
  • Fonction : Auteur

Résumé

Bayesian statistical calculations and linear-bisector calculations for obtaining Cepheid distances and radii by the infrared surface brightness method have been compared for a set of 38 Cepheids. The distances obtained by the two techniques agree to 1.5% ± 0.6% and the radii agree to 1.1% ± 0.7%. Thus the two methods yield the same distances and radii at the 2sigma level. This implies that the short distance to the LMC found in recent linear-bisector studies of Cepheids is not a result of simplifications in the mathematical approach. The computed uncertainties in distance and radius are larger in the Bayesian calculation typically by a factor of three.

Dates et versions

hal-00285432 , version 1 (05-06-2008)

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Citer

Thomas G. Barnes, Jesper Storm, William H. Jefferys, Wolfgang P. Gieren, Pascal Fouqué. Infrared surface brightness distances to Cepheids: a comparison of Bayesian and linear-bisector calculations.. Memorie della Societa astronomica italiana, 2006, 77, pp.194. ⟨hal-00285432⟩
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